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Station Nation: Meet Nick Kopp, SpaceX Dragon Flight Lead
Nick Kopp is a Dragon flight lead in the Transportation Integration Office at Johnson Space Center in Houston. He is currently leading NASA’s efforts to prepare, launch, and return the agency’s 32nd SpaceX commercial resupply services mission. He works directly with SpaceX and collaborates with NASA’s many internal, external, and international partners to ensure the success of this and other cargo missions to the International Space Station.
Read on to learn about his career with NASA and more!
Nick Kopp’s official portrait.NASA/Bill Stafford The time and effort spent building, maintaining, and conducting science on the International Space Station is spent by people in our community and communities around the world to further humanity's collective understanding of the universe around us.Nick Kopp
Transportation Integration Office Flight Lead
Where are you from?
I am from Cleveland, Ohio.
Tell us about your role at NASA.
I work directly with SpaceX to ensure the Dragon cargo spacecraft meets NASA’s requirements to visit the space station. I also collaborate with NASA’s various partners who are safely flying science investigations and other cargo to and from the space station. For the upcoming flight, I’ve worked extensively with SpaceX to prepare to return the Dragon cargo spacecraft off the coast of California.
How would you describe your job to family or friends who may not be familiar with NASA?
I’m responsible for getting stuff to and from the International Space Station safely.
How long have you been working for NASA?
I have been working for NASA for about 15 years at both Marshall Space Flight Center in Alabama and Johnson Space Center in Texas.
What advice would you give to young individuals aspiring to work in the space industry or at NASA?
It takes so many different people with all kinds of different skills working together to make missions happen. I would suggest looking at NASA’s websites to find the skill or task that makes you want to learn more and then focusing your energy into that skill. Surround yourself with people with similar goals. Connect with people in the industry and ask them questions. You are in control of your destiny!
Nick Kopp in front of the International Space Station Payload Operations Center at the agency’s Marshall Space Flight Center in Huntsville, Alabama.What was your path to NASA?
I’ve wanted to work at NASA since I was a kid and my grandfather showed me the Moon through his home-built telescope. I studied aerospace engineering at the University of Illinois, where I joined Students for the Exploration and Development of Space and attended a conference at NASA’s Goddard Space Flight Center in Maryland. I met some folks from the Payload Operations Integration Center and learned of the awesome space station science operations at Marshall. I was lucky enough to be chosen for a contractor job working directly with astronauts on the space station to conduct science experiments!
Is there someone in the space, aerospace, or science industry that has motivated or inspired you to work for the space program? Or someone you discovered while working for NASA who inspires you?
After working with him from the ground when he was aboard the space station, I was lucky enough to spend many overnight shifts getting to know NASA astronaut and Flight Director TJ Creamer. TJ’s path to NASA and his servant leadership have left an ongoing legacy for people at the agency. His general attitude, extreme competence, friendly demeanor, and genuine care for people around him continue to inspire me every day to become a great leader.
What is your favorite NASA memory?
My favorite NASA memory is being selected as a payload operations director on the International Space Station Payload Operations and Integration Center flight control team. I looked up to those in this position for 10 years and did everything I could to gather the skills and knowledge I needed to take on the role. I became responsible for the minute-to-minute operations of astronauts conducting science investigations on the space station. I vividly remember the joy I felt learning of the news of my assignment, taking my first shift, my first conversation with an astronaut in space, and the bittersweet decision to leave and continue my career goals at NASA in a different role.
Nick Kopp, right, behind a console in the International Space Station Payload Operations Integration Center at the agency’s Marshall Space Flight Center.What do you love sharing about station? What’s important to get across to general audiences to help them understand the benefits to life on Earth?
Although it takes place off the planet, research on the space station is conducted for people on Earth. The time and effort spent building, maintaining, and conducting science on the International Space Station is spent by people in our community and communities around the world to further humanity’s collective understanding of the universe around us. When we understand more about science, we can be more successful. So many people around the planet have had life-changing benefits from experiments that can only be done by people conducting research in microgravity, above the atmosphere, where you can view most of Earth.
If you could have dinner with any astronaut, past or present, who would it be?
I would have dinner with anyone from the Apollo 13 crew. I’d love to learn how they felt that NASA’s culture drove the outcome of that mission.
Do you have a favorite space-related memory or moment that stands out to you?
While working a night shift at the operations center in Huntsville, Alabama, we were monitoring payloads returning to Earth on a Dragon cargo spacecraft. We took a quick break outside the control center to watch as the spacecraft re-entered Earth’s atmosphere above us on its way to splash down off the coast of Florida. It was a clear night. As the spacecraft flew overhead, we saw the ablative heat shield create a shimmering trail of fire and sparkles that stretched across the whole night sky. It looked as though Tinker Bell just flew over us!
What are some of the key projects you’ve worked on during your time at NASA? What have been your favorite?
Some of my favorite projects I’ve worked on include:
- Serving as the International Space Station Program’s representative as flight lead for NASA’s SpaceX Crew-8 mission
- Troubleshooting unexpected results when conducting science on the space station
- Writing instructions for astronauts filming a virtual reality documentary on the space station
- Assessing design changes on the Space Launch System rocket’s core stage
- Managing and training a team of flight controllers
- Helping NASA move Dragon spacecraft returns from Florida to California
What are your hobbies/things you enjoy outside of work?
I love playing board games with my wife, sailing, flying, traveling around the world, and learning about leadership and project management theory.
Day launch or night launch?
The Crew-8 night launch, specifically, where the Falcon 9 booster landed just above me!
Favorite space movie?
Spaceballs
NASA “worm” or “meatball” logo?
Meatball
Every day, we’re conducting exciting research aboard our orbiting laboratory that will help us explore further into space and bring benefits back to people on Earth. You can keep up with the latest news, videos, and pictures about space station science on the Station Research & Technology news page. It’s a curated hub of space station research digital media from Johnson and other centers and space agencies.
Sign up for our weekly email newsletter to get the updates delivered directly to you.
Follow updates on social media at @ISS_Research on Twitter, and on the space station accounts on Facebook and Instagram.
NASA’s Perseverance Mars Rover Studies Trove of Rocks on Crater Rim
6 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) This mosaic showing the Martian surface outside of Jezero Crater was taken by NASA’s Perseverance on Dec. 25, 2024, at the site where the rover cored a sample dubbed “Silver Mountain” from a rock likely formed during Mars’ earliest geologic period.NASA/JPL-Caltech/ASU/MSSSThe diversity of rock types along the rim of Jezero Crater offers a wide glimpse of Martian history.
Scientists with NASA’s Perseverance rover are exploring what they consider a veritable Martian cornucopia full of intriguing rocky outcrops on the rim of Jezero Crater. Studying rocks, boulders, and outcrops helps scientists understand the planet’s history, evolution, and potential for past or present habitability. Since January, the rover has cored five rocks on the rim, sealing samples from three of them in sample tubes. It’s also performed up-close analysis of seven rocks and analyzed another 83 from afar by zapping them with a laser. This is the mission’s fastest science-collection tempo since the rover landed on the Red Planet more than four years ago.
Perseverance climbed the western wall of Jezero Crater for 3½ months, reaching the rim on Dec. 12, 2024, and is currently exploring a roughly 445-foot-tall (135-meter-tall) slope the science team calls “Witch Hazel Hill.” The diversity of rocks they have found there has gone beyond their expectations.
“During previous science campaigns in Jezero, it could take several months to find a rock that was significantly different from the last rock we sampled and scientifically unique enough for sampling,” said Perseverance’s project scientist, Katie Stack Morgan of NASA’s Jet Propulsion Laboratory in Southern California. “But up here on the crater rim, there are new and intriguing rocks everywhere the rover turns. It has been all we had hoped for and more.”
One of Perseverance’s hazard cameras captured the rover’s coring drill collecting the “Main River” rock sample on “Witch Hazel Hill” on March 10, 2025, the 1,441st Martian day, or sol, of the mission. NASA/JPL-CaltechThat’s because Jezero Crater’s western rim contains tons of fragmented once-molten rocks that were knocked out of their subterranean home billions of years ago by one or more meteor impacts, including possibly the one that produced Jezero Crater. Perseverance is finding these formerly underground boulders juxtaposed with well-preserved layered rocks that were “born” billions of years ago on what would become the crater’s rim. And just a short drive away is a boulder showing signs that it was modified by water nestled beside one that saw little water in its past.
Oldest Sample Yet?Perseverance collected its first crater-rim rock sample, named “Silver Mountain,” on Jan. 28. (NASA scientists informally nickname Martian features, including rocks and, separately, rock samples, to help keep track of them.) The rock it came from, called “Shallow Bay,” most likely formed at least 3.9 billion years ago during Mars’ earliest geologic period, the Noachian, and it may have been broken up and recrystallized during an ancient meteor impact.
About 360 feet (110 meters) away from that sampling site is an outcrop that caught the science team’s eye because it contains igneous minerals crystallized from magma deep in the Martian crust. (Igneous rocks can form deep underground from magma or from volcanic activity at the surface, and they are excellent record-keepers — particularly because mineral crystals within them preserve details about the precise moment they formed.) But after two coring attempts (on Feb. 4 and Feb. 8) fizzled due to the rock being so crumbly, the rover drove about 520 feet (160 meters) northwest to another scientifically intriguing rock, dubbed “Tablelands.”
Data from the rover’s instruments indicates that Tablelands is made almost entirely of serpentine minerals, which form when large amounts of water react with iron- and magnesium-bearing minerals in igneous rock. During this process, called serpentinization, the rock’s original structure and mineralogy change, often causing it to expand and fracture. Byproducts of the process sometimes include hydrogen gas, which can lead to the generation of methane in the presence of carbon dioxide. On Earth, such rocks can support microbial communities.
Coring Tablelands went smoothly. But sealing it became an engineering challenge.
Sealing the “Green Gardens” sample — collected by NASA’s Perseverance Mars rover from a rock dubbed “Tablelands” along the rim of Jezero Crater on Feb. 16, 2025 — presented an engineering challenge. The sample was finally sealed on March 2.NASA/JPL-Caltech/ASU/MSSS Flick Maneuver“This happened once before, when there was enough powdered rock at the top of the tube that it interfered with getting a perfect seal,” said Kyle Kaplan, a robotics engineer at JPL. “For Tablelands, we pulled out all the stops. Over 13 sols,” or Martian days, “we used a tool to brush out the top of the tube 33 times and made eight sealing attempts. We even flicked it a second time.”
During a flick maneuver, the sample handling arm — a little robotic arm in the rover’s belly — presses the tube against a wall inside the rover, then pulls the tube away, causing it to vibrate. On March 2, the combination of flicks and brushings cleaned the tube’s top opening enough for Perseverance to seal and store the serpentine-laden rock sample.
Eight days later, the rover had no issues sealing its third rim sample, from a rock called “Main River.” The alternating bright and dark bands on the rock were like nothing the science team had seen before.
Up NextFollowing the collection of the Main River sample, the rover has continued exploring Witch Hazel Hill, analyzing three more rocky outcrops (“Sally’s Cove,” “Dennis Pond,” and “Mount Pearl”). And the team isn’t done yet.
“The last four months have been a whirlwind for the science team, and we still feel that Witch Hazel Hill has more to tell us,” said Stack. “We’ll use all the rover data gathered recently to decide if and where to collect the next sample from the crater rim. Crater rims — you gotta love ’em.”
More About PerseveranceA key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover is characterizing the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet and is the first mission to collect and cache Martian rock and regolith.
NASA’s Mars Sample Return Program, in cooperation with ESA (European Space Agency), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.
The Mars 2020 Perseverance mission is part of NASA’s Mars Exploration Program portfolio and the agency’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.
NASA’s Jet Propulsion Laboratory, managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.
For more about Perseverance:
https://science.nasa.gov/mission/mars-2020-perseverance
Meet the Mars Samples: Sapphire Canyon (Sample 25) News Media ContactsDC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
2025-051
Share Details Last Updated Apr 10, 2025 Related Terms Explore More 5 min read Perseverance Rover Witnesses One Martian Dust Devil Eating Another Article 1 week ago 6 min read How NASA’s Perseverance Is Helping Prepare Astronauts for Mars Article 2 weeks ago 6 min read NASA’s Curiosity Rover Detects Largest Organic Molecules Found on MarsLee esta historia en español aquí. Researchers analyzing pulverized rock onboard NASA’s Curiosity rover have found…
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NASA’s SpaceX 32nd Resupply Mission Launches New Research to Station
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Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA and SpaceX are launching the company’s 32nd commercial resupply services mission to the International Space Station later this month, bringing a host of new research to the orbiting laboratory. Aboard the SpaceX Dragon spacecraft are experiments focused on vision-based navigation, spacecraft air quality, materials for drug and product manufacturing, and advancing plant growth with less reliance on photosynthesis.
This and other research conducted aboard the space station advances future space exploration, including missions to the Moon and Mars, and provides many benefits to humanity.
