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NASA Interns Blast Off for Their First Week at Goddard
Several hundred new faces walked through the gates of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the first time on June 3. Who is this small army of motivated space-enthusiasts? It’s Goddard’s 2024 summer intern cohort.
Across Goddard’s campuses, more than 300 on-site and virtual interns spend the 10-week program contributing across all manners of disciplines, science, engineering, finance, communications, and many more. From helping engineers who will send new space telescopes into orbit, to communicating NASA’s scientific discoveries to the world, this cohort of interns hopes to bring their new ideas and perspectives to Goddard this summer.
About 200 interns attended summer orientation at Goddard’s Greenbelt, Maryland, campus of NASA’s Goddard Space Flight Center, on June 3, 2024. This was the first in-person summer orientation since 2019.Credit: NASA/Jimmy Acevedo The Artemis Generation Takes FlightThis group of interns is part of the Artemis Generation: they come to NASA near the culmination of the campaign that will return humanity to the Moon for the first time in more than 50 years. Through Artemis, NASA will land the first woman and first person of color on the lunar surface.
“I’m just excited to contribute to Artemis,” said Kate Oberlander, who just graduated from UCLA in aerospace engineering. “We’ll be helping connect communications between the Moon and Earth for the Artemis campaign, and that is so monumental. That’s exciting to be a part of.”
In addition to work on their projects, interns also have networking opportunities where they can meet current NASA employees and learn about careers in aerospace.
“I’ve been really enjoying getting to know my fellow interns, and also getting that professional development alongside technical skills,” said Oberlander, who plans on returning to UCLA to earn her master’s degree and learn more about optics, electromagnetics, and space exploration. She said her internship this summer will bring all her favorite subjects together.
Down to Earth: Interns Work Across FieldsInterns at Goddard take on a diverse set of projects across many disciplines. “It’s a lot of learning — but I love learning. I’m like a sponge,” said Addie Colwell, an environmental science student at the University of Vermont.
Colwell’s internship focuses on stormwater management at Goddard. “We have to renovate the embankment of the stormwater pond,” Colwell said. “I’m assessing how that’s going to impact the wildlife there. It’s a lot of species identification and research.”
Emma Stefanacci, a science communication master’s student at the University of Wisconsin, Madison, will be working on the astrophysics social media team.
“I’m excited to see what social media looks like, as I haven’t been able to play in that realm of communications before,” said Stefanacci. She will help develop a campaign for the launch anniversary of XRISM, a telescope collaboration between NASA and the Japan Aerospace Exploration Agency (JAXA).
This summer, NASA’s Wallops Flight Facility on Virginia’s Eastern Shore also hosts a diverse intern cohort, some of whom are shown here in the Range Control Center. Goddard manages Wallops on behalf of NASA.Credit: NASA/Pat Benner Working on the Next Generation of Space DiscoveryKevin Mora is a student at Arizona State University studying computer science. Mora is working on several projects this summer, one of them focusing on pipeline coding in Python to help engineers working on the Nancy Grace Roman Space Telescope. “It’s literally like a pipeline — just moving data from here to there,” Mora said. “It helps the engineers that are building Roman get stuff done faster.”
The Roman Space Telescope is the next in line to carry on the Hubble and Webb legacy. Roman will have a much wider field of view than the space telescopes preceding it, giving scientists a bigger picture of the universe, and hopefully telling us more about dark matter and dark energy. Many interns are working on this space telescope, which is expected to launch by 2027.
Alongside new faces in this year’s program, some interns are returning to NASA for repeat sessions. Cord Mazzetti, a recent electrical engineering graduate of the University of Texas at Austin, will be continuing work on quantum clock synchronization that he began researching at Goddard last summer.
“It’s nice to be back here at NASA and to be able to dive into my work even faster,” said Mazzetti.
In-person Orientation Returns to CampusThe interns’ orientation was the first to be held in-person since before the COVID-19 pandemic, according to Laura Schmidt, an internships specialist in NASA’s Office of STEM Engagement.
“It was thrilling to welcome our incredible group of interns and host our first onsite summer orientation in five years,” Schmidt said. “The energy was palpable as we welcomed nearly 200 interns onsite at Goddard, and I have no doubt that the stage is set for a fantastic summer ahead.”
By Avery Truman and Matthew Kaufman
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Share Details Last Updated Jun 17, 2024 EditorKaty MersmannContactRob Garnerrob.garner@nasa.govLocationGoddard Space Flight Center Related TermsNASA Satellites Find Snow Didn’t Offset Southwest US Groundwater Loss
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Despite some years with significant snowfalls, long-term drought conditions in the Great Basin region of Nevada, California, Arizona, and Utah, along with increasing water demands, have strained water reserves in the western U.S. As a result, inland bodies of water, including the Great Salt Lake pictured here, have shrunk dramatically, exposing lakebeds that may release toxic dust when dried.Dorothy Hall/University of MarylandRecord snowfall in recent years has not been enough to offset long-term drying conditions and increasing groundwater demands in the U.S. Southwest, according to a new analysis of NASA satellite data.
Declining water levels in the Great Salt Lake and Lake Mead have been testaments to a megadrought afflicting western North America since 2000. But surface water only accounts for a fraction of the Great Basin watershed that covers most of Nevada and large portions of California, Utah, and Oregon. Far more of the region’s water is underground. That has historically made it difficult to track the impact of droughts on the overall water content of the Great Basin.
A new look at 20 years of data from the Gravity Recovery and Climate Experiment (GRACE) series of satellites shows that the decline in groundwater in the Great Basin far exceeds stark surface water losses. Over about the past two decades, the underground water supply in the basin has fallen by 16.5 cubic miles (68.7 cubic kilometers). That’s roughly two-thirds as much water as the entire state of California uses in a year and about six times the total volume of water that was left in Lake Mead, the nation’s largest reservoir, at the end of 2023.
While new maps show a seasonal rise in water each spring due to melting snow from higher elevations, University of Maryland earth scientist Dorothy Hall said occasional snowy winters are unlikely to stop the dramatic water level decline that’s been underway in the U.S. Southwest.
The finding came about as Hall and colleagues studied the contribution of annual snowmelt to Great Basin water levels. “In years like the 2022-23 winter, I expected that the record amount of snowfall would really help to replenish the groundwater supply,” Hall said. “But overall, the decline continued.” The research was published in March 2024 in the journal Geophysical Research Letters.
“A major reason for the decline is the upstream water diversion for agriculture and households,” Hall said. Populations in the states that rely on Great Basin water supplies have grown by 6% to 18% since 2010, according to the U.S. Census Bureau. “As the population increases, so does water use.”
Runoff, increased evaporation, and water needs of plants suffering hot, dry conditions in the region are amplifying the problem. “With the ongoing threat of drought,” Hall said, “farmers downstream often can’t get enough water.”
Gravity measurements from the GRACE series of satellites show that the decline in water levels in the Great Basin region from April 2002 to September 2023 has most severely affected portions of southern California (indicated in red).D.K. Hall et al./Geophysical Research Letters 2024While measurements of the water table in the Great Basin — including the depths required to connect wells to depleted aquifers — have hinted at declining groundwater, data from the joint German DLR-NASA GRACE missions provide a clearer picture of the total loss of water supply in the region. The original GRACE satellites, which flew from March 2002 to October 2017, and the successor GRACE–Follow On (GRACE–FO) satellites, which launched in May 2018 and are still active, track changes in Earth’s gravity due primarily to shifting water mass.