Investigations traveling to the space station include:
Robotic spacecraft guidanceSmartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a vision-based sensor developed by NASA to control a formation flight of small satellites. Based on a previous in-space demonstration of the technology, this investigation is designed to refine the maneuvers of multiple robots and integrate the information with spacecraft systems.
Potential benefits of this technology include improved accuracy and reliability of systems for guidance, navigation, and control that could be applied to docking crewed spacecraft in orbit and remotely operating multiple robots on the lunar or Martian surface.
Two of the space station’s Astrobee robots are used to test a vision-based guidance system for Smartphone Video Guidance Sensor (SVGS)NASA Protection from particlesDuring spaceflight, especially long-duration missions, concentrations of airborne particles must be kept within ranges safe for crew health and hardware performance. The Aerosol Monitors investigation tests three different air quality monitors in space to determine which is best suited to protect crew health and ensure mission success. The investigation also tests a device for distinguishing between smoke and dust. Aboard the space station, the presence of dust can cause false smoke alarms that require crew member response. Reducing false alarms could save valuable crew time while continuing to protect astronaut safety.
Better materials, better drugsThe DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials. It also evaluates how well the materials reduce joint inflammation and whether they can help regenerate cartilage lost due to arthritis. These materials are less toxic, more stable, and more compatible with living tissues than current drug delivery technologies.
Environmental influences such as gravity can affect the quality of these materials and delivery systems. In microgravity, they are larger and have greater uniformity and structural integrity. This investigation could help identify the best formulations and methods for cost-effective in-space production. These nanomaterials also could be used to create novel systems targeting therapy delivery that improves patient outcomes with fewer side effects.
Stem cells grown along the Janus base nanomaterials (JBNs) made aboard the International Space Station.University of Connecticut Next-generation pharmaceutical nanostructuresThe newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility. The cassette can process more sample types, including tiny gold particles used in devices that detect cancer and other diseases or in targeted drug delivery systems. Microgravity makes it possible to produce larger and more uniform gold particles, which improves their use in research and real-life applications of technologies related to human health.
Helping plants growRhodium USAFA NIGHT examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis. Because photosynthesis needs light, which requires spacecraft power to generate, alternatives would reduce energy use. The investigation also examines whether using supplements increases plant growth on the space station, which has been observed in preflight testing on Earth. In future plant production facilities aboard spacecraft or on celestial bodies, supplements could come from available organic materials such as waste.
Understanding how plants adapt to microgravity could help grow food during long-duration space missions or harsh environments on Earth.
Hardware for the Rhodium Plant LIFE, which was the first in a series used to study how space affects plant growth.NASA Atomic clocks in spaceAn ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity. Results have applications to scientific measurement studies, the search for dark matter, and fundamental physics research that relies on highly accurate atomic clocks in space. The experiment also tests a technology for synchronizing clocks worldwide using global navigation satellite networks.
An artist’s concept shows the Atomic Clock Ensemble in Space hardware mounted on the Earth-facing side of the space station’s exterior.ESADownload high-resolution photos and videos of the research mentioned in this article.
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NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise
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NASA, ESA, CSA, R. Crawford (STScI)
Observations from NASA’s James Webb Space Telescope have provided a surprising twist in the narrative surrounding what is believed to be the first star observed in the act of swallowing a planet. The new findings suggest that the star actually did not swell to envelop a planet as previously hypothesized. Instead, Webb’s observations show the planet’s orbit shrank over time, slowly bringing the planet closer to its demise until it was engulfed in full.
“Because this is such a novel event, we didn’t quite know what to expect when we decided to point this telescope in its direction,” said Ryan Lau, lead author of the new paper and astronomer at NSF NOIRLab (National Science Foundation National Optical-Infrared Astronomy Research Laboratory) in Tucson, Arizona. “With its high-resolution look in the infrared, we are learning valuable insights about the final fates of planetary systems, possibly including our own.”
Two instruments aboard Webb conducted the post-mortem of the scene – Webb’s MIRI (Mid-Infrared Instrument) and NIRSpec (Near-Infrared Spectrograph). The researchers were able to come to their conclusion using a two-pronged investigative approach.
Image A: Planetary Engulfment Illustration NASA’s James Webb Space Telescope’s observations of what is thought to be the first-ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly depreciated over time, as seen in this artist’s concept. NASA, ESA, CSA, R. Crawford (STScI) Constraining the HowThe star at the center of this scene is located in the Milky Way galaxy about 12,000 light-years away from Earth.
The brightening event, formally called ZTF SLRN-2020, was originally spotted as a flash of optical light using the Zwicky Transient Facility at Caltech’s Palomar Observatory in San Diego, California. Data from NASA’s NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) showed the star actually brightened in the infrared a year before the optical light flash, hinting at the presence of dust. This initial 2023 investigation led researchers to believe that the star was more Sun-like, and had been in the process of aging into a red giant over hundreds of thousands of years, slowly expanding as it exhausted its hydrogen fuel.
However, Webb’s MIRI told a different story. With powerful sensitivity and spatial resolution, Webb was able to precisely measure the hidden emission from the star and its immediate surroundings, which lie in a very crowded region of space. The researchers found the star was not as bright as it should have been if it had evolved into a red giant, indicating there was no swelling to engulf the planet as once thought.
Reconstructing the SceneResearchers suggest that, at one point, the planet was about Jupiter-sized, but orbited quite close to the star, even closer than Mercury’s orbit around our Sun. Over millions of years, the planet orbited closer and closer to the star, leading to the catastrophic consequence.
“The planet eventually started to graze the star’s atmosphere. Then it was a runaway process of falling in faster from that moment,” said team member Morgan MacLeod of the Harvard-Smithsonian Center for Astrophysics and the Massachusetts Institute of Technology in Cambridge, Massachusetts. “The planet, as it’s falling in, started to sort of smear around the star.”
In its final splashdown, the planet would have blasted gas away from the outer layers of the star. As it expanded and cooled off, the heavy elements in this gas condensed into cold dust over the next year.
Inspecting the LeftoversWhile the researchers did expect an expanding cloud of cooler dust around the star, a look with the powerful NIRSpec revealed a hot circumstellar disk of molecular gas closer in. Furthermore, Webb’s high spectral resolution was able to detect certain molecules in this accretion disk, including carbon monoxide.
“With such a transformative telescope like Webb, it was hard for me to have any expectations of what we’d find in the immediate surroundings of the star,” said Colette Salyk of Vassar College in Poughkeepsie, New York, an exoplanet researcher and co-author on the new paper. “I will say, I could not have expected seeing what has the characteristics of a planet-forming region, even though planets are not forming here, in the aftermath of an engulfment.”
The ability to characterize this gas opens more questions for researchers about what actually happened once the planet was fully swallowed by the star.
“This is truly the precipice of studying these events. This is the only one we’ve observed in action, and this is the best detection of the aftermath after things have settled back down,” Lau said. “We hope this is just the start of our sample.”
These observations, taken under Guaranteed Time Observation program 1240, which was specifically designed to investigate a family of mysterious, sudden, infrared brightening events, were among the first Target of Opportunity programs performed by Webb. These types of study are reserved for events, like supernova explosions, that are expected to occur, but researchers don’t exactly know when or where. NASA’s space telescopes are part of a growing, international network that stands ready to witness these fleeting changes, to help us understand how the universe works.
Researchers expect to add to their sample and identify future events like this using the upcoming Vera C. Rubin Observatory and NASA’s Nancy Grace Roman Space Telescope, which will survey large areas of the sky repeatedly to look for changes over time.
The team’s findings appear today in The Astrophysical Journal.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
To learn more about Webb, visit: https://science.nasa.gov/webb
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View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
View/Download the science paper from the The Astrophysical Journal.
Media ContactsLaura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hannah Braun – hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Read more about Webb’s impact on exoplanet research
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NASA Offers Free High School Engineering Program This Summer
NASA’s Glenn Research Center in Cleveland is launching the NASA Glenn High School Engineering Institute this summer. The free, work-based learning experience is designed to help high school students prepare for a future in the aerospace workforce.
Rising high school juniors and seniors in Northeast Ohio can submit applications for this new, in-person summer program from Friday, April 11, through Friday, May 9.
The NASA Glenn High School Engineering Institute will immerse students in NASA’s work while providing essential career readiness tools to help them in future science, technology, engineering, and mathematics-focused academic and professional pursuits.
Throughout the five-day institute, students will use authentic NASA mission content and work alongside Glenn’s technical experts to gain a deeper understanding of the engineering design process, develop practical engineering solutions to real-world challenges, and test prototypes to answer questions in key mission areas:
- Acoustic dampening – How can we reduce noise pollution from jet engines?
- Power management and distribution – How can we develop a smart power system for future space stations?
- Simulated lunar operations – Can we invent tires that don’t use air?
Program Dates
Selected students will participate in one of the following week-long sessions.
- Session 1: July 7 – 11, 2025
- Session 2: July 14 – 18, 2025
- Session 3: July 21 – 25, 2025
Eligibility and Application Requirements
To be eligible for this program, students must:
- Be entering 11th or 12th grade for the 2025-2026 academic year
- Have a minimum 3.2 GPA, verified by their school counselor
- Submit a letter of recommendation from a teacher
Additional application requirements are outlined in the Supplemental Application.
How to Apply:
To be considered for this opportunity, complete and submit the NASA Gateway application and the Supplemental Application by Friday May 9.
Questions pertaining to the NASA Glenn High School Engineering Institute should be directed to Gerald Voltz at GRC-Ed-Opportunities@mail.nasa.gov.
For information about NASA Glenn, visit:
-end-
Debbie Welch
Glenn Research Center, Cleveland
216-433-8655
debbie.welch@nasa.gov
Data – and our ability to understand and use it – shapes nearly every aspect…
Article 1 day ago 3 min read University High Triumphs at JPL-Hosted Ocean Sciences Bowl Article 1 week ago 2 min read Students Explore Technical Careers at NASA Article 3 weeks agoNASA’s Juno Back to Normal Operations After Entering Safe Mode
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NASA’s Juno Back to Normal Operations After Entering Safe Mode NASA’s Juno flies above Jupiter’s Great Red Spot in this artist’s concept. NASA/JPL-CaltechThe spacecraft was making its 71st close approach to Jupiter when it unexpectedly entered into a precautionary status.
Data received from NASA’s Juno mission indicates the solar-powered spacecraft went into safe mode twice on April 4 while the spacecraft was flying by Jupiter. Safe mode is a precautionary status that a spacecraft enters when it detects an anomaly. Nonessential functions are suspended, and the spacecraft focuses on essential tasks like communication and power management. Upon entering safe mode, Juno’s science instruments were powered down, as designed, for the remainder of the flyby.
The mission operations team has reestablished high-rate data transmission with Juno, and the spacecraft is currently conducting flight software diagnostics.The team will work in the ensuing days to transmit the engineering and science data collected before and after the safe-mode events to Earth.
Juno first entered safe mode at 5:17 a.m. EDT, about an hour before its 71st close passage of Jupiter — called perijove. It went into safe mode again 45 minutes after perijove. During both safe-mode events, the spacecraft performed exactly as designed, rebooting its computer, turning off nonessential functions, and pointing its antenna toward Earth for communication.
Of all the planets in our solar system, Jupiter is home to the most hostile environment, with the radiation belts closest to the planet being the most intense. Early indications suggest the two Perijove 71 safe-mode events occurred as the spacecraft flew through these belts. To block high-energy particles from impacting sensitive electronics and mitigate the harmful effects of the radiation, Juno features a titanium radiation vault.
Including the Perijove 71 events, Juno has unexpectedly entered spacecraft-induced safe mode four times since arriving at Jupiter in July 2016: first, in 2016 during its second orbit, then in 2022 during its 39th orbit. In all four cases, the spacecraft performed as expected and recovered full capability.
Juno’s next perijove will occur on May 7 and include a flyby of the Jovian moon Io at a distance of about 55,300 miles (89,000 kilometers).
More About JunoNASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. The Italian Space Agency (ASI) funded the Jovian InfraRed Auroral Mapper. Lockheed Martin Space in Denver built and operates the spacecraft. Various other institutions around the U.S. provided several of the other scientific instruments on Juno.
More information about Juno is available at:
News Media ContactsDC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
Deb Schmid
Southwest Research Institute, San Antonio
210-522-2254
dschmid@swri.org
2025-049
Share Details Last Updated Apr 09, 2025 Related Terms Explore More 2 min read For Your Processing Pleasure: The Sharpest Pictures of Jupiter’s Volcanic Moon Io in a GenerationArticle
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Hubble Helps Determine Uranus’ Rotation Rate with Unprecedented Precision
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ESA/Hubble, NASA, L. Lamy, L. Sromovsky
An international team of astronomers using the NASA/ESA Hubble Space Telescope has made new measurements of Uranus’ interior rotation rate with a novel technique, achieving a level of accuracy 1,000 times greater than previous estimates. By analyzing more than a decade of Hubble observations of Uranus’ aurorae, researchers have refined the planet’s rotation period and established a crucial new reference point for future planetary research.