GRACE-based maps of fluctuating water levels have improved recently as the team has learned to parse more and finer details from the dataset. “Improved spatial resolution helped in this study to distinguish the location of the mass trends in the Western U.S. roughly ten times better than prior analyses,” said Bryant Loomis, who leads GRACE data analysis at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The diminishing water supplies of the U.S. Southwest could have consequences for both humans and wildlife, Hall said. In addition to affecting municipal water supplies and limiting agricultural irrigation, “It exposes the lake beds, which often harbor toxic minerals from agricultural runoff, waste, and anything else that ends up in the lakes.”
In Utah, a century of industrial chemicals accumulated in the Great Salt Lake, along with airborne pollutants from present-day mining and oil refinement, have settled in the water. The result is a hazardous muck that is uncovered and dried as the lake shrinks. Dust blown from dry lake beds, in turn, exacerbates air pollution in the region. Meanwhile, shrinking lakes are putting a strain on bird populations that rely on the lakes as stopovers during migration.
According to the new findings, Hall said, “The ultimate solution will have to include wiser water management.”
By James R. Riordon
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Scientists have predicted that droughts, floods will become more frequent and severe as our planet…
Article 1 year ago 9 min read Drought Makes its Home on the Range Article 3 years agoSlow Your Student’s ‘Summer Slide’ and Beat Boredom With NASA STEM
The school year has come to an end, and those long summer days are stretching ahead like an open runway. Parents and educators often worry about the “summer slide,” the concept that students may lose academic ground while out of school. But summer doesn’t mean students’ imaginations have to stay grounded!
Are you hoping to slow the summer slide or simply to beat back boredom with some fun options that will also keep young minds active? NASA’s Office of STEM Engagement has pulled together this collection of hands-on activities and interesting resources to set students up for a stellar summer vacation. Read on for ways to keep students entertained and engaged, from learning about NASA’s exciting missions, to exploring the world, to making some out-of-this-world art and more.
Take NASA With You on Summer VacationWhether you’re whiling away the hours on a quiet summer day or setting out on a travel adventure, NASA offers fun resources for young explorers to learn while passing the time.
Prepare for air travel with the Four Forces of Flight, a set of four activities explaining the forces that make airplanes work, and NASA’s Junior Pilot Program, in which Orville the flying squirrel teaches youngsters about sustainable aviation that’s making airplanes safer and faster. Students can also learn about NASA’s X-59 experimental aircraft, which will fly faster than the speed of sound while reducing the sound of sonic booms to mere “sonic thumps,” and the whole family can sign up as virtual passengers on NASA’s upcoming flights through the NASA Flight Log.
Traveling to somewhere new? Astronauts living and working in low Earth orbit take many photographs of Earth as it rotates. Explore the world using the Explore Astronaut Photography interactive map, or test geography knowledge through the “Where in the World” Expedition I and Expedition II interactive quizzes.
Of course, some kids prefer to kick back with a good book while on the couch, at the beach, in the backseat, or on a plane – and NASA is ready with reading material! Kids aged 3 to 8 can learn about the Space Launch System (SLS) rocket that will return humans to the Moon with the “Hooray for SLS” children’s book and related activities. Students of all ages are invited to take their imaginations on a lunar adventure with fictional astronaut Callie Rodriguez through the First Woman graphic novel series.
Blast Boredom With STEM Crafts and CreativityMaking, baking, coloring, or drawing – there are plenty of ways to keep kids’ artistic abilities engaged while learning.
Students can download and create their own Artemis illustrations through Learn How to Draw Artemis, featuring the SLS rocket and Orion spacecraft, and younger kids can learn the ABCs of human spaceflight with the Commercial Crew A to Z Activity and Coloring Booklet. Learn about the search for life in the universe while getting creative and colorful with Astrobiology Coloring and Drawing Pages.
If crafts are more appealing, create and launch a soda-straw rocket and use printable templates to build a model of the Orion spacecraft or the Parker Solar Probe. Kids can even create a sundial and use the Sun to tell time on a sunny day.
Finally, summer isn’t complete without a sweet treat, so bake some sunspot cookies. Real sunspots are not made of chocolate, but in this recipe, they are!
Hungry for More?Don’t let the summer doldrums get you down. NASA STEM offers an entire universe of activities, resources, and opportunities for STEM fans at a variety of grade levels. Check out the NASA STEM Search and discover more NASA STEM categories below.
Explore the NASA STEM Search Now Keep Exploring Discover More Topics From NASAFor Students Grades K-4
For Students Grades 5-8
For Students Grades 9-12
Learning Resources
Investigating the Origins of the Crab Nebula With NASA’s Webb
New data revises our view of this unusual supernova explosion.
A team of scientists used NASA’s James Webb Space Telescope to parse the composition of the Crab Nebula, a supernova remnant located 6,500 light-years away in the constellation Taurus. With the telescope’s MIRI (Mid-Infrared Instrument) and NIRCam (Near-Infrared Camera), the team gathered data that is helping to clarify the Crab Nebula’s history.
The Crab Nebula is the result of a core-collapse supernova from the death of a massive star. The supernova explosion itself was seen on Earth in 1054 CE and was bright enough to view during the daytime. The much fainter remnant observed today is an expanding shell of gas and dust, and outflowing wind powered by a pulsar, a rapidly spinning and highly magnetized neutron star.
The Crab Nebula is also highly unusual. Its atypical composition and very low explosion energy previously have been explained by an electron-capture supernova — a rare type of explosion that arises from a star with a less-evolved core made of oxygen, neon, and magnesium, rather than a more typical iron core.
“Now the Webb data widen the possible interpretations,” said Tea Temim, lead author of the study at Princeton University in New Jersey. “The composition of the gas no longer requires an electron-capture explosion, but could also be explained by a weak iron core-collapse supernova.”
Image A: Crab Nebula (NIRCam and MIRI) This image by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument) shows different structural details of the Crab Nebula. The supernova remnant is comprised of several different components, including doubly ionized sulfur (represented in green), warm dust (magenta), and synchrotron emission (blue). Yellow-white mottled filaments within the Crab’s interior represent areas where dust and doubly ionized sulfur coincide. The observations were taken as part of General Observer program 1714. Studying the Present to Understand the PastPast research efforts have calculated the total kinetic energy of the explosion based on the quantity and velocities of the present-day ejecta. Astronomers deduced that the nature of the explosion was one of relatively low energy (less than one-tenth that of a normal supernova), and the progenitor star’s mass was in the range of eight to 10 solar masses — teetering on the thin line between stars that experience a violent supernova death and those that do not.
However, inconsistencies exist between the electron-capture supernova theory and observations of the Crab, particularly the observed rapid motion of the pulsar. In recent years, astronomers have also improved their understanding of iron core-collapse supernovae and now think that this type can also produce low-energy explosions, providing that the stellar mass is adequately low.
Webb Measurements Reconcile Historic ResultsTo lower the level of uncertainty surrounding the Crab’s progenitor star and nature of the explosion, the team led by Temim used Webb’s spectroscopic capabilities to hone in on two areas located within the Crab’s inner filaments.
Theories predict that because of the different chemical composition of the core in an electron-capture supernova, the nickel to iron (Ni/Fe) abundance ratio should be much higher than the ratio measured in our Sun (which contains these elements from previous generations of stars). Studies in the late 1980s and early 1990s measured the Ni/Fe ratio within the Crab using optical and near-infrared data and noted a high Ni/Fe abundance ratio that seemed to favor the electron-capture supernova scenario.
The Webb telescope, with its sensitive infrared capabilities, is now advancing Crab Nebula research. The team used MIRI’s spectroscopic abilities to measure the nickel and iron emission lines, resulting in a more reliable estimate of the Ni/Fe abundance ratio. They found that the ratio was still elevated compared to the Sun, but only modestly and much lower in comparison to prior estimates.
The revised values are consistent with electron-capture, but do not rule out an iron core-collapse explosion from a similarly low-mass star. (Higher-energy explosions from higher-mass stars are expected to produce ratios closer to solar abundances.) Further observational and theoretical work will be needed to distinguish between these two possibilities.
“At present, the spectral data from Webb covers two small regions of the Crab, so it’s important to study much more of the remnant and identify any spatial variations,” said Martin Laming of the Naval Research Laboratory in Washington and a co-author of the paper. “It would be interesting to see if we could identify emission lines from other elements, like cobalt or germanium.”
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Besides pulling spectral data from two small regions of the Crab Nebula’s interior to measure the abundance ratio, the telescope also observed the remnant’s broader environment to understand details of the synchrotron emission and the dust distribution.
The images and data collected by MIRI enabled the team to isolate the dust emission within the Crab and map it in high resolution for the first time. By mapping the warm dust emission with Webb, and even combining it with the Herschel Space Observatory’s data on cooler dust grains, the team created a well-rounded picture of the dust distribution: The outermost filaments contain relatively warmer dust, while cooler grains are prevalent near the center.
“Where dust is seen in the Crab is interesting because it differs from other supernova remnants, like Cassiopeia A and Supernova 1987A,” said Nathan Smith of the Steward Observatory at the University of Arizona and a co-author of the paper. “In those objects, the dust is in the very center. In the Crab, the dust is found in the dense filaments of the outer shell. The Crab Nebula lives up to a tradition in astronomy: The nearest, brightest, and best-studied objects tend to be bizarre.”
These findings have been accepted for publication in The Astrophysical Journal Letters.
The observations were taken as part of General Observer program 1714.
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).
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These findings have been accepted for publication in The Astrophysical Journal Letters.
Media ContactsLaura Betz – laura.e.betz@nasa.gov, Rob Gutro – rob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Abigail Major – amajor@stsci.edu / Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Infographic: Massive Stars: Engines of Creation
Articles: Explore Other Webb Supernova Articles
3D visualization video : “Crab Nebula: The Multiwavelength Structure of a Pulsar Wind Nebula”
Sonification: Multiwavelength image of the Crab Nebula
Explore More: Crab Nebula resources from NASA’s Universe of Learning
Related For KidsInteractive: Explore the Crab Nebula in multiple wavelengths
Activity: Create a stellar life cycle bookmark and bracelet
Activity: Flipbook resource for stellar evolution
En Español Keep Exploring Related Topics James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
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Share Details Last Updated Jun 17, 2024 Editor Stephen Sabia Contact Laura Betz laura.e.betz@nasa.gov Related Terms
Globetrotting NASA Research Model Increases Accuracy
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The NASA 5.2% scale, semi-span version of the High Lift Common Research Model installed in the German-Dutch Wind Tunnels – Braunschweig Low-Speed Wind Tunnel in Braunschweig, Germany on May 4, 2023. NASANASA and its international partners are using the same generically shaped wing design to create physical and digital research models to better understand how air moves around an aircraft during takeoff and landing.
Various organizations are doing computer modeling with computational tools and conducting wind tunnel tests using the same High Lift Common Research Model (CRM-HL), a NASA-led effort.
This ensures the aerospace community is getting accurate answers despite any differences in testing conditions or facilities.
What started as a voluntary partnership in 2019 has grown into the CRM-HL ecosystem with 10 partners across five countries. The team is building eight wind tunnel models, which will be tested at eight wind tunnels during the next three years.
What we are learning today would take us 10 years to do alone. The partners are using each other’s research for the mutual benefit of all.Melissa Rivers
NASA Researcher
“What we are learning today would take us 10 years to do alone,” said Melissa Rivers, subproject manager in NASA’s Transformational Tools and Technologies project, which leads the CRM-HL research. “The partners are using each other’s research for the mutual benefit of all.”
The team will define and assess common wind tunnel conditions in more than 14 tests across the globe.
“Through this research, we are learning about differences that occur when we build and test several identical airplane models in multiple wind tunnels,” Rivers said.
Researchers can use data from these wind tunnel tests to then check if the research tools using computational fluid dynamics are accurately predicting the physics of an aircraft.
“The computer simulations and computational fluid dynamics tools are key contributions from this international partnership,” said NASA’s Mujeeb Malik, a lead researcher for the project. “The runs [tests] are critical to figuring out what we do not know and determining what we want to test.”
The partners are developing a standard way to communicate their data so that everyone can better compare the results from their models and wind tunnel tests.
NASA also is developing a cloud-based solution to give each partner access to the data and foster collaboration.
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This silent, 20-second video shows a computer simulation of air flowing over a 5.2% scale of NASA's High Lift Common Research Model wing design. The color key at lower right indicates the speed of the air.NASA Expanding Collaborations with Common Research ModelsThis high lift research effort builds on the success of a previous Common Research Model effort focused on transonic speeds.
Between 2008 and 2014, many organizations built their own versions of NASA’s model. They then tested the models in tunnels around the world.
The transonic model helped the community better understand the physics of aircraft at cruise. The current high lift model focuses on the takeoff and landing portions of flight when the aircraft is flying slower than at cruise.
Since there are more wind tunnels that can run low-speed tests, more partners can participate in the current collaboration.
The partners working on the CRM-HL span five countries – United States, United Kingdom, France, Germany, and Japan and include:
- NASA
- German Aerospace Center
- National Office for Aerospace Studies and Research, the French Aerospace Lab
- JAXA (Japan Aerospace Exploration Agency)
- European Transonic Wind Tunnel
- Aerospace Technology Institute
- Boeing
- Kawasaki Heavy Industries
- QinetiQ
- Airbus
Data from the CRM-HL research effort also are driving NASA’s High Lift Prediction Workshop series. The series is sponsored by the Applied Aerodynamics Technical Committee of the American Institute of Aeronautics and Astronautics.
The workshops are intended to engage the broader aviation community in these efforts and inspire researchers around the world.
Another goal of this research is to help realize Certification by Analysis, which supports key objectives of the NASA Computational Fluid Dynamics Vision 2030 Study.
NASA, industry, and academia developed the study to lay out a long-term plan for developing future computational capabilities and meeting software and hardware needs for computational fluid dynamics.
The aerospace community will require these resources to efficiently makeaccurate predictions of how air moves around an aircraft. This work also informs the analysis and design of aircraft.