These images from the NASA/ESA Hubble Space Telescope showcase the dynamic aurora on Uranus in October 2022. These observations were made by the Space Telescope Imaging Spectrograph (STIS) and includes both visible and ultraviolet data. An international team of astronomers used Hubble to make new measurements of Uranus’ interior rotation rate by analyzing more than a decade of the telescope’s observations of Uranus’ aurorae. This refinement of the planet’s rotation period achieved a level of accuracy 1000 times greater than previous estimates and serves as a crucial new reference point for future planetary research. ESA/Hubble, NASA, L. Lamy, L. SromovskyDetermining a planet’s interior rotation rate is challenging, particularly for a world like Uranus, where direct measurements are not possible. A team led by Laurent Lamy (of LIRA, Observatoire de Paris-PSL and LAM, Aix-Marseille Univ., France), developed an innovative method to track the rotational motion of Uranus’ aurorae: spectacular light displays generated in the upper atmosphere by the influx of energetic particles near the planet’s magnetic poles. This technique revealed that Uranus completes a full rotation in 17 hours, 14 minutes, and 52 seconds — 28 seconds longer than the estimate obtained by NASA’s Voyager 2 during its 1986 flyby.
“Our measurement not only provides an essential reference for the planetary science community but also resolves a long-standing issue: previous coordinate systems based on outdated rotation periods quickly became inaccurate, making it impossible to track Uranus’ magnetic poles over time,” explains Lamy. “With this new longitude system, we can now compare auroral observations spanning nearly 40 years and even plan for the upcoming Uranus mission.”
This image of Uranus’ aurorae was taken by the NASA/ESA Hubble Space Telescope on 10 October 2022. These observations were made by the Space Telescope Imaging Spectrograph (STIS) and includes both visible and ultraviolet data. An international team of astronomers used Hubble to make new measurements of Uranus’ interior rotation rate by analyzing more than a decade of the telescope’s observations of Uranus’ aurorae. This refinement of the planet’s rotation period achieved a level of accuracy 1000 times greater than previous estimates and serves as a crucial new reference point for future planetary research. ESA/Hubble, NASA, L. Lamy, L. SromovskyThis breakthrough was possible thanks to Hubble’s long-term monitoring of Uranus. Over more than a decade, Hubble has regularly observed its ultraviolet auroral emissions, enabling researchers to produce magnetic field models that successfully match the changing position of the magnetic poles with time.
“The continuous observations from Hubble were crucial,” says Lamy. “Without this wealth of data, it would have been impossible to detect the periodic signal with the level of accuracy we achieved.”
Unlike the aurorae of Earth, Jupiter, or Saturn, Uranus’ aurorae behave in a unique and unpredictable manner. This is due to the planet’s highly tilted magnetic field, which is significantly offset from its rotational axis. The findings not only help astronomers understand Uranus’ magnetosphere but also provide vital information for future missions.
These findings set the stage for further studies that will deepen our understanding of one of the most mysterious planets in the Solar System. With its ability to monitor celestial bodies over decades, the Hubble Space Telescope continues to be an indispensable tool for planetary science, paving the way for the next era of exploration at Uranus.
These results are based on observations acquired with Hubble programs GO #12601, 13012, 14036, 16313 and DDT #15380 (PI: L. Lamy). The team’s paper was published in Nature Astronomy.
The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Related Images & Videos Uranus Aurorae Image Trio (October 2022)
Close-up: Uranus Aurorae (October 2022)
Claire Andreoli
Astrophysics Communications Manager
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
Bethany Downer
ESA/Hubble Chief Science Communications Officer
Bethany.Downer@esahubble.org
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Expedition 73 Crew Launches to International Space Station
A Soyuz rocket launches to the International Space Station with Expedition 73 crew members including NASA astronaut Jonny Kim on Tuesday, April 8, 2025, at the Baikonur Cosmodrome in Kazakhstan.
The crew arrived at the space station the same day, bringing the number of residents to 10 for the next two weeks. Expedition 73 will begin on Saturday, April 19, following the departure of NASA astronaut Don Pettit and Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner, as they conclude a seven-month science mission aboard the orbiting laboratory.
Throughout his eight-month stay aboard the orbital outpost, Kim will conduct scientific research in technology development, Earth science, biology, and human research.
Follow space station activities on the International Space Station blog.
Image credit: NASA/Joel Kowsky
NASA Science Supports Data Literacy for K-12 Students
3 min read
NASA Science Supports Data Literacy for K-12 StudentsData – and our ability to understand and use it – shapes nearly every aspect of our world, from decisions in our lives to the skills we need in the workplace and more. All of us, as either producers or consumers of data, will experience how it can be used to problem-solve and think critically as we navigate the world around us. For that reason, Data Science has become an increasingly essential and growing field that combines the collection, organization, analysis, interpretation, and sharing of data in virtually every area of life. As more data become more openly available, our Data Science skills will be of increasing importance. And yet, there is a widening gap between what students learn in school and the skills they will need to succeed in a data-driven world. The integration of Data Science into K-12 education opens doors to higher education, high-paying careers, and empowering learners to eventually participate in the creation of new knowledge and understanding of our world, and at least 29 states have reported some level of data science implementation at the K-12 level, including standard or framework adoption, course piloting, and educator professional learning.
In February 2025, the first-ever Data Science Education K-12: Research to Practice Conference (DS4E) took place in San Antonio, TX. A number of representatives from NASA’s Science Activation program and other NASA partners attended and presented along with over 250 educators, researchers, and school leaders from across the nation. Science Activation projects share a passion for helping people of all ages and backgrounds connect with NASA science experts, content, experiences, and learning resources, and the AEROKATS & ROVER Education Network (AREN); Place-Based Learning to Advance Connections, Education, and Stewardship (PLACES); Global Learning and Observations to Benefit the Environment (GLOBE) Mission Earth; and My NASA Data teams did just that. Their presentations at the conference included:
- “BYOD – Build or Bring Your Own Data: Developing K-12 Datasets” (PLACES)
- “Using NASA Data Resources as a Tool to Support Storytelling with Data in K-12 Education” (My NASA Data)
- “Place-Based Data Literacy: Real People, Real Places, Real Data” (AREN)
Conference participants expressed interest in learning more about NASA assets, including data and subject matter experts. Stemming from their participation in this first DS4E, several Science Activation teams are collaborating to potentially host regional events next year under the umbrella of this effort (PLACES in particular), a wonderful example of how Science Activation project teams help lead the charge in the advancement of key Science, Technology, Education, and Mathematics (STEM) fields, such as Data Science, to activate minds and promote a deeper understanding of our world and beyond.
Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
Data Science Education K-12 Research to Practice Conference Share Details Last Updated Apr 09, 2025 Editor NASA Science Editorial Team Related Terms Explore More 3 min read Findings from the Field: A Research Symposium for Student ScientistsArticle
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Mike Drury: A 40-Year Legacy of Precision
Deputy Integration and Testing Manager – Goddard Space Flight Center
Mike Drury began at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, as a temporary technician — a contractor hired for six weeks to set up High Capacity Centrifuge tests. Six weeks then turned into three months and, eventually, over 40 years.
Mike Drury, the deputy integration and testing manager for NASA’s Nancy Grace Roman Space Telescope, stands inside a clean room in front of Roman’s primary support structure and propulsion system. The “bunny suit” that he’s wearing protects the telescope from contaminants like dust, hair, and skin.NASA/Chris GunnNow, Mike is the deputy integration and testing manager for NASA’s Nancy Grace Roman Space Telescope. In this role, Mike oversees both Roman’s assembly and the many verification processes that ensure it is ready for launch.
“It’s a privilege to work here. There’s really no regrets,” Mike says. “This is a big place, and it is what you make it. You can really spread your wings and go into a lot of different areas and do different things.”
When Mike first began at Goddard, only government-employed technicians could work on space flight hardware. However, times were changing. The “old-timers,” as Mike affectionately calls them, soon began training a small group of contractors, including Mike, for flight hardware work. Mike credits these “old-timers” for the mindset he still carries decades later.
“They taught me how to approach things and execute, and that helped me through my entire career,” Mike says. “It’s that approach — making sure things are done right, without cutting any corners — that I always liked about working here.”
Not everyone can say that they worked on space missions while in college, but Mike can. Mike took advantage of a program through his contract that paid for classes. For 10 years, Mike studied at Anne Arundel Community College while continuing full-time work at Goddard, eventually earning an associate’s degree in mathematics.
While in community college, Mike also stocked up on several physics and calculus credits which helped prepare him to study thermal engineering at Johns Hopkins University. After seven more years of night classes, Mike completed a bachelor’s degree in mechanical engineering.
“Night school was really difficult between full-time work and traveling because I was working on several missions,” Mike says. “You needed that perseverance to just keep going and working away at it. So I just hung in there.”
In this 1989 picture, Mike works on NASA’s BBXRT (Broad Band X-ray Telescope) at NASA’s Kennedy Space Center in Florida. BBXRT flew on the space shuttle Columbia in 1990.NASAIn his 17 years of night school, Mike worked on seven missions, expanding his skill set from test set-up, to clean room tech work, to training astronauts. While working on the Hubble Space Telescope, Mike helped to train astronauts for their in-orbit tech work to install various instruments.
“Every mission I’ve worked on I’ve learned something,” Mike says. “Every test you learn more and more about other disciplines.”
After graduating from Johns Hopkins, Mike worked for a short time as an engineer before becoming an integration supervisor. In 2006, Mike took on the position of James Webb Space Telescope ISIM (Integrated Science Instrument Module) integration and test manager. After Webb’s ISIM was integrated with the Optical Telescope Element, Mike became the OTIS (Optical Telescope Element and Integrated Science Instrument Module) integration and testing manager.
“It was a tough eight to 10 years of work,” Mike says. “Loading the OTIS into the shipping container to be sent to NASA’s Johnson Space Center in Houston for further testing was a great accomplishment.”
To ensure that Webb’s ISIM would thrive in space, Mike was involved in more than three months of round-the-clock thermal vacuum testing. During this time, a blizzard stranded Mike and others on-site at Goddard for three days. Mike spent his nights overseeing thermal vacuum tests and his days driving test directors and operators to their nearby hotel rooms with his four-wheel-drive truck — a winter storm savior in short supply.
In this 1992 picture, Mike works alongside another technician on DXS (Diffuse X-Ray Spectrometer) in the shuttle bay at NASA’s Kennedy Space Center in Florida. DXS was a University of Wisconsin-Madison experiment flown during the January 1993 flight of NASA’s Space Shuttle Endeavor.NASAFor Mike, the hard work behind space missions is well worth it.
“As humans, we want to discover new things and see things. That’s what keeps me coming back — the thought of discovery and space flight,” Mike says. “I get excited talking to some of the Hubble or Webb scientists about the discoveries they’ve made. They answer questions but they also find themselves asking new ones.”
Some of these new questions opened by Hubble and Webb will be addressed by Mike’s current project — Roman.
“This team I would say is the best I’ve ever worked with. I say that because it’s the Goddard family. Everyone here on Roman has the same agenda, and that’s a successful, on-time launch,” Mike says. “My ultimate goal is to be staying on the beach in Florida after watching Roman blast off. That would be all the icing on the cake.”
Mike is also focusing on laying the groundwork for the next era at Goddard. He works hard to instill a sense of import, intention, and precision in his successors, just as the “old-timers” instilled in him 40 years ago.
“I talk to a lot of my colleagues that I’ve worked with for years, and we’re all excited to hand it off to the next generation,” Mike says. “It’s so exciting to see. I’m the old guy now.”
By Laine Havens
NASA’s Goddard Space Flight Center
NASA’s Planetary Defenders Documentary Premieres April 16
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)NASA is bringing the world of planetary defense to the public with its new documentary, “Planetary Defenders.”
Dr. Shantanu Naidu, Asteroid Radar Researcher, from NASA’s Jet Propulsion Laboratory points toward the Goldstone Solar System Radar in Barstow, CA – the most powerful planetary radar on Earth.Credit: NASAWhat would humanity do if an asteroid were headed for Earth? The documentary takes viewers inside the real-life efforts of scientists and engineers working to detect, track, and mitigate potential asteroid threats. Featuring firsthand accounts from experts on the front lines, the film reveals the science, technology, and personal dedication behind planetary defense. The film also showcases the teamwork that drives this critical global effort.
Debuting on NASA+ Wednesday, April 16, NASA is inviting the public to participate in a special YouTube Premiere event at 4:30 p.m. EDT. During this interactive screening, viewers can watch the first public showing of the film together and ask questions to NASA planetary defense experts.
To engage audiences further, NASA is providing digital creators with a toolkit that includes resources, activities, and ways to join the mission of planetary defense.
Established in 2016, NASA’s Planetary Defense Coordination Office leads the agency’s mission to find, track, and understand asteroids and comets that could pose a risk to Earth.
Stay up to date on NASA’s planetary defense efforts: https://www.nasa.gov/planetarydefense
About the AuthorEmily Furfaro Share Details Last Updated Apr 09, 2025 Related Terms Explore More 3 min read Hubble Helps Determine Uranus’ Rotation Rate with Unprecedented PrecisionAn international team of astronomers using the NASA/ESA Hubble Space Telescope has made new measurements…
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Sols 4505-4506: Up, up and onto the Devil’s Gate
- Curiosity Home
- Science
- News and Features
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- Mars Missions
- Mars Home
3 min read
Sols 4505-4506: Up, up and onto the Devil’s Gate This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4503 (2025-04-07 00:33:50 UTC). NASA/JPL-CaltechWritten by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick
Earth planning date: Monday, April 7, 2025
Over the weekend, we completed our drive up the steep side of a canyon, up onto “Devil’s Gate,” a small butte which forms part of the ridge along the top of the canyon and now we can see down into the next canyon. It is always true that we are going somewhere no one has been before – that’s the idea of an exploratory mission after all, and everyone kind of gets used to it, we don’t stop to think about it. But today, coming over the top of a hill like this and fully looking for the first time into an area that we have only had glimpses of before, it really brings it home that the mission is doing something extraordinary, something out of this world …. and brings that feeling of awe back into focus.
We did not pass SRAP (Slip Risk Assessment Process) a couple of times as we climbed up the side of this canyon, meaning that the contact science instruments (APXS and MAHLI) had to stand down for that day’s planning. However, this morning, in addition to a brand new vista, we saw that all six wheels are firmly on the ground and we passed SRAP quickly this morning, which must have been a relief to the rover planner in charge of assessing it today! (no one wants to be the bearer of bad news, day after day!)
Bedrock here has both flat bedrock and amazing large nodular features, which appear to have “wind tails” caused by winds consistently blowing in the same direction. This is a Touch and Go plan, so APXS and MAHLI are focusing on a single target, the brushed “Coronado” target on the flat bedrock in front of us. ChemCam will use LIBS to investigate the nodular features at “La Cumbre Peak.”
Near the rover, Mastcam will image some small diagenetic features at “Boulder Oaks” and the LIBS target. The 3×2 (2 rows of 3 images) “La Jolla Valley” mosaic focuses on a very nodular patch, just outside of the workspace reachable by the arm. Further from the rover, the 6×2 mosaic (2 rows of 6 images) “Los Penasquitos” looks at an amazing almost vertical vein. This discontinuous vein stretches for about 6 meters (about 18 feet), with vein fins sticking above the surface at various points, like a series of shark fins breaking the bedrock surface. Much further afield, ChemCam will acquire a long distance image on “Condor Peak,” which appears to have large scale vein networks, known as “boxwork structures” and may be an early example of the boxworks we are hoping to reach in Fall 2025.
The ENV (Environmental and Atmospheric group) planned a Mastcam “tau” measurement, to look at dust in the atmosphere. There is a paired Navcam activity, looking at dust devils towards the north of the crater on the first sol and towards the south on the second sol. A suprahorizon movie and our usual DAN and REMS measurements round out this plan.
Let’s see what the next drive will reveal to us!
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Welcome to the Mission Support Directorate
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Portrait of David Mitchell, Thursday, Jan. 27, 2022, NASA Headquarters Mary W. Jackson building in Washington.NASA/Bill Ingalls David Mitchell, Associate Administrator for Mission Support DirectorateHave you ever wondered how NASA manages to achieve all the incredible missions it does, like probing the Sun and studying the history of our Universe? We do it through teamwork, one of our core values. And an essential part of NASA’s team is what we call Mission Support. Mission Support makes sure NASA’s missions, centers, and programs have the capabilities and services they need to explore the unknown, innovate for the future, and inspire the world.
To illustrate Mission Support at NASA, look at the example of the Roman Space Telescope. It’s not just scientists and engineers who are making the telescope happen. The program works with NASA’s financial office to plan the budget for the telescope. Engineers design the telescope with tools developed in coordination with NASA’s shared services and information technology offices. NASA’s engineering authority checks the design, and international relations manages NASA’s collaborations with other countries on the telescope. All of this is Mission Support.
Of course, there is much more to Mission Support, but I think you get the picture. The Mission Support Directorate (MSD) enables Mission Support by:
- Planning and executing the Mission Support budgets for safety, security, and mission services as well as construction and environmental management.
- Executing strategy and governance to ensure Mission Support is financially sound, aligned with the agency’s goals, and serving NASA’s missions.
- Addressing Mission Support’s financial, operational, legal, and reputational risks to ensure resilience and mission success.
- Working with mission directorates and centers to ensure NASA is prioritizing the Mission Support services they need most urgently to be successful.
- Integrating Mission Support services across the agency to maximize efficiency and effectiveness.
Current and future missions require significant support to be successful. MSD is working today to ensure Mission Support is there for NASA to explore the unknown, innovate for the future, and inspire the world.
To learn more, visit MSD Organization.
Sixty Years in Canberra: NASA’s Deep Space Network
Deep Space Station 43 (DSS-43), a 230-foot-wide (70-meter-wide) radio antenna at NASA’s Deep Space Network facility in Canberra, Australia, is seen in this March 4, 2020, image. DSS-43 was more than six times as sensitive as the original antenna at the Canberra complex, so it could communicate with spacecraft at greater distances from Earth. In fact, Canberra is the only complex that can send commands to, and receive data from, Voyager 2 as it heads south almost 13 billion miles (21 billion kilometers) through interstellar space. More than 15 billion miles (24 billion kilometers) away, Voyager 1 sends its data down to the Madrid and Goldstone complexes, but it, too, can only receive commands via Canberra.
As the Canberra facility celebrated its 60th anniversary on March 19, 2025, work began on a new radio antenna. Canberra’s newest addition, Deep Space Station 33, will be a 112-foot-wide (34-meter-wide) multifrequency beam-waveguide antenna. Buried mostly below ground, a massive concrete pedestal will house cutting-edge electronics and receivers in a climate-controlled room and provide a sturdy base for the reflector dish, which will rotate during operations on a steel platform called an alidade.
When it goes online in 2029, the new Canberra dish will be the last of six parabolic dishes constructed under NASA’s Deep Space Network Aperture Enhancement Program, which is helping to support current and future spacecraft and the increased volume of data they provide. The network’s Madrid facility christened a new dish in 2022, and the Goldstone, California, facility is putting the finishing touches on a new antenna.
Image credit: NASA
Findings from the Field: A Research Symposium for Student Scientists
3 min read
Findings from the Field: A Research Symposium for Student ScientistsWithin the scientific community, peer review has become the process norm for which an author’s research or ideas undergo careful examination by other experts in their field. It encourages each scientist to meet the high standards that they themselves, as writers and reviewers, have aided in setting. It has become essential to the academic writing practice.
Historically, the peer review process has been limited to higher education and scholars more established in their academic careers. It has been required by only the more reputable publications, which can mean that lesser-known journals that don’t require this rigorous peer review process contain lower quality or less reliable information.
In an effort to give scientists of all ages the opportunity to participate in and contribute to the advancement of human knowledge in a meaningful and reliable way, the Gulf of Maine Research Institute (GMRI) began publishing Findings from the Field, a journal of student ecological and environmental science, launched in 2017. Students conduct authentic scientific inquiry, subject their research to the peer review process, and submit their revised work for editorial board review before publication—the same process a NASA scientist must go through! This hands-on, real-world experience in scientific communication sharpens these young scientists’ skills and immerses them in the collaborative nature of research—an essential foundation for the next generation of scientists.
After 7 years and 7 published volumes, Findings from the Field was ready to expand, and the Findings Student Research Symposium was launched. The Symposium was a success from the start, with 65 student scientists joining the event the first year and attendance climbing to 95 for year two. On March 10, 2025, GMRI (the anchor institution for the NASA Science Activation program’s Learning Ecosystems Northeast (LENE) project) welcomed nearly 100 young scientists, ranging from grades 5-12. These students, representing eight schools across Maine and New Hampshire, came together to share their research and engage in an evolving, intergenerational scientific community—one that fosters curiosity, collaboration, and scientific discovery.
Students presented their research through posters and live presentations, covering topics ranging from invasive green crab species, to the changing landscapes of Ash and Hemlock trees, and more. By connecting students with professional researchers, fostering peer discussions, and providing a platform for publishing legitimate scientific work, the Findings Symposium is a launch pad for the future of the scientific community.
One important element of the Symposium is the opportunity for young scientists to dialogue with professional scientists. Students engaged with researchers from Markus Frederich’s lab at the University of New England, volunteers from local organizations like Unum and Avangrid, and expert staff from GMRI.
Student Madalyn Bartlett from Sacoppee Valley Middle School shared, “It makes me feel really proud, because I get to talk to professional scientists that have a lot of experience in this, and it make me feel like I am contributing to something bigger than my school and my community.”
These interactions emphasize that science isn’t confined to white coats and labs—it’s about curiosity, observation, and shared knowledge. The keynote speaker, Kat Gardner-Vandy from a former NASA Science Activation project team, Native Earth | Native Sky, reinforced this message, inspiring students to see themselves as vital contributors to science and our collective knowledge about the world.
The Learning Ecosystems Northeast project is supported by NASA under cooperative agreement award number NNX16AB94A and is part of NASA’s Science Activation Portfolio. Learn more about Learning Ecosystems Northeast: https://www.learningecosystemsnortheast.org/
Native Earth | Native Sky’s Kat Gardner-Vandy delivering the keynote speech to students at the Findings Symposium. Share Details Last Updated Apr 08, 2025 Editor NASA Science Editorial Team Related Terms Explore More 34 min read Style Guidelines for ‘The Earth Observer’ NewsletterArticle
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NASA’s First Flight With Crew Important Step on Long-term Return to the Moon, Missions to Mars
The Artemis II test flight will be NASA’s first mission with crew under Artemis. Astronauts on their first flight aboard NASA’s Orion spacecraft will confirm all of the spacecraft’s systems operate as designed with crew aboard in the actual environment of deep space. Through the Artemis campaign, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars – for the benefit of all.
The unique Artemis II mission profile will build upon the uncrewed Artemis I flight test by demonstrating a broad range of SLS (Space Launch System) and Orion capabilities needed on deep space missions. This mission will prove Orion’s critical life support systems are ready to sustain our astronauts on longer duration missions ahead and allow the crew to practice operations essential to the success of Artemis III and beyond.
Leaving EarthThe mission will launch a crew of four astronauts from NASA’s Kennedy Space Center in Florida on a Block 1 configuration of the SLS rocket. Orion will perform multiple maneuvers to raise its orbit around Earth and eventually place the crew on a lunar free return trajectory in which Earth’s gravity will naturally pull Orion back home after flying by the Moon. The Artemis II astronauts are NASA’s Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen.
The initial launch will be similar to Artemis I as SLS lofts Orion into space, and then jettisons the boosters, service module panels, and launch abort system, before the core stage engines shut down and the core stage separates from the upper stage and the spacecraft. With crew aboard this mission, Orion and the upper stage, called the interim cryogenic propulsion stage (ICPS), will then orbit Earth twice to ensure Orion’s systems are working as expected while still close to home. The spacecraft will first reach an initial orbit, flying in the shape of an ellipse, at an altitude of about 115 by 1,400 miles. The orbit will last a little over 90 minutes and will include the first firing of the ICPS to maintain Orion’s path. After the first orbit, the ICPS will raise Orion to a high-Earth orbit. This maneuver will enable the spacecraft to build up enough speed for the eventual push toward the Moon. The second, larger orbit will take approximately 23.5 hours with Orion flying in an ellipse between about 115 and 46,000 miles above Earth. For perspective, the International Space Station flies a nearly circular Earth orbit about 250 miles above our planet.
After the burn to enter high-Earth orbit, Orion will separate from the upper stage. The expended stage will have one final use before it is disposed through Earth’s atmosphere—the crew will use it as a target for a proximity operations demonstration. During the demonstration, mission controllers at NASA’s Johnson Space Center in Houston will monitor Orion as the astronauts transition the spacecraft to manual mode and pilot Orion’s flight path and orientation. The crew will use Orion’s onboard cameras and the view from the spacecraft’s windows to line up with the ICPS as they approach and back away from the stage to assess Orion’s handling qualities and related hardware and software. This demonstration will provide performance data and operational experience that cannot be readily gained on the ground in preparation for critical rendezvous, proximity operations and docking, as well as undocking operations in lunar orbit beginning on Artemis III.
Checking Critical SystemsFollowing the proximity operations demonstration, the crew will turn control of Orion back to mission controllers at Johnson and spend the remainder of the orbit verifying spacecraft system performance in the space environment. They will remove the Orion Crew Survival System suit they wear for launch and spend the remainder of the in-space mission in plain clothes, until they don their suits again to prepare for reentry into Earth’s atmosphere and recovery from the ocean.