Certification by Analysis would significantly reduce the amount of flight tests required for an aircraft or engine to meet the requirements for airworthiness.
This could save aircraft development programs time and millions of dollars. It could also improve product safety and performance.
The Federal Aviation Administration (FAA) sets the requirements for airworthiness. Companies must provide test results to show new aircraft and engines meet the regulations.
“Before the FAA would allow this type of certification, the analysis must be as accurate as flight testing,” said Rivers.
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Share Details Last Updated Jun 15, 2024 EditorJim BankeContactDiana Fitzgeralddiana.r.fitzgerald@nasa.gov Related TermsTropical Solstice Shadows
Solstices mark the changing of seasons, occur twice a year, and feature the year’s shortest and longest daylight hours – depending on your hemisphere. These extremes in the length of day and night make solstice days more noticeable to many observers than the subtle equality of day and night experienced during equinoxes. Solstices were some of our earliest astronomical observations, celebrated throughout history via many summer and winter celebrations.
Solstices occur twice yearly, and in 2024 they arrive on June 20 at 4:50 PM EDT (20:50 UTC), and December 21 at 4:19 AM EST (9:18 UTC). The June solstice marks the moment when the Sun is at its northernmost position in relation to Earth’s equator, and the December solstice marks its southernmost position. The summer solstice occurs on the day when the Sun reaches its highest point at solar noon for regions outside of the tropics, and those observers experience the longest amount of daylight for the year. Conversely, during the winter solstice, the Sun is at its lowest point at solar noon for the year and observers outside of the tropics experience the least amount of daylight- and the longest night – of the year.
The June solstice marks the beginning of summer for folks in the Northern Hemisphere and winter for Southern Hemisphere folks, and in December the opposite is true, as a result of the tilt of Earth’s axis of rotation. For example, this means that the Northern Hemisphere receives more direct light from the Sun than the Southern Hemisphere during the June solstice. Earth’s tilt is enough that northern polar regions experience 24-hour sunlight during the June solstice, while southern polar regions experience 24-hour night, deep in Earth’s shadow. That same tilt means that the Earth’s polar regions also experience a reversal of light and shadow half a year later in December, with 24 hours of night in the north and 24 hours of daylight in the south. Depending on how close you are to the poles, these extreme lighting conditions can last for many months, their duration deepening the closer you are to the poles.
A presenter from the San Antonio Astronomy Club in Puerto Rico demonstrating some Earth-Sun geometry to a group during a “Zero Shadow Day” event. As Puerto Rico lies a few degrees south of the Tropic of Cancer, their two zero shadow days arrive just a few weeks before and after the June solstice. Globes are a handy and practical way to help visualize solstices and equinoxes for large outdoor groups, especially outdoors during sunny days!Credit: Juan Velázquez / San Antonio Astronomy ClubWhile solstice days are very noticeable to observers in mid to high latitudes, that’s not the case for observers in the tropics – areas of Earth found between the Tropic of Cancer and the Tropic of Capricorn. Instead, individuals experience two “zero shadow” days per year. These days, with the sun directly overhead at solar noon, objects cast a minimal shadow compared to the rest of the year. If you want to see your own shadow at that moment, you have to jump! The exact date for zero shadow days depends on latitude; observers on the Tropic of Cancer (23.5° north of the equator) experience a zero-shadow day on the June solstice, and observers on the Tropic of Capricorn (23.5° south of the equator) get their zero-shadow day on December’s solstice. Observers on the equator experience two zero shadow days, being exactly in between these two lines of latitude; equatorial zero shadow days fall on the March and September equinoxes.
There is some serious science that can be done by carefully observing solstice shadows. In approximately 200 BC, Eratosthenes is said to have observed sunlight shining straight down the shaft of a well during high noon on the solstice, near the modern-day Egyptian city of Aswan. Inspired, he compared measurements of solstice shadows between that location and measurements taken north, in the city of Alexandria. By calculating the difference in the lengths of these shadows, along with the distance between the two cities, Eratosthenes calculated a rough early estimate for the circumference of Earth – and also provided further evidence that the Earth is a sphere!
Are you having difficulty visualizing solstice lighting and geometry? You can build a Suntrack model that helps demonstrate the path the Sun takes through the sky during the seasons. You can find more fun activities and resources like this model on NASA’s Wavelength and Energy activity.
Originally posted by Dave Prosper: June 2022
Last Updated by Kat Troche: April 2024
Simplified SummaryThe June solstice happens when the Sun is farthest north from the equator, and the December solstice is when it’s farthest south. During the June one, places outside the tropics have the longest day of the year, and during December’s, they have the shortest. In the Northern Hemisphere, June marks the start of summer, while in the Southern Hemisphere, it’s winter, and it’s the opposite in December. This happens because of the axis on which Earth leans. Because of this tilt, places near the North Pole have continuous daylight in June, while places near the South Pole have continuous darkness. In December, it’s the other way around. This goes on for months, depending on how close you are to the poles. People in the tropics, between the Tropic of Cancer and the Tropic of Capricorn, don’t see as big of a change in daylight. Instead, they have two days a year where shadows almost disappear because the Sun is directly overhead at noon. If you want to see your shadow, you have to jump! The exact days depend on where you are. Around 200 BC, Eratosthenes noticed the Sun was directly overhead on the solstice in one place, comparing that to another place where it wasn’t overhead, and was able to calculate Earth’s size and shape.
NASA, Boeing to Discuss Starliner’s Mission
NASA and Boeing will discuss Starliner’s mission and departure from the International Space Station as part of the agency’s Boeing Crew Flight Test in a pre-departure media teleconference at 12 p.m. EDT Tuesday, June 18.
NASA, Boeing, and station management teams will evaluate mission requirements and weather conditions at available landing locations in the southwestern U.S. before committing to the spacecraft’s departure from the orbiting laboratory.
Participants in the news conference include:
- Steve Stich, manager, NASA’s Commercial Crew Program
- Dana Weigel, manager, NASA’s International Space Station Program
- Mike Lammers, flight director, NASA’s Johnson Space Center in Houston
- Mark Nappi, vice president and program manager, Commercial Crew Program, Boeing
Media interested in participating must contact the NASA Johnson newsroom no later than 10 a.m., June 18, at 281-483-5111 or jsccommu@mail.nasa.gov. To ask questions, media must dial into the teleconference no later than 15 minutes before the start of the event.
Audio of the teleconference will stream live on NASA’s website at:
As part of NASA’s Commercial Crew Program, NASA astronauts Butch Wilmore and Suni Williams lifted off at 10:52 a.m., June 5, on a United Launch Alliance Atlas V rocket from Space Launch Complex-41 at Cape Canaveral Space Force Station in Florida on an end-to-end test of the Starliner system. The crew docked to the forward-facing port of the station’s Harmony module at 1:34 p.m., June 6.
For NASA’s blog and more information about the mission, visit:
https://www.nasa.gov/commercialcrew
-end-
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Johnson Space Center, Houston
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NASA Announces Winners of 2024 Student Launch Competition
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) High school and collegiate student teams gathered just north of NASA’s Marshall Space Flight Center in Huntsville, Alabama, to participate in the agency’s annual Student Launch competition April 13. Credits: NASA/Charles BeasonOver 1,000 students from across the U.S. and Puerto Rico launched high-powered, amateur rockets on April 13, just north of NASA’s Marshall Space Flight Center in Huntsville, Alabama, as part of the agency’s annual Student Launch competition.