While still close to Earth, the crew will assess the performance of the life support systems necessary to generate breathable air and remove the carbon dioxide and water vapor produced when the astronauts breathe, talk, or exercise. The long orbital period around Earth provides an opportunity to test the systems during exercise periods, where the crew’s metabolic rate is the highest, and a sleep period, where the crew’s metabolic rate is the lowest. A change between the suit mode and cabin mode in the life support system, as well as performance of the system during exercise and sleep periods, will confirm the full range of life support system capabilities and ensure readiness for the lunar flyby portion of the mission.
Orion will also checkout the communication and navigation systems to confirm they are ready for the trip to the Moon. While still in the elliptical orbit around Earth, Orion will briefly fly beyond the range of GPS satellites and the Tracking and Data Relay Satellites of NASA’s Space Network to allow an early checkout of agency’s Deep Space Network communication and navigation capabilities. When Orion travels out to and around the Moon, mission control will depend on the Deep Space Network to communicate with the astronauts, send imagery to Earth, and command the spacecraft.
After completing checkout procedures, Orion will perform the next propulsion move, called the translunar injection (TLI) burn. With the ICPS having done most of the work to put Orion into a high-Earth orbit, the service module will provide the last push needed to put Orion on a path toward the Moon. The TLI burn will send crew on an outbound trip of about four days and around the backside of the Moon where they will ultimately create a figure eight extending over 230,000 miles from Earth before Orion returns home.
To the Moon and “Free” Ride HomeOn the remainder of the trip, astronauts will continue to evaluate the spacecraft’s systems, including demonstrating Earth departure and return operations, practicing emergency procedures, and testing the radiation shelter, among other activities.
The Artemis II crew will travel approximately 4,600 miles beyond the far side of the Moon. From this vantage point, they will be able to see the Earth and the Moon from Orion’s windows, with the Moon close in the foreground and the Earth nearly a quarter-million miles in the background.
With a return trip of about four days, the mission is expected to last about 10 days. Instead of requiring propulsion on the return, this fuel-efficient trajectory harnesses the Earth-Moon gravity field, ensuring that—after its trip around the far side of the Moon—Orion will be pulled back naturally by Earth’s gravity for the free return portion of the mission.
Two Missions, Two Different TrajectoriesFollowing Artemis II, Orion and its crew will once again travel to the Moon, this time to make history when the next astronauts walk on the lunar surface. Beginning with Artemis III, missions will focus on establishing surface capabilities and building Gateway in orbit around the Moon.
Through Artemis, NASA will explore more of the Moon than ever before and create an enduring presence in deep space.
NASA’s Deep Space Network Starts New Dish, Marks 60 Years in Australia
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The radio antennas of NASA’s Canberra Deep Space Communications Complex are located near the Australian capital. It’s one of three Deep Space Network facilities around the world that keep the agency in contact with dozens of space missions.NASA Located at Tidbinbilla Nature Reserve near the Australian capital city, the Canberra complex joined the Deep Space Network on March 19, 1965, with one 85-foot-wide (26-meter-wide) radio antenna. The dish, called Deep Space Station 42, was decommissioned in 2000. This photograph shows the facility in 1965.NASACanberra joined the global network in 1965 and operates four radio antennas. Now, preparations have begun on its fifth as NASA works to increase the network’s capacity.
NASA’s Deep Space Network facility in Canberra, Australia celebrated its 60th anniversary on March 19 while also breaking ground on a new radio antenna. The pair of achievements are major milestones for the network, which communicates with spacecraft all over the solar system using giant dish antennas located at three complexes around the globe.
Canberra’s newest addition, Deep Space Station 33, will be a 112-foot-wide (34-meter-wide) multifrequency beam-waveguide antenna. Buried mostly below ground, a massive concrete pedestal will house cutting-edge electronics and receivers in a climate-controlled room and provide a sturdy base for the reflector dish, which will rotate during operations on a steel platform called an alidade.
Suzanne Dodd, the director for the Interplanetary Network Directorate at JPL, addresses an audience at the Deep Space Network’s Canberra complex on March 19, 2025. That day marked 60 years since the Australian facility joined the network.NASA“As we look back on 60 years of incredible accomplishments at Canberra, the groundbreaking of a new antenna is a symbol for the next 60 years of scientific discovery,” said Kevin Coggins, deputy associate administrator of NASA’s SCaN (Space Communications and Navigation) Program at NASA Headquarters in Washington. “Building cutting-edge antennas is also a symbol of how the Deep Space Network embraces new technologies to enable the exploration of a growing fleet of space missions.”
When it goes online in 2029, the new Canberra dish will be the last of six parabolic dishes constructed under NASA’s Deep Space Network Aperture Enhancement Program, which is helping to support current and future spacecraft and the increased volume of data they provide. The network’s Madrid facility christened a new dish in 2022, and the Goldstone, California, facility is putting the finishing touches on a new antenna.
Canberra’s RoleThe Deep Space Network was officially founded on Dec. 24, 1963, when NASA’s early ground stations, including Goldstone, were connected to the new network control center at the agency’s Jet Propulsion Laboratory in Southern California. Called the Space Flight Operations Facility, that building remains the center through which data from the three global complexes flows.
The Madrid facility joined in 1964, and Canberra went online in 1965, going on to help support hundreds of missions, including the Apollo Moon landings.
Three eye-catching posters feature the larger 230-foot (70-meter) antennas located at the three Deep Space Network complexes around the world.NASA/JPL-Caltech“Canberra has played a crucial part in tracking, communicating, and collecting data from some of the most momentous missions in space history,” said Kevin Ferguson, director of the Canberra Deep Space Communication Complex. “As the network continues to advance and grow, Canberra will continue to play a key role in supporting humanity’s exploration of the cosmos.”
By being spaced equidistant from one another around the globe, the complexes can provide continual coverage of spacecraft, no matter where they are in the solar system as Earth rotates. There is an exception, however: Due to Canberra’s location in the Southern Hemisphere, it is the only one that can send commands to, and receive data from, Voyager 2 as it heads south almost 13 billion miles (21 billion kilometers) through interstellar space. More than 15 billion miles (24 billion kilometers) away, Voyager 1 sends its data down to the Madrid and Goldstone complexes, but it, too, can only receive commands via Canberra.
New TechnologiesIn addition to constructing more antennas like Canberra’s Deep Space Station 33, NASA is looking to the future by also experimenting with laser, or optical, communications to enable significantly more data to flow to and from Earth. The Deep Space Network currently relies on radio frequencies to communicate, but laser operates at a higher frequency, allowing more data to be transmitted.
As part of that effort, NASA is flying the laser-based Deep Space Optical Communications experiment with the agency’s Psyche mission. Since the October 2023 launch, it has demonstrated high data rates over record-breaking distances and downlinked ultra-high definition streaming video from deep space.
“These new technologies have the potential to boost the science and exploration returns of missions traveling throughout the solar system,” said Amy Smith, deputy project manager for the Deep Space Networkat JPL, which manages the network. “Laser and radio communications could even be combined to build hybrid antennas, or dishes that can communicate using both radio and optical frequencies at the same time. That could be a game changer for NASA.”
For more information about the Deep Space Network, visit:
https://www.nasa.gov/communicating-with-missions/dsn/
NASA’s New Deep Space Network Antenna Has Its Crowning Moment NASA’s New Experimental Antenna Tracks Deep Space Laser VIDEO: How Do We Know Where Faraway Spacecraft Are? News Media ContactIan J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov
2024-048
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Article 2 weeks ago Share Details Last Updated Apr 08, 2025 Related Terms Explore More 5 min read Perseverance Rover Witnesses One Martian Dust Devil Eating Another Article 5 days ago 3 min read University High Triumphs at JPL-Hosted Ocean Sciences Bowl Article 1 week ago 6 min read NASA’s Curiosity Rover Detects Largest Organic Molecules Found on MarsLee esta historia en español aquí. Researchers analyzing pulverized rock onboard NASA’s Curiosity rover have found…
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Style Guidelines for ‘The Earth Observer’ Newsletter
34 min read
Style Guidelines for ‘The Earth Observer’ Newsletter IntroductionEditorial Process for The Earth Observer Types of Articles in The Earth ObserverGeneral article format
— Announcement article
— Feature article
— Hybrid article
— In Memoriam article
— Kudos article
— Summary articleGuidelines for Preparing Articles for The Earth Observer
— Writing for the web
— Catchy headline
— Naming files
— Use visuals to draw the reader in
— Search engine optimization
—— Headline and subheads
—— Links
—— Alternate text for graphics
— Submitting An Outline
— Submitting Your DraftSpecific Style Guidelines
— Acronyms
— Affiliations
— Capitalize Earth, Moon, Sun
— Chemical formulas
— Compound words
— Cross-references
— Dates, months, and seasons
— Directions and regions
— Footnotes
— Formal titles
— Hyperlinks, the how and the why
—— How to insert a hyperlink
— Hyphens, en dashes, and em dashes—oh my!!
— Italics and quotes
— Items in a series
— Numbers
— Ordinal numbers
— References
— References to teams
— State abbreviations
— Typographical emphasisGuidelines for Graphics, Photos, Visualizations, Animations
— Inserting figures, photos, animations, and visualizations
— Caption, credit, and tags
— Graphic/photo requirementsFinal Thoughts Introduction
This document contains guidelines to assist you as you prepare articles for The Earth Observer (EO) newsletter. Our Editorial Team appreciates your cooperation in keeping these guidelines in mind as you prepare articles for submission. Our team reviews every article, but following the style guidelines will expedite the editorial process.
Please be aware that this style guide is a living document and as such continues to evolve. If it has been a while since you have submitted an article for The Earth Observer, please be sure you are using the latest version of the Style Guide. The date of the most recent update is printed in the footer of the document to make it easier to maintain the most current version of the document.
Editing is sometimes more art than science, and while the Editorial Team will endeavor to follow the rules that follow in most cases, there may be specific cases where the Executive Editor may decide to deviate from these guidelines.
The Earth Observer Editorial ProcessThe EO has a robust editorial team to assist with the editorial process to maintain the quality and style of the publication.
The EO editorial staff includes:
- Steve Platnick, assigned task representative
- Alan B. Ward, executive editor
- Dalia Kirshenblat, managing editor
- Doug Bennett, associate editor
- Stacy W. Kish, assistant/technical editor
- Ernest Hilsenrath, technical editor
- Jim Irons, technical editor
- Mike Marosy, design/production
The editorial process is iterative. The author will typically go through two rounds of edits with the EO Editorial Team. The text is then put into a preview layout on a staging server for the author’s final review before the story is published on the EO website.
Types of Articles in The Earth ObserverThe Earth Observer provides authors an opportunity to tell their compelling stories of Earth Science. As such it does not impose strict word count limits, but the EO has established certain general guidelines that provide a framework to follow for several types of articles.
General article format
Please write articles in MS Word and save as a .doc file.
The article should begin with an introduction that provides the essentials – who, what, where, when, and why – to provide the reader with an overview of the topic to be discussed. For articles about meetings include the number of people who attended (e.g., in-person and virtual) and the objective of the meeting.
The introduction paragraph is followed by a transition paragraph that takes the reader into the main content of the article. The article should wrap up with a conclusion.
The suggested page length for each type of article includes inserted visual elements. In addition to the Word file, please also send separate higher resolution files for graphics, photos, animations, or visualizations. More specific requirements are available in the Guidelines for Graphics, Photos, Visualizations, Animations.
Announcement article
Announcement articles promote a variety of topics. Historically this type of article includes releases of new or updated Earth Science data products, information on new tools for processing and viewing data, previews of outreach activities for the Science Support Office (e.g., AGU, Earth Day), and details on upcoming science meetings or workshops (i.e., beyond the information conveyed on the NASA science calendar).
The article is structured like a Feature article, but it is shorter, no more than two pages, including graphics and captions – see Guidelines for Graphics, Photos, Visualizations, Animations.
For Example: NASA Invites You to Create Landsat-Inspired Arts and Crafts, The Earth Observer, Mar–Apr 2021, 33:4, 13–14. Other examples are available on the archived issues of The Earth Observer.
If you have an idea for an Announcement article, please email the EO Editorial Team who will work with you on a draft. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
Feature article
Feature articles cover a wide range of Earth science topics, including satellite mission launches and historic milestones, field campaign updates, data processing tool tutorials, and summaries of NASA Science Support Office outreach events. Typically, these articles span ~8–14 pages (3000–4000 words). There are cases where longer or shorter articles are acceptable.
A photo essay format for some topics, such as outreach event summaries, offer an option to convey a significant portion of the information using a collection of photos and descriptive captions.
For Example: Looking Back on Looking Up: The 2024 Total Solar Eclipse
If you have an idea for an Feature article, please email the EO Editorial Team who will work with you on a draft. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
Hybrid article
Hybrid articles combine elements of a Feature and a Summary article. Often, these articles start with a few pages of descriptive text about the subject, followed by a summary of a particular meeting. Owing to their hybrid nature, these articles tend to run a bit longer than the standard Summary article. These articles typically range between 8–12 pages (3000–5000 words.)
If you have an idea for a Hybrid article, please email the EO Editorial Team who will work with you on a draft. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
In Memoriam article
In Memoriam articles recognize individuals who have played prominent roles in NASA Earth Science. These articles tend to include biographical information about the deceased individual, a brief mention of their education, and a summary of their major career achievements – with emphasis on achievements related to NASA. A typical In Memoriam article layout includes one or more photos, including one of the person being memorialized.
For Example: In Memoriam: Mary Cleave [1947–2023] The In Memoriam link provides recent examples of In Memoriam articles published in The Earth Observer. Other articles are available by searching the publication’s archived issues.
This type of article is structured like a Feature article with the exception that the subject is referred to by their first name. In Memoriam drafts should be no more than two pages in Word – including graphics and captions – see Guidelines for Graphics, Photos, Visualizations, Animations.
If you know someone to eulogize in The Earth Observer for their contributions to NASA Earth Science, please email the EO Editorial Team who will work with you on a draft. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
Kudos article
Kudos articles acknowledges individuals or groups either within or connected to (funded by) NASA who receive significant NASA-wide awards.
A Kudo article follows a structure similar to a Feature article. It should be a maximum of one page in Word – including a photo of person(s) or group being honored – see Guidelines for Graphics, Photos, Visualizations, Animations.
For Example: MOPITT Canadian Principal Investigator Receives Two Awards, The Earth Observer, Mar–Apr 2021, 33:2, 28 [bottom]. Other examples are available by searching through archived issues of The Earth Observer.
If you know an individual or a group of people worthy of recognition for their NASA-related achievement, please email the EO Editorial Team who will work with you on a draft submission. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
Summary article
Summary articles provide an overview of recent scientific meetings and/or workshops. Ideally, a Summary article should be no more than 6 pages (~2500 words).
Provide the flavor of the event rather than describe it in detail. Summarize the overall nature and sense of sessions. The Editorial Team has found that a mix of narrative descriptions of key (usually programmatic) presentations (e.g., plenary sessions) and summaries with less detail for the remaining (e.g., technical) presentations is optimum.
Now that The Earth Observer is published online, it is the view of the Editorial Team format summary articles using a “minutes-style” report of the meeting. While space no longer precludes publishing such an article as it did in the past, the format does not translate well to the online communication medium. Unless a reader is really interested in the specific topic(s) discussed in the article, it is likely that they will not scroll through to the end – no matter how nice the layout looks.
If you have an idea for a Summary article, please email the EO Editorial Team who will work with you on a draft. The EO Editorial Team emails are available in the section – The Earth Observer Editorial Process
Guidelines for Preparing Articles for The Earth ObserverEOis a hybrid publication, landing somewhere between a science journal and popular science magazine. Therefore, the focus should be on phenomena rather than data. The article provides an opportunity to publicize your mission, research to ~1653 subscribers (as of August 2024) around the world. Please review the content in this guideline before writing your article and reach out to the Editorial Team if you have any questions.
Writing for the web
The EO audience ranges from scientists to the general public. When writing an article, use plain language and active voice. When in doubt, write the article so that it would be understandable to a friend or relative not in the field.
For Example:
Passive voice: The rate of evaporation is controlled by the size of an opening.
Active voice: The size of an opening controls the rate of evaporation.
Avoid using jargon and technical language. When it is necessary to use technical language, please use ITALICS to offset the word in the text. Follow the italicized word with a brief definition or explanation.
For Example: Inference – formally derived uncertainty for area estimates of biomass, height, or other metrics – can take different forms, each of which includes specific assumptions. In this breakout session, participants considered the strengths and limitations of different inference types (e.g., intensity of computation or the ability to use different models).
Writing content for a website differs from print. The human eye is more inclined to read shorter paragraphs separated by breaks. It is ideal to keep sentences and paragraphs short.
Use one space after a period. The two spaces after a period is an artifact of conventional type writers.
Avoid editorializing in the article. For example, do not characterize a spacewalk as “daring” or “dangerous.” Describe the events factually. If things are described well, readers easily can decide for themselves whether they are daring or dangerous. Never, under any circumstances, insert any personal, political, ideological, or religious opinions or beliefs into NASA news media products.
Catchy headline
Write a headline that is short, searchable, and shareable. Try to keep the headline to 60 characters (including spaces). Longer headlines may be invisible to search engines.
Unlike journal articles, The Earth Observer only includes individuals who made a significant contributions to the EO article. A typical article should only lists one or two authors. In some occasions, an article may have up to four authors. The authors should be formatted as follows:
First Last, Organization, author email
If there are more you wish to give credit, consider doing so in an Acknowledgment section, as discussed in the next paragraph.
Naming files
For consistency moving documents through the editorial process, please name the file by the file type, the topic, and the author’s last name.
For Example: announcement_topic_author
feature_topic_author
hybrid_topic_author
memoriam_topic_author
kudos_topic_author
summary_topic_author
Use visuals to draw the reader in
The Earth Observer is now published online. Visual elements are critical to all EO stories and are a required element to submissions. The Editorial Team would prefer having too many graphics (i.e., photos, figures, animations, and visualizations) than too few. It is helpful to insert this content into the Word file as well as include the graphics as separate files at the time of the initial submission of the draft for editorial review. See the Guidelines for Graphics, Photos, Visualizations, Animations section for more information.
Search engine optimization
Search Engine Optimization (SEO) is a broad set of techniques to capitalize how search engines, such as Google, scrub content on the internet. By optimizing how articles are written, it is possible to influence where content shows up in an organic, online search. The different approaches can fill an entire book. This style guide provides a few pointers to help tweak articles to optimize how the content appears in online searches.
Headline and subheads
A headline should be clear and compelling to reveal what the content is about as well as entice the searcher to click for more. A SEO headline is a ranking factor in search engine results. A headline can be crafted to rank higher in search results, which increases an article’s visibility and generate more clicks. This can be done by using SEO search terms — those terms that a person would type into a search box — in the headline. Shorter headlines (i.e., 60 characters including spaces) are often more effective during searches.
Subheads provide a way to organize an article and separates the content into digestible sections. Like headlines, subheads can be optimized for SEO searches. Subheads may include key takeaways from the specific section. Keep subheads clear and concise.
Links
Earth Observer articles are now being posted online. Footnotes are no longer a functional option, which is a significant change for authors who have published articles in our print issues in the past. It is helpful to hyperlink words or short phrases in the article that directs the reader to additional content from the meeting, such as presentations, poster sessions, talks by attendees, programs/satellites, journal articles, etc. Relevant links should also be added to captions. See the Hyperlinks section for guidance on how to insert and format a hyperlink in the article.
Internal links tie content in the article to other pages within an organization, such as NASA, to boost site authority. External links direct a reader to sites outside the organization. This approach also drives up site authority in SEO searches. By connecting relevant pages, it will improve article navigation and ensure users can locate relevant information.
Alternate text for graphics
Alternate text, or alt text, is the small description added to visual elements on the back end of a website. Search engines use the alt text to identify relevant content. Alt text also improves accessibility for all users. Tools that read webpages aloud can read alt text to help explain what visual elements contain for the visually impaired.
Alt text should be concise, accurate, and use keywords. Keywords are highly relevant words or phrases associated with the picture and the content of the article.
For Example: Figure 1. Forty SWOT Early Adopter (EA) teams span the globe with a wide range of operational and applied science project topics.
Figure credit: NASA
Key word tag: A global map showing the locations of early adopter organizations.
Submitting An Outline
An outline is not requiredprior to submitting the first draft of an article, but an outline may be beneficial for lengthy articles (i.e., features, hybrids). Outlines are particularly helpful for first-time authors or when an author is seeking guidance about the appropriateness of content for The Earth Observer. It is hard for the team to comment without seeing something in writing. More generally, submitting an outline presents an opportunity for the editorial team to provide input on the article during the writing process – as opposed to waiting until the first draft is submitted.
Submitting Your Draft
Do not submit a draft for review unless it is complete (i.e., contains all visual elements, captions, credits, and content). Unless you clearly indicate otherwise, the Editorial Team will assume your submission is ready for them to review. Version control problems result when text is updated after reviews have started.
The initial draft submitted for editorial review should include graphics. including captions and credits. The editorial process is delayed when graphics, credits, and captions are added iteratively once the process has begun.
Specific Style GuidelinesOver more than 35 years as a NASA publication, The Earth Observer has developed its own unique style. Please review these specific guidelines detailed below, and let the Editorial Team know if you have any questions. In addition, The Earth Observer also adheres to the NASA Stylebook and Communications Manual, 9th edition (June 2020), which is closely aligned with the AP Stylebook.
Acronyms
Science is rife with acronyms. On first usage, always spell out the acronym and follow with the acronym in parenthesis. From that point on in the article, use the acronym. To ensure photos, figures, visualizations, and animations are understandable if removed from the larger text, please spell out acronyms in captions.
Well-known acronyms (e.g., NASA, U.S., etc.) do not need to be spelled out. Separate the acronym for United States (e.g., U.S.) and United Kingdom (e.g., U.K.) with periods.
For Example: Level-1 (L1), Global Ecosystem Dynamics Investigation (GEDI), International Space Station (ISS), Precision Orbit Determination (POD), etc.
Only capitalize proper nouns as defined by the dictionary or AP style. The Earth Observer style does capitalize the first letter of a specific product that will be turned into an acronym.
For Example: Do not capitalize the first letter of each word in “solid rocket booster (SBR),” even though the subsequent use of the acronym SRB will appear in the article.
A compound acronym arises when parentheses occur inside of parentheses. In this situation, use [BRACKETS] for the outer set of parentheses and (PARENTHESES) for those inside.
For Example: Thomas Neumann [GSFC—Deputy Director of GSFC’s Earth Sciences Division (ESD)] welcomed meeting participants on behalf of the ESD.
Affiliations
Use a possessive for an organization when it is part of NASA. Do not use a possessive when using the agency as an adjective.
For Example: NASA’s Goddard Space Flight Center (GSFC); subsequent references would just use “GSFC.”
For Example: SWOT data products available through PO.DAAC provides centralized, searchable access that is available using an in-cloud commercial web service through the NASA EarthData portal.
Write out an organization that is not part of NASA.
For Example: Gustavo Oliveira [Clark University] presented details on the project “Irrigation as Climate-Change Adaptation in the Cerrado Biome of Brazil.”
When multiple “levels” of affiliation are listed, start with the “top-level” affiliation as a possessive followed by lower level. If the affiliations are mentioned again later in the article, only the acronym for the lowest level needs to be repeated.
For Example: For NASA’s Goddard Space Flight Center’s Global Modeling and Assimilation Office (GMAO), subsequent references to this entity would be “GMAO.”
For Example: For University of Maryland, Baltimore County’s Earth System Science Interdisciplinary Center (ESSIC), subsequent references to this entity would be “ESSIC.”
When a person is affiliated with two (or more) distinct entities, separate the two entities by slashes.
For Example: Project Scientist Felix Landerer (NASA/JPL), followed by detailed assessments of the G-FO mission and operations status from the core SDS centers and flight operations teams.
When a NASA Center and contractor are listed, please list the NASA Center followed by contractor and separate the two entities by a slash.
For Example: NASA’s Goddard Space Flight Center (GSFC)/Global Science & Technology, Inc. (GST).
Capitalize Earth, Moon, Sun
NASA capitalizes the first letter in Earth, Moon, and Sun.In addition, do not use the modified ‘the’ before Earth.
For Example: This strategy acknowledges the urgency of global changes, such as accelerating environmental shifts, understanding Earth’s interconnected systems, and developing scalable information.
Chemical formulas
Chemical formulas should be treated like acronyms. Spell out a chemical formula upon first use in an article followed by the chemical formula in parenthesis. Use appropriate subscripts and superscripts in the chemical formula. From that point onward, use the chemical formula in the article.
For Example: The data show that global and East Asian emissions of oxides of nitrogen (NOx) have decreased since 2010, contrasting India and Southeast Asia’s rising trends. In Southeast Asia, NOx and sulfur dioxide (SO2) emissions increased from 1990–2018, while black carbon (BC) emissions peaked in 2007.
Compound words
Make one word out of all compound words (e.g., multipurpose, multiangle).
Exception: Hyphenate cases where the same vowel repeats (e.g., bio-optical, multi-imager).
Cross-references
It is common to reference a previous EO article to provide context and background for the current story. The Editorial Staff recommends authors cross-reference prior EOarticle. The title of the article, volume, issue, and page range in parenthesis. The information should be italicized, except for “The Earth Observer,” which should be plain text.
The name of the cross-referenced article should be hyperlinked to that article. You can find past Earth Observer newsletters on the archive page.