Teams of middle school, high school, college, and university students were tasked to design, build, and launch a rocket and scientific payload to an altitude between 4,000 and 6,000 feet, while making a successful landing and executing a scientific or engineering payload mission.
“These bright students rise to a nine-month challenge that tests their skills in engineering, design, and teamwork,” said Kevin McGhaw, director of NASA’s Office of STEM Engagement Southeast Region. “They are the Artemis Generation, the future scientists, engineers, and innovators who will lead us into the future of space exploration.”
NASA announced the University of Notre Dame is the overall winner of the agency’s 2024 Student Launch challenge, followed by Iowa State University, and the University of North Carolina at Charlotte. A complete list challenge winners can be found on the agency’s student launch web page.
Each year NASA implements a new payload challenge to reflect relevant missions. This year’s payload challenge is inspired by the Artemis missions, which seek to land the first woman and first person of color on the Moon.
The complete list of award winners are as follows:
2024 Overall Winners
- First place: University of Notre Dame, Indiana
- Second place: Iowa State University, Ames
- Third place: University of North Carolina at Charlotte
3D Printing Award:
College Level:
- First place: University of Tennessee Chattanooga
Middle/High School Level:
- First place: First Baptist Church of Manchester, Manchester, Connecticut
Altitude Award
College Level:
- First place: Iowa State University, Ames
Middle/High School Level:
- First place: Morris County 4-H, Califon, New Jersey
Best-Looking Rocket Award:
College Level:
- First place: New York University, Brooklyn, New York
Middle/High School Level:
- First place: Notre Dame Academy High School, Los Angeles
American Institute of Aeronautics and Astronautics Reusable Launch Vehicle Innovative Payload Award:
College Level:
- First place: University of Colorado Boulder
- Second place: Vanderbilt University, Nashville, Tennessee
- Third place: Carnegie Mellon, Pittsburgh, Pennsylvania
Judge’s Choice Award:
Middle/High School Level:
- First place: Cedar Falls High School, Cedar Falls, Iowa
- Second place: Young Engineers in Action, LaPalma, California
- Third place: First Baptist Church of Manchester, Manchester, Connecticut
Project Review Award:
College Level:
- First place: University of Florida, Gainesville
AIAA Reusable Launch Vehicle Award:
College Level:
- First place: University of Florida, Gainesville
- Second place: University of North Carolina at Charlotte
- Third place: University of Notre Dame, Indiana
AIAA Rookie Award:
College Level:
- First place: University of Colorado Boulder
Safety Award:
College Level:
- First place: University of Notre Dame, Indiana
- Second place: University of Florida, Gainesville
- Third place: University of North Carolina at Charlotte
Social Media Award:
College Level:
- First place: University of Colorado Boulder
Middle/High School Level:
- First place: Newark Memorial High School, Newark, California
STEM Engagement Award:
College Level:
- First place: University of Notre Dame, Indiana
- Second place: University of North Carolina at Charlotte
- Third place: New York University, Brooklyn, New York
Middle/High School Level:
- First place: Notre Dame Academy High School, Los Angeles, California
- Second place: Cedar Falls High School, Cedar Falls, Iowa
- Third place: Thomas Jefferson High School for Science and Technology, Alexandria, Virginia
Service Academy Award:
First place: United States Air Force Academy, USAF Academy, Colorado
Vehicle Design Award:
Middle/High School Level:
- First place: First Baptist Church of Manchester, Manchester, Connecticut
- Second place: Explorer Post 1010, Rockville, Maryland
- Third place: Plantation High School, Plantation, Florida
Payload Design Award:
Middle/High School Level:
- First place: Young Engineers in Action, LaPalma, California
- Second place: Cedar Falls High School, Cedar Falls, Iowa
- Third place: Spring Grove Area High School, Spring Grove, Pennsylvania
Student Launch is one of NASA’s nine Artemis Student Challenges, activities which connect student ingenuity with NASA’s work returning to the Moon under Artemis in preparation for human exploration of Mars.
The competition is managed by Marshall’s Office of STEM Engagement (OSTEM). Additional funding and support are provided by NASA’s OSTEM via the Next Gen STEM project, NASA’s Space Operations Mission Directorate, Northrup Grumman, National Space Club Huntsville, American Institute of Aeronautics and Astronautics, National Association of Rocketry, Relativity Space, and Bastion Technologies.
To watch the full virtual awards ceremony, please visit NASA Marshall’s YouTube channel.
For more information about Student Launch, visit:
https://www.nasa.gov/stem/studentlaunch/home/index.html
For more information about other NASA challenges, please visit:
https://stem.nasa.gov/artemis/
Taylor Goodwin
Marshall Space Flight Center, Huntsville, Ala.
256.544.0034
taylor.goodwin@nasa.gov
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NASA Joins National Space Council in Celebration of Black Space Week
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Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA astronaut and Expedition 64 Flight Engineer Victor Glover reviews procedures on a computer for the Monoclonal Antibodies Protein Crystal Growth (PCG) experiment inside the Harmony module.Each year, Black Space Week celebrates the achievements of Black Americans in space-related fields.
To kick-off Black Space Week 2024, NASA is collaborating with the National Space Council for the Beyond the Color Lines: From Science Fiction to Science Fact forum on Monday, June 17, at 11:30 a.m. EDT at the National Museum of African American History and Culture in Washington.
Participants include Mr. Chirag Parikh, Deputy Assistant to the President and Executive Director, National Space Council; Dr. Quincy Brown, Director of Space STEM and Workforce Policy, White House National Space Council; and other private-sector and government agency leadership.
Current and former NASA astronauts will join the Standing on the Shoulders of Giants panel to discuss the past, present, and future of space exploration. The panel will be moderated by the Honorable Charles F. Bolden Jr., former administrator of NASA and a former astronaut who flew on four Space Shuttle missions. Participants include:
- Victor J. Glover, Jr., NASA Astronaut and U.S. Navy Captain
- Jessica Watkins, NASA Astronaut
- Yvonne Cagle, NASA Astronaut
- Leland Melvin, former NASA Astronaut
- Joan Higginbotham, former NASA Astronaut
Additional panels include HERStory, sharing the untold stories of Black women leaders in space, STEM, arts, diplomacy, and business, and a discussion with young leaders, educators, and scientists about education and career paths for the future of space.
Additional event details, including registration and streaming information, can be found at nmaahc.si.edu.
NASA to Discuss Outcome of 5th Biennial Asteroid Threat Exercise
NASA will host a virtual media briefing at 3:30 p.m. EDT, Thursday, June 20, to discuss a new summary of a recent tabletop exercise to simulate national and international responses to a hypothetical asteroid impact threat.
The fifth biennial Planetary Defense Interagency Tabletop Exercise was held April 2 and 3, 2024, at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland.
NASA’s Planetary Defense Coordination Office, in partnership with FEMA (Federal Emergency Management Agency) and with the assistance of the U.S. Department of State Office of Space Affairs, convened the tabletop exercise to inform and assess our ability as a nation to respond effectively to the threat of a potentially hazardous asteroid or comet. This exercise supports NASA’s planetary defense strategy to protect our planet and continues the agency’s mission to innovate for the benefit of humanity.
Video of the briefing will stream live on NASA TV and NASA’s YouTube channel.
The following participants will review the history and purpose of the exercise, the scenario encountered during this year’s simulation, and its findings and recommendations:
- Lindley Johnson, NASA’s Planetary Defense Officer Emeritus, NASA Headquarters, Washington
- Leviticus “L.A.” Lewis, FEMA detailee to NASA’s Planetary Defense Coordination Office, NASA Headquarters
- Terik Daly, planetary defense section supervisor, Johns Hopkins Applied Physics Laboratory, Laurel, Maryland
To register for the briefing, media must RSVP no later than two hours before the event to Alise Fisher at alise.m.fisher@nasa.gov. NASA’s media accreditation policy is available online.
While there are no known significant asteroid impact threats for the foreseeable future, hypothetical exercises like this one, which are conducted about every two years, provide valuable insights on how the United States could respond effectively if a potential asteroid impact threat is identified.
This year’s exercise was the first to include participation by NASA’s international collaborators in planetary defense and the first to have the benefit of actual data from NASA’s successful DART (Double Asteroid Redirection Test) mission, the world’s first in-space technology demonstration for defending Earth against potential asteroid impacts.
NASA established the Planetary Defense Coordination Office in 2016 to manage the agency’s ongoing efforts in planetary defense.
To learn more about planetary defense at NASA, visit:
https://science.nasa.gov/planetary-defense/
-end-
Charles Blue / Karen Fox
Headquarters, Washington
202-802-5345 / 202-358-1600
charles.e.blue@nasa.gov / karen.fox@nasa.gov
NASA-Led Mission to Map Air Pollution Over Both U.S. Coasts
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)This summer between June 17 and July 2, NASA will fly aircraft over Baltimore, Philadelphia, parts of Virginia, and California to collect data on air pollutants and greenhouse gas emissions.
The campaign supports the NASA Student Airborne Research Program for undergraduate interns.
Two NASA aircraft, including the P-3 shown here, will be flying over Baltimore, Philadelphia, Virginia and California between June 17 and July 2, to collect data on air pollutants and greenhouse gas emissions. Credit: (NASA/ Zavaleta)The East Coast flights will take place from June 17-26. Researchers and students will fly multiple times each week in Dynamic Aviation’s King Air B200 aircraft at an altitude of 1,000 feet over Baltimore and Philadelphia as well as Norfolk, Hampton, Hopewell, and Richmond in Virginia. Meanwhile, a NASA P-3 aircraft based out of NASA’s Wallops Flight Facility in Virginia will fly over the same East Coast locations to collect different measurements.
The West Coast flights will occur from June 29 – July 2. During the period, those same aircraft will conduct similar operations over Los Angeles, Imperial Valley, and Tulare Basin in California.
The research aircraft will fly at lower altitudes than most commercial planes and will conduct maneuvers including vertical spirals from 1,000 to 10,000 feet, circling over power plants, landfills, and urban areas. They will also occasionally conduct “missed approaches” at local airports, where the aircraft will perform a low-level flyby over a runway to collect samples close to the surface.
The aircraft carry instruments that will collect data on a range of greenhouse gases including carbon dioxide and methane, as well as air pollutants such as nitrogen dioxide, formaldehyde, and ozone. One purpose of this campaign is to validate space-based measurements observed by the TEMPO (Tropospheric Emissions: Monitoring of Pollution) mission. Launched on a commercial satellite in April 2023, the TEMPO instrument provides hourly daytime measurements of air pollutants across the United States, northern Mexico, and southern Canada.
“The goal is that this data we collect will feed into policy decisions that affect air quality and climate in the region,” said Glenn Wolfe, a research scientist and the principal investigator for the campaign at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
The B-200 aircraft is owned by Dynamics Aviation, an aircraft company contracted by NASA.
For more information about Student Airborne Research Program, visit:
https://science.nasa.gov/earth-science/early-career-opportunities/student-airborne-research-program/
By Tayler Gilmore
NASA’s Goddard Space Flight Center, Greenbelt, Maryland
Share Details Last Updated Jun 14, 2024 EditorJennifer R. MarderContactJeremy EggersLocationGoddard Space Flight Center Related Terms Explore More 5 min read Surf, Turf, Above Earth: Students Participate in NASA Field ResearchFlying over and tromping through watery landscapes along the East Coast, working alongside NASA scientists,…
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Article 8 months ago 4 min read NASA Scientists Take to the Seas to Study Air Quality Article 1 week agoNASA’s Wallops Flight Facility to Launch Student Experiments
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) A Terrier-Improved Orion sounding rocket carrying students experiments for the RockOn! mission successfully launched from NASA’s Wallops Flight Facility Aug. 17, 2023 at 6 a.m. EDT.NASA/ Kyle HoppesMore than 50 student and faculty teams are sending experiments into space as part of NASA’s RockOn and RockSat-C student flight programs. The annual student mission, “RockOn,” is scheduled to launch from Wallops Island, Virginia, on a Terrier-Improved Orion sounding rocket Thursday, June 20, with a launch window that opens at 5:30 a.m. EDT.
An introduction to rocketry for college studentsThe RockOn workshop is an introductory flight opportunity for community college and university students. RockOn participants spend a week at NASA’s Wallops Flight Facility, where they are guided through the process of building and launching an experiment aboard a sounding rocket.
“RockOn provides students and faculty with authentic, hands-on experiences tied to an actual launch into space from a NASA facility,” said Chris Koehler, on contract with NASA as RockOn’s principal investigator. “These experiences are instrumental in the creation of our next STEM workforce.”
RockOn student experiments are placed into canisters to be integrated into the payload.NASA/ Madison Olson Unique & advanced experimentsIn addition to the RockOn workshop experiments, the rocket will carry student team experiments from six different institutions as part of the RockSat-C program. The RockSat-C experiments are unique to each institution and were created off site.
RockSat-C “has been an incredible introduction into the world of NASA and how flight missions are built from start to finish,” said TJ Tomaszewski, student lead for the University of Delaware. “The project started as just a flicker of an idea in students’ minds. After countless hours of design, redesign, and coffee, the fact that we finished an experiment capable of going to space and capable of conducting valuable scientific research makes me so proud of my team and so excited for what’s possible next. Everybody dreams about space, and the fact that we’re going to launch still doesn’t feel real.”
Students participating in the 2024 RockSat-C program were able to see the RockOn rocket in the testing facility at Wallops Flight Facility.NASA/ Berit BlandRockSat-C participants include:
- Temple University, Philadelphia
Experiments will utilize X-ray spectrometry, muon detection, and magnetometry to explore the interplay among cosmic phenomena, such as X-rays, cosmic muons, and Earth’s magnetic field, while also quantifying atmospheric methane levels as a function of altitude.
- Southeastern Louisiana University, Hammond
The ION experiment aims to measure the plasma density in the ionosphere. This will be achieved by detecting the upper hybrid resonant frequency using an impedance probe mounted on the outside of the rocket and comparing the results to theoretical models. The secondary experiment, known as the ACC experiment, aims to record the rocket’s re-entry dynamics and measure acceleration in the x, y, and z directions.