For Example: ESIP was created in response to a National Research Council (NRC) review of the Earth Observing System Data and Information System (EOSDIS). (To learn more about EOSDIS, see Earth Science Data Operations: Acquiring, Distributing, and Delivering NASA Data for the Benefit of Society, in the March–April 2017 issue of The Earth Observer [Volume 29, Issue 2, pp. 4–18].) As NASA’s first Earth Observing System (EOS) missions were launching or preparing to launch, the NRC called on NASA to develop a new, distributed structure that would be operated and managed by the Earth science community and would include observation and research, application, and education data.
Dates, months, and seasons
When referencing a date, spell out the month, followed by the day (if included) and year. This style differs from AP. A comma always follows a year if the date is written in-line of the sentence.
For Example: January 27, 2022; January 2022
For Example: PACE launched on February 8, 2024, from Vandenberg Space Force Base in California.
Capitalize a season followed by a year, but not when just referring to a season.
For Example: Spring 2022; summer
Spell out time zones, such as Eastern Daylight Time, and thereafter replace with the acronym (i.e., EDT).
For Example: In Cleveland, the eclipse began at 1:59 PM. Eastern Daylight Time (EDT), with totality spanning 3:13–3:17 PM.
Directions and regions
EO articles follow AP style for directions (e.g., north, south, east, west, northeast, southwest, norther, western, southern, eastern). The directions should be lowercase when indicating a compass direction and when it is used to describe sections of states or cities.
For Example: The cold front is moving east.
The direction should be capitalized for a proper name or large regions.
For Example: NASA’s South/Southeast Asia Research Initiative (SARI) is a regional initiative under the LCLUC program that addresses the critical needs of the South/Southeast Asia region.
For Example: West Virginia or North Dakota
Footnotes
The Earth Observer has transitioned to an online publication. Footnotes will no longer be used in articles. Instead of footnotes, the publication will use hyperlinks to direct readers to additional content. Refer to the section on Hyperlinks for more information on how to include a hyperlink in an article. A good mantra to follow – if you are unsure if a reference is needed, leave it out.
Formal titles
Formal titles, such as Ms. or Dr., are used in articles that are more personal, such as Kudos, In Memoriam, and The Editor’s Corner. For all other articles, the professional title is not used. When you introduce a person in the story, present the name in BOLD followed by their agency and position in ITALICS, offset by brackets.
For Example: First Last [Agency—Job Title] began by providing an update on the status of the new launch date for the. . . .
After the individual is introduced in the article, EO style follows a particular style for using the name again. If the individual’s name is included in the same paragraph where the person was introduced, only use the last name [UNBOLD]. If the individual is mentioned later in the article, several paragraphs removed from introduction, use the full name [FIRST LAST, UNBOLD].
Hyperlinks, the how and the why
Prior to moving online, The Earth Observer used footnotes to reference information in an article. The online publication will now use hyperlinks to refer the reader to additional content on a topic. As a general rule, hyperlink content regarding missions, instruments, field campaigns, models, papers, and other programs named in the article. It is not necessary to link to each individual institution mentioned when individuals are identified in summaries.
How to insert a hyperlink
The first step in this process is to identify the anchor text to highlight in the sentence. The anchor text includes a word or phrase that points the reader to additional content.
For Example: Anchor text: Volume 35 Issue 6 of The Earth Observer
Find the Uniform Resource Locator (URL) for the webpage. The URL is an address that specifies the location of a resource on the internet.
For Example: URL: https://eospso.gsfc.nasa.gov/sites/default/files/eo_pdfs/EO%20Nov-Dec%202023-Digital%20508.pdf
Note: When inserting a link to a prior published article from The Earth Observer’s archive, be certain to capture the URL for the first page of the referenced article, as opposed to the issue’s first page.
To insert a hyperlink, copy the URL from the website where the additional content can be found. Select the word or phrase to use as anchor text. Do not include an acronym as part of the anchor text for a hyperlink. Select the hyperlink command under the Insert dropdown menu. Paste the URL into the link box. Be sure the ‘Web Page or File’ tab is selected (not the Email tab). The hyperlinked text will appear blue and underlined.
For Example: It is possible to find this information in Volume 35 Issue 6 of The Earth Observer.
For Example: The Hyperwall presentation highlighted recent discoveries from the James Webb Space Telescope (JWST) mission.
Hyphens, en dashes, and em dashes—oh my!!
Hyphen: – A hyphen is used to separate compound adjectives or words.
For Example: The satellite reached a near-Earth orbit.
En Dash: – An en dash spans the length of a typed lowercase ‘n.’ This special character is used to separate numbers.
For Example: The meeting was held March 5–8 in Denver, CO. [Note there is no space between the numbers in this example.]
The Earth Observer style follows the NASA style guide that uses an en dash to insert a pause in the sentence. The en dash is set apart by a space on either side. In this instance, the en dash is used instead of an em dash.
For Example: The passport identified six hidden images – all six posters from the Science Explorers Poster Series– strategically placed within the exhibit’s perimeter.
You can insert an en dash in Word on a Mac by typing the “Option” and “hyphen/dash” keys simultaneously.
You can also insert an en dash in Word using the Insert tab and select Advanced Symbols. A box will open with a variety of characters. Select “Garamond” from the Font pulldown menu (Garamond is the newsletter’s preferred font), then select the – symbol (or “en dash”) from the array of options displayed. You will then see a confirmation of your selection appear below the symbol options (i.e., “Insert [Garamond] character 150 (Unicode character 2013).” Please note: the character number (150 in the case of Garamond) could be different. For example, an en dash in Palatino font is character 208.
Em Dash: — An em dash spans the length of a typed lowercase ‘m.’ This special character is used when separating the organization and the job title when introducing a person in the article. In other styles, the em dash is used as a pause in a sentence. Following NASA style guidelines, the pause is provided by the en dash.
For Example: Thomas Neumann [GSFC—Deputy Director of GSFC’s Earth Sciences Division (ESD)] welcomed meeting participants on behalf of the ESD.
You can insert an em dash in Word by going to the Insert tab and selecting Advanced Symbols. A box will open with a variety of characters. Select character 151. For more detailed guidance, please refer to the section above regarding how to insert an en dash.
Italics and quotes
Place Latin phrases in ITALICS (e.g., in situ, a priori, ad hoc, ex officio) on every appearance in the article. Do not italicize abbreviated Latin phrases (e.g., i.e., a.k.a., et al.). Use the Latin phrase i.e., instead of ‘such as’ and e.g., instead of ‘that is to say.’
For Example: The Afternoon Satellite Constellation, a.k.a., the“A-Train,” can see Earth in a whole new dimension.
For Example: Guy Schumann [Water in Sight]explained this Swedish start-up company uses SWOT data to validate in situ gauge data in Malawi.
Place technical language in the text in ITALICS followed by a definition. Only use the italics on the first usage of the word.
For Example:There were several large polynyas – areas of open ice where sea ice would be expected – detected.
Items in a series
The Earth Observer deviates from AP style in the use of commas in a list or series. Use the Oxford comma in a series of items.
For Example: The sensor measures at three different wavelengths corresponding to blue, green, red, and infrared light.
In more complex series where one of the items is a series of items within a series, it is permissible to use semi-colons to separate the series (see below).
For Example: The blue, green, and red channels; the two-infrared channels; and ultraviolet channel were all impacted.
Numbers
In the article, spell out zero to nine. Use numerals for any number greater than or equal to 10. If a sentence contains several numbers, excluding a year, that are both greater than and less than 10, use the numerals for all numbers.
For Example: Improving the data calibrations of the accelerometer measurements – which are noise contaminated on one of the two G-FO spacecraft – remains a core focus of the project SDS team.
For Example: The NASA Hyperwall served as the backdrop for 57 Hyperwall Storiesat the meeting, including 8 presentations delivered by the 2023 winnersof the AGU Michael Freilich Student Visualization Competition.
For Example: Following the project team’s status presentations, there was a 30-minute session to answer questions from the science community and discuss in more detail the mission performance, near-term operations and data processing plans, as well as to gather suggestions and feedback from the community.
Ordinal numbers
Ordinal numbers are words representing position or rank in sequential order. The EO follows AP rules in how to present ordinal numbers in an article. Spell out one through nine and use figures for 10 and above. This rule holds for article headlines and subheads.
For Example: AEOIP Holds Third Annual Workshop
For Example: As GPM is now well into its 10th year in orbit, the time is fitting to reflect on and celebrate what this mission has accomplished and showcase its contributions to science and society.
References
The Earth Observer is not a peer-reviewed journal and typically does not include a list of references. It is helpful to hyperlink key words/phrases to other resources, such as journal articles. See Hyperlinks section to learn how to insert and format this text.
In rare instances when a formal reference is required (e.g., referencing a Figure that originally appeared in another journal article), please use theAmerican Meteorological Society format.
References to teams
In a story, spell out “Science Team (ST)” in the first instance and use the team acronym from that point forward in the story.
For Example: The Precipitation Measurement Mission (PMM) Science Team (ST) includes more than 20 international partners.
For other named teams, use the initial caps for the team name and then use “Team” as shorthand afterwards (e.g., “Informatics Team” first time, then abbreviate as “Team” subsequently).
Do not capitalize generic references to a team (e.g., a team of experts).
State abbreviations
The Earth Observer differs from AP style in how it presents state abbreviations. This publication uses the two-letter postal code for state abbreviations.
For Example: The meeting was held March 5–8 in Denver, CO.
Typographical emphasis
Please do not use specialized typographic formatting (e.g., Heading 1, Heading 2, etc.). Instead, please use internal formatting (e.g., BOLD and ITALIC) as directed in the style guide (e.g., headings, subheads, author/speaker names, etc.). If you do use the specialized typographic formatting, it affects the insertion and layout of text on the EO website, which takes time to correct and slows publication.
When inserting a table, do not use framed or shaded boxes.
Units
Do not spell out units. Use the standard abbreviation. Include both English and metric units in the text. One exception is The Editor’s Corner column, which does not use both the English and metric units.
For Example: The data collected from G/G-FO has a native resolution of about 300 km (~186 mi).
Guidelines for Graphics, Photos, Visualizations, AnimationsThe EO supports several visual options to enhance the text of an article. A figure refers to a visual display of data. An photo refers to a photograph. An animation is a series of images or model results that illustrate a concept. A visualization is a video of content.
To maintain a consistent design for The Earth Observer, please insert the graphic, photo, animation, or visualization in the appropriate location in the Word document. Along with the Word document, please submit the photo, graphic, visualization, or animation as separate files.
Inserting figures, photos, animations, and visualizations
Upon first usage in the text, include the correct graphic descriptor (i.e., figure, photo, animation, or visualization) and appropriate number in the text in bold. Restart numbering for each visual element type (e.g., Figure 1, Photo 1, Figure 2, Figure 3, Photo 2, Visualization 1).
For Example: The GMI is a 13-channel conically scanning PMW radiometer providing observations across a wide swath (885 km or ~550 mi) to estimate precipitation – see Figure 1.
The EO editorial staff ask that no additional formatting be used when inserting these files into the Word document. At the location in the text where the photo, figure, animation, or visualization should appear in the story, advance the text by two lines. Place the cursor in the first blank line. Go to the insert tab and select the picture icon. Select ‘Picture from File’ from the dropdown. Navigate to the location on your computer where the file is located and select ‘Insert.’
Caption, credit, and tags
After inserting the figure, photo, visualization, or animation, provide a caption and credit. It is important to think of the caption and credit as stand-alone items in the story.
The graphic may need to be revised to accommodate EO style. Remove indicators, ‘a’, b’, etc from panels or items of note. EO style requires that different panels or points of interest in the graph should use “pointers,” such as top, middle, bottom.
The caption should be descriptive and not overly technical. It should convey the content in image/figure without relying too heavily on the surrounding text to add context. Relevant links should also be added to captions. Spell out all acronyms, whether for equipment or institutions, are already spelled out in the text, because the image can be lifted from the article and used without the article where it originated. The pointer in the caption should be enclosed in brackets and the text ITALICIZED (e.g., [left]).
The credit line should include the name of the institution or individual who should be credited for the image/figure/photograph. If an institution is listed, write the name [NO ITALICS]. Ifan individual is listed, include their institution in brackets. If the credit refers to a journal article, please use a reference to the journal (e.g., Williams et al. 2024) and link the credit reference to the DOI for the journal article. Note: there is no period after the credit line.
For Example:
Photo 1. Group photo of 2024 Quadrennial Ozone Symposium in-person attendees at the University of Colorado, Boulder’s University Memorial Center.
Photo credit: Chelsea Thompson [National Oceanic and Atmospheric Administration]
Photo 2. Sophie Godin-Beekman presents awards during the QOS dinner. Luke Western accepts the Dobson Award [left]; [Herman Smith receives the Farman award [middle]; and Valerie Thouret accepts the Farman award on behalf of Philippe Nédélec [right].