- Old Dominion University, Norfolk, Virginia
The Monarch3D team will redesign and improve upon a pre-existing experiment from the previous year’s team that will print in suborbital space. This project uses a custom-built 3D printer made by students at Old Dominion.
- University of Delaware, Newark
Project UDIP-4 will measure the density and temperature of ionospheric electrons as a function of altitude and compare the quality of measurements obtained from different grounding methods. Additionally, the project focuses on developing and testing new CubeSat hardware in preparation for an orbital CubeSat mission named DAPPEr.
- Stevens Institute of Technology, Hoboken, New Jersey
The Atmospheric Inert Gas Retrieval project will develop a payload capable of demonstrating supersonic sample collection at predetermined altitudes and investigating the noble gas fractionation and contamination of the acquired samples. In addition, their payload will test the performance of inexpensive vibration damping materials by recording and isolating launch vibrations using 3D-printed components.
- Cubes in Space, Virginia Beach, Virginia
The Cubes in Space (CiS) project provides students aged 11 to 18 with a unique opportunity to conduct scientific and engineering experiments in space. CiS gives students hands-on experience and a deeper understanding of scientific and engineering principles, preparing them for more complex STEM studies and research in the future. Students develop and design their unique experiments to fit into clear, rigid plastic payload cubes, each about 1.5 inches on a side. Up to 80 of these unique student experiments are integrated into the nose cone of the rocket.
Approximately 80 small cubes will be launched as part of the RockOn sounding rocket mission.Courtesy Cubes in Space/Jorge Salazar; used with permission Watch the launchThe launch window for the mission is 5:30-9:30 a.m. EDT, Thursday June 20, with a backup day of June 21. The Wallops Visitor Center’s launch viewing area will open at 4:30 a.m. A livestream of the mission will begin 15 minutes before launch on the Wallops YouTube channel. Launch updates also are available via the Wallops Facebook page.
These circular areas show where and when people may see the rocket launch in the sky, depending on cloud cover. The different colored sections indicate the time (in seconds) after liftoff that the sounding rocket may be visible.NASA/ Christian BillieNASA’s Sounding Rocket Program is conducted at the agency’s Wallops Flight Facility, which is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland. NASA’s Heliophysics Division manages the sounding rocket program for the agency.
Share Details Last Updated Jun 14, 2024 EditorAmy BarraContactAmy Barraamy.l.barra@nasa.govLocationWallops Flight Facility Related Terms Explore More 4 min read Double Header: NASA Sounding Rockets to Launch Student ExperimentsNASA's Wallops Flight Facility is scheduled to launch two sounding rockets carrying student developed experiments…
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22 min read
Summary of the Ninth DSCOVR EPIC and NISTAR Science Team MeetingIntroduction
The ninth Deep Space Climate Observatory (DSCOVR) Earth Polychromatic Camera (EPIC) and National Institute of Standards and Technology (NIST) Advanced Radiometer [NISTAR] Science Team Meeting (STM) was held virtually October 16–17, 2023. Over 35 scientists attended, most of whom were from NASA’s Goddard Space Flight Center (GSFC), with several participating from other NASA field centers, U.S. universities, and U.S. Department of Energy laboratories. One international participant joined the meeting from Estonia. A full overview of DSCOVR’s Earth-observing instruments was printed in a previous article in The Earth Observer and will not be repeated here. This article provides the highlights of the 2023 meeting. The meeting agenda and full presentations can be downloaded from GSFC’s Aura Validation Data Center.
Opening Presentations
The opening session consisted of a series of presentations from DSCOVR mission leaders and representatives from GSFC and NASA Headquarters (HQ), who gave updates on the mission and the two Earth-viewing science instruments on board. Alexander Marshak [GSFC—DSCOVR Deputy Project Scientist] opened the meeting. He discussed the agenda for the meeting and mentioned that both Earth science instruments on DSCOVR are functioning normally – see Figure 1. At this time, more than 115 papers related to DSCOVR are listed on the EPIC website. Marshak emphasized the importance of making the Earth Science community more aware of the availability of the various EPIC and NISTAR science data products.
Figure 1. Sun-Earth-Vehicle (SEV) angle (red curve) and the distance between Earth and the DSCOVR satellite (blue curve) versus time starting from the DSCOVR launch on February 15, 2015 to April 1, 2024. These two measurements are used to track the location and orientation, respectively, of DSCOVR. The spacecraft changes its location by about 200,000 km (~124,274 mi) over about a 3-month period, and its SEV gets close to zero (which would correspond to perfect backscattering). The gap around the year 2020 was when DSCOVR was in Safe Mode for an extended period. Figure credit: Adam Szabo (Original figure by Alexander Marshak, with data provided by Joe Park/NOAA)Adam Szabo [GSFC—DSCOVR Project Scientist] welcomed the STM participants and briefly reported that the spacecraft, located at “L1” – the first of five Lagrange points in the Sun-Earth system – was still in “good health.” The EPIC and NISTAR instruments on DSCOVR continue to return their full science observations. Szabo gave an update on the 2023 Earth Science Senior Review, which DSCOVR successfully passed with overall science scores of ‘Excellent/Very Good.’ The Senior Review Panel unanimously supported the continuation of DSCOVR for the 2024–2026 period.
Thomas Neumann [GSFC, Earth Sciences Division (ESD)—Deputy Director] welcomed meeting participants on behalf of the ESD. Neumann noted the impressive engineering that has led to 8.5 years of operations and counting. He also commended the team on the continued production of important science results from these instruments – with nearly 110 papers in the peer-reviewed literature.
Following Neumann’s remarks, Steve Platnick [GSFC, Earth Sciences Division—Deputy Director for Atmospheres] welcomed the members of the DSCOVR ST as well as users of EPIC and NISTAR observations. He thanked NASA HQ for its continued strong interest in the mission. Platnick also expressed his appreciation for the mission team members who have worked hard to maintain operation of the DSCOVR satellite and instruments during this challenging time.
Richard Eckman [NASA HQ, Earth Science Division—DSCOVR EPIC/NISTAR Program Scientist] noted that a new call for proposals will be in ROSES-2025 and looks forward to learning about recent accomplishments by ST members, which will be essential in assessing the mission’s performance.
Jack Kaye [NASA HQ, Earth Science Division—Associate Director for Research] discussed the NASA research program that studies the Earth, using satellites, aircraft, surface-based measurements, and computer models. The two Earth science instruments on DSCOVR (EPIC and NISTAR) play an important role in the program. He highlighted the uniqueness of the DSCOVR observations from the Sun–Earth “L1” point providing context for other missions and the ability to discern diurnal variations.
Updates on DSCOVR Operations
The DSCOVR mission components continue to function nominally, with progress on several fronts, including data acquisition, processing, archiving, and release of new versions of several data products. The number of people using the content continues to increase, with a new Science Outreach Team having been put in place to aid users in several aspects of data discovery, access, and user friendliness.
Hazem Mahmoud [NASA’s Langley Research Center (LaRC)] discussed the new tools in the Atmospheric Science Data Center (ASDC). He reported on DSCOVR metrics since 2015 and mentioned the significant increase in using ozone (O3) products. He also announced that ASDC is moving to the Amazon Web Services (AWS) cloud.