Photo credits: Irina Petropavlovskikh [CIRES Global Monitoring Laboratory]
Figure 1.Annual mean anomalies of ozone (%) in the upper stratosphere [top three panels] near 42 km (26 mi) altitude or 2-hPa pressure, and for the lower stratosphere, [bottom three panels] near 22 km (14 mi) or 50 hPa for three zonal bands: 35°N–60°N [top graph in each grouping] , 20°S–20°N [middle graph in each grouping], and 35°S–60°S [bottom graph in each grouping]. Anomalies are with respect to the 1998–2008 baseline. Colored lines correspond to different long-term satellite records. The black line is the merged ground-based dataset. The gray-shaded area shows the range of chemistry–climate model simulations from CCMI-1 refC2 (SPARC/IO3C/GAW 2019).
Figure credit: from the BAMS State of the Climate in 2023
Along with the caption, please include alternate keywords to include with the graphic. The alternative text does not appear with the article, but is added to the backend of website (i.e., Content Management System). The alt text aids in SEO. See the section on Search Engine Optimization for additional guidance.
Key word tag: A global map showing the locations of early adopter organizations.
If a figure or photo contain multiple elements, provide directionals in the caption to direction the reader to the different elements. The directionals should be italicized and in brackets. When referencing multiple Figures at once, use an en dash to separate the figure numbers.
For Example [in text]: After the presentation, the attendees heard from Karen St. Germain [NASA HQ—Director of NASA’s Earth Science Division], who gave inspiring remarks and answered questions for 15 minutes – see Photos 6–7.
For Example: Photos 6–7. Former NASA astronaut Paul Richards takes audience questions at the NASA Earth Day event. Credit: NASA
For Example: Figure 2. The Ghana Climate Hazards Center Coupled Model Intercomparison Project Phase 6 climate projection dataset map of temperatures exceeding 41 °C (106 °F) [left], future climate projection (SSP) for 2050 [middle], and the difference between the two [right]. Figure credit: Williams et al. 2024
Graphic/photo requirements
- Photos and graphics should be at least 1440 pixels wide. If the photo is small or low resolution, padding will be added to each side to fit the dimensions for the website.
- Provide high-resolution graphics source files of all graphics. Submit graphics and photos as a .gif, .tif, or .eps file.
- Do not resize photos or graphics.
- Submit raw data in plain text for tables. The Editorial Team will reconfigure the content into tables to insert on the EO website.
There are many style topics not specified here. As stated earlier, the NASA Stylebook and Communications Manual and AP Style Guide (in that order) should be followed when something is not explicitly described in this guide.
In addition, previous articles from The Earth Observer (particularly those from recent years) can serve as templates for future articles. It is a good idea when preparing to submit an article to look at some previous articles available in The Earth Observer archive.
The Earth Observer: Editorial Guidelines
Last Updated: 01/30/25
NASA Astronaut to Answer Questions from Students in Florida
Students from Dade City, Florida, will have the chance to connect with NASA astronaut Nichole Ayers as she answers prerecorded science, technology, engineering, and mathematics-related questions from aboard the International Space Station.
Watch the 20-minute space-to-Earth call at 1 p.m. EDT on Friday, April 11, on NASA+ and learn how to watch NASA content on various platforms, including social media.
The event, hosted by Academy at the Farm and open to students and their families, will occur in Dade City. Academy at the Farm is a charter school that plans to use the event to connect the students with space exploration and the work being done aboard the space station.
Media interested in covering the event must RSVP by 5 p.m., Wednesday, April 9, to Ashley Cantwell at acantwell@academyatthefarm.com or 813-957-8878.
For more than 24 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing skills needed to explore farther from Earth. Astronauts aboard the orbiting laboratory communicate with NASA’s Mission Control Center in Houston 24 hours a day through SCaN’s (Space Communications and Navigation) Near Space Network.
Important research and technology investigations taking place aboard the space station benefit people on Earth and lays the groundwork for other agency missions. As part of NASA’s Artemis campaign, the agency will send astronauts to the Moon to prepare for future human exploration of Mars; inspiring Artemis Generation explorers and ensuring the United States continues to lead in space exploration and discovery.
See videos and lesson plans highlighting space station research at:
https://www.nasa.gov/stemonstation
-end-
Gerelle Dodson
Headquarters, Washington
202-358-1600
gerelle.q.dodson@nasa.gov
Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov
Eclipses, Science, NASA Firsts: Heliophysics Big Year Highlights
7 min read
Eclipses, Science, NASA Firsts: Heliophysics Big Year HighlightsOne year ago today, a total solar eclipse swept across the United States. The event was a cornerstone moment in the Heliophysics Big Year, a global celebration of the Sun’s influence on Earth and the entire solar system. From October 2023 to December 2024 — a period encompassing two solar eclipses across the U.S., two new NASA heliophysics missions, and one spacecraft’s history-making solar flyby — NASA celebrated the Sun’s widespread influence on our lives.
An infographic showing key numbers summarizing the activities and events of the Heliophysics Big Year, which spanned from Oct. 14, 2023 – Dec. 24, 2024. NASA/Miles Hatfield/Kristen Perrin Annular Solar EclipseAn annular (or “ring of fire”) solar eclipse occurred Oct. 14, 2023, and kicked off the Helio Big Year with a bang. Millions of people across North America witnessed the Moon crossing in front of the Sun, creating this brilliant celestial event. NASA’s live broadcast had more than 11 million views across different platforms.
On Oct. 14, 2023, an annular solar eclipse crossed North, Central, and South America. Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere were able to experience this “ring of fire” eclipse. NASA’s official broadcast and outreach teams were located in Kerrville, TX, and Albuquerque, NM, to capture the event and celebrate with the communities in the path of annularity.Credit: NASA/Ryan Fitzgibbons
Before the eclipse, NASA introduced the 2023 Eclipse Explorer, an interactive map to explore eclipse details for any location in the United States. NASA shared tips on eclipse safety, including through a video with NSYNC’s Lance Bass and even with an augmented reality filter.
Scientists also studied conditions during the annular eclipse with sounding rockets, balloons, and amateur radio.
Total Solar EclipseOn April 8, 2024, millions of people across North America experienced a total solar eclipse that darkened parts of 15 U.S. states in the path of totality.
Ahead of the event, NASA hosted a widespread safety campaign, handed out over 2 million solar viewing glasses, and produced an interactive map to help viewers plan their viewing experience. On eclipse day, NASA also hosted a live broadcast from locations across the country, drawing over 38 million views.
Researchers studied the eclipse and its effects on Earth using a variety of techniques, including international radar networks, scientific rockets, weather balloons, and even high-altitude NASA WB-57 jets. Several NASA-funded citizen science projects also conducted experiments. These projects included more than 49,000 volunteers who contributed an astounding 53 million observations.
This infographic shares metrics from citizen science projects that occurred during the total solar eclipse on April 8, 2024.NASA/Kristen Perrin“We have opened a window for all Americans to discover our connection to the Sun and ignited enthusiasm for engaging with groundbreaking NASA science, whether it’s through spacecraft, rockets, balloons, or planes,” said Kelly Korreck, a Heliophysics program scientist at NASA Headquarters in Washington. “Sharing the excitement of NASA heliophysics with our fellow citizens has truly been amazing.”
Science Across the Solar SystemNASA’s heliophysics missions gather data on the Sun and its effects across the solar system.
The Atmospheric Waves Experiment (AWE) mission launched from NASA’s Kennedy Space Center in Florida Nov. 9, 2023, and was installed on the International Space Station nine days later. This mission studies atmospheric gravity waves, how they form and travel through Earth’s atmosphere, and their role in space weather.
Orbital footage from the International Space Station shows NASA’s Atmospheric Waves Experiment (AWE) as it was extracted from SpaceX’s Dragon cargo spacecraft.NASA/International Space StationOn Nov. 4, 2024, the Coronal Diagnostic Experiment (CODEX) mission also launched to the space station, where it studies the solar wind, with a focus on what heats it and propels it through space.
Pictured is the CODEX instrument inside the integration and testing facility at NASA’s Goddard Space Flight Center.NASA/CODEX teamThe Aeronomy of Ice in the Mesosphere (AIM) mission ended after 16 years studying Earth’s highest clouds, called polar mesospheric clouds.
An artist’s concept shows the Aeronomy of Ice in the Mesosphere (AIM) spacecraft orbiting Earth. NASA’s Goddard Space Flight/Center Conceptual Image LabNASA’s Ionospheric Connection Explorer (ICON) also ended after three successful years studying the outermost layer of Earth’s atmosphere, called the ionosphere.
NASA’s ICON, shown in this artist’s concept, studied the frontiers of space, the dynamic zone high in our atmosphere where terrestrial weather from below meets space weather above. NASA’s Goddard Space Flight Center/Conceptual Image LabVoyager has been operating for more than 47 years, continuing to study the heliosphere and interstellar space. In October 2024, the Voyager 1 probe stopped communicating. The mission team worked tirelessly to troubleshoot and ultimately reestablish communications, keeping the mission alive to continue its research.
In this artist’s conception, NASA’s Voyager 1 spacecraft has a bird’s-eye view of the solar system. The circles represent the orbits of the major outer planets: Jupiter, Saturn, Uranus, and Neptune. Launched in 1977, Voyager 1 visited the planets Jupiter and Saturn. The spacecraft is now 13 billion miles from Earth, making it the farthest and fastest-moving human-made object ever built. In fact, Voyager 1 is now zooming through interstellar space, the region between the stars that is filled with gas, dust, and material recycled from dying stars. NASA’s Hubble Space Telescope is observing the material along Voyager’s path through space.NASA/STSciWhile the goal of the NASA heliophysics fleet is to study the Sun and its influence, these missions often make surprising discoveries that they weren’t originally designed to. From finding 5,000 comets to studying the surface of Venus, NASA highlighted and celebrated these bonus science connections during the Helio Big Year.
Solar MaximumSimilar to Earth, the Sun has its own seasons of activity, with a solar minimum and solar maximum during a cycle that lasts about 11 years. The Helio Big Year happened to coincide with the Sun’s active period, with NASA and NOAA announcing in October 2024 that the Sun had reached solar maximum, the highest period of activity. Some of the largest solar storms on current record occurred in 2024, and the largest sunspot in nearly a decade was spotted in the spring of 2024, followed by a colossal X9.0 solar flare Oct. 3, 2024.
Sunspots are cooler, darker areas on the solar surface where the Sun’s magnetic field gets especially intense, often leading to explosive solar eruptions. This sunspot group was so big that nearly 14 Earths could fit inside it! The eruptions from this region resulted in the historic May 2024 geomagnetic storms, when the aurora borealis, or northern lights, were seen as far south as the Florida Keys.Credit: NASA/Beth Anthony
Viewers across the U.S. spotted auroras in their communities as a result of these storms, proving that you can capture amazing aurora photography without advanced equipment.
The Big Finale: Parker’s Close Approach to the SunNASA’s Parker Solar Probe holds the title as the closest human-made object to the Sun. On Dec. 24, 2024, Parker made history by traveling just 3.8 million miles from the Sun’s surface at a whopping 430,000 miles per hour.
“Flying this close to the Sun is a historic moment in humanity’s first mission to a star,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters.
Controllers have confirmed NASA’s mission to “touch” the Sun survived its record-breaking closest approach to the solar surface on Dec. 24, 2024.Credit: NASA/Joy Ng
Parker Solar Probe’s close approach capped off a momentous Heliophysics Big Year that allowed NASA scientists to gather unprecedented data and invited everyone to celebrate how the Sun impacts us all. In the growing field of heliophysics, the Helio Big Year reminded us all how the Sun touches everything and how important it is to continue studying our star’s incredible influence.
A Big Year AheadThough the Helio Big Year is over, heliophysics is only picking up its pace in 2025. We remain in the solar maximum phase, so heightened solar activity will continue into the near future. In addition, several new missions are expected to join the heliophysics fleet by year’s end.
The PUNCH mission, a set of four Sun-watching satellites imaging solar eruptions in three dimensions, and EZIE, a trio of Earth-orbiting satellites tracing the electrical currents powering Earth’s auroras, have already launched. The LEXI instrument, an X-ray telescope studying Earth’s magnetosphere from the Moon, also launched through NASA’s CLPS (Commercial Lunar Payload Services) initiative.
Future missions slated for launch include TRACERS, which will investigate the unusual magnetic environment near Earth’s poles, and ESCAPADE, venturing to Mars to measure the planet’s unique magnetic environment.
The last two missions will share a ride to space. The Carruthers Geocorona Observatory will look back at home, studying ultraviolet light emitted by the outermost boundaries of our planet’s atmosphere. The IMAP mission will instead look to the outermost edges of our heliosphere, mapping the boundaries where the domain of our Sun transitions into interstellar space.
By Desiree Apodaca
NASA’s Goddard Space Flight Center
Missions
Humans in Space
Climate Change
Solar System