Karin Blank [GSFC] covered the EPIC geolocation algorithm, including the general algorithm framework. She highlighted additional problems that needed to be resolved and detailed the various stages to refine the algorithm, emphasizing the enhancements made to improve geolocation accuracy.
Marshall Sutton [GSFC] reported on the DSCOVR Science Operations Center (DSOC) and Level-2 (L2) processing. DSOC is operating nominally. EPIC L1A, L1B, and NISTAR data files are produced daily. EPIC L1 products are processed into L2 science products using the computing power of the NASA Center for Climate Simulations (NCCS). Products include daily data images, including a cloud fraction map, aerosol map, and the anticipated aerosol height image. In addition, Sutton reported that the DSCOVR spacecraft has enough fuel to remain in operation until 2033.
EPIC Calibration
Alexander Cede [SciGlob] and Ragi Rajagopalan [LiftBlick OG] reported on the latest EPIC calibration version (V23) that includes the new flat field corrections based on the lunar observations from 2023 and an update to the dark count model. The EPIC instrument remains healthy and shows no change in parameters, e.g., read noise, enhanced or saturated pixels, or hot or warm pixels. The current operational dark count model still describes the dark count in a satisfactory way.
Liang-Kang Huang [Science Systems and Applications, Inc. (SSAI)] reported on EPIC’s July 2023 lunar measurements, which filled in the area near diagonal lines of the charged coupled device (CCD) not covered by 2021 and 2022 lunar data. With six short wavelength channels ranging from 317 to 551 nm, the two sets of lunar data are consistent with each other. For the macroscopic flat field corrections, he recommended the six fitted sensitivity change functions of radius and polar angle.
Igor Geogdzhaev [NASA’s Goddard Institute for Space Studies (GISS)/Columbia University] reported how continuous EPIC observations provide stable visible and near infrared (NIR) channels compared to the contemporaneous data from Visible Infrared Imaging Radiometer Suite (VIIRS) on NASA’s Suomi National Polar-orbiting Partnership (Suomi NPP) and the NASA–National Oceanic and Atmospheric Administration (NOAA) Joint Polar Satellite System (JPSS) missions. (To date, two JPSS missions have launched, JPSS-1, which is now known as NOAA-20, and JPSS-2, which is now known as NOAA-21.) Analysis of near simultaneous data from EPIC and from the Advanced Baseline Imager (ABI) on the Geostationary Operational Environmental Satellite–R (GOES R) platforms showed a high correlation coefficient, good agreement between dark and bright pixels, and small regression zero intercepts. EPIC moon views were used to derive oxygen (O2) channel reflectance by interpolation of the calibrated non-absorbing channels.
Conor Haney [LaRC] reported that the EPIC sensor was intercalibrated against measurements from the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra and Aqua platforms as well as from VIIRS on Suomi NPP and NOAA-20, using ray-matched pair radiances, and was found to be radiometrically stable when tested against two invariant calibration targets: over deep convective clouds over the tropical Pacific (dark target) and over the Libya-4 site located in the Libyan desert in Africa (bright target). The ray-matched and Earth target EPIC gain trends were found to be consistent within 1.1%, and the EPIC sensor degradation was found to be less than 1% over the seven-year record. Preliminary results intercalibrating EPIC with the Advanced Himawari Imager (AHI) on the Japan Aerospace Exploration Agency’s (JAXA) “Himawari–8” Geostationary Meteorological Satellite were also promising when both subsatellite positions were close—i.e., during equinox.
NISTAR Status and Science with Its Observations
The NISTAR instrument remains fully functional and continues its uninterrupted data record. The presentations here include more details on specific topics related to NISTAR as well as on efforts to combine information from both EPIC and NISTAR.
Steven Lorentz [L-1 Standards and Technology, Inc.] reported that NISTAR has been measuring the irradiance from the Sun-lit Earth in three bands for more than eight years. The bands measure the outgoing reflected solar and total radiation from Earth at a limited range of solar angles. These measurements assist researchers in answering questions addressing Earth radiation imbalance and predicting future climate change. NISTAR continues to operate nominally, and the team is monitoring any in-orbit degradation. Lorentz explained the evolution of the NISTAR view angle over time. He also provided NISTAR shortwave (SW) and photodiode (PD) intercomparison. NISTAR has proven itself to be an extremely stable instrument – although measurements of the offsets have measurement errors. A relative comparison with the scaled-PD channel implies long-term agreement below a percent with a constant background.
Clark Weaver [University of Maryland, College Park (UMD)] discussed updates to a new reflected- SW energy estimate from EPIC. This new product uses generic Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) aircraft observations over homogeneous scenes to spectrally interpolate between the coarse EPIC channels. This approach assumes the spectra from an EPIC pixel is a weighted combination of a solid cloud scene and the underlying (cloud-free) surface. Weaver and his team used a vector discrete ordinate radiative transfer model with a full linearization facility, called VLIDORT, to account for the different viewing/illumination geometry of the sensors. Each pixel residual between EPIC observations at six different wavelengths (between 340 and 780 nm) and the composite high-resolution spectrum from AVIRIS has been reduced by about 50%, since the last report. While the total reflected energy for a single EPIC image can be about 15 W/m2 different than the NISTAR measurement, by 2017 the offset bias was, on average, about 1 W/m2.
Andrew Lacis [GISS] said that DSCOVR measurements of Earth’s reflected solar radiation from the “L1” position offer a unique perspective for the continuous monitoring of Earth’s sunlit hemisphere. Six years of EPIC data show the seasonal and diurnal variability of Earth’s planetary albedo – but with no discernible trend. Planetary scale variability, driven by changing patterns in cloud distribution, is seen to occur at all longitudes over a broad range of time scales. The planetary albedo variability is strongly correlated at neighboring longitudes but shows strongly anticorrelated behavior at diametrically distant longitudes.
Update on EPIC Products and Science Results
EPIC has a suite of data products available. The following subsections summarize content during the DSCOVR STM related to these products. They provide updates on several of the data products and on related algorithm improvements.
Total Column Ozone
Natalya Kramarova [GSFC] reported on the status of the EPIC total O3 using the V3 algorithm. The absolute calibrations are updated every year using collocated observations from the Ozone Mapping and Profiling Suite (OMPS) on Suomi NPP. EPIC total O3 measurements are routinely compared with independent satellite and ground-based measurements. Retrieved EPIC O3 columns agree within ±5–7 Dobson Units (DU, or 1.5–2.5%) with independent observations, including those from satellites [e.g., Suomi NPP/OMPS, NASA’s Aura/Ozone Monitoring Instrument (OMI), European Union’s (EU) Copernicus Sentinel-5 Precursor/TROPOspheric Monitoring Instrument (TROPOMI)], sondes, and ground-based Brewer and Dobson spectrophotometers. The EPIC O3 record is stable and shows no substantial drifts with respect to OMPS. In the future, the EPIC O3 team plans to compare EPIC time resolved O3 measurements with observations from NASA’s Tropospheric Emissions Monitoring of Pollution (TEMPO) and the South Korean Geostationary Environment Monitoring Spectrometer (GEMS) – both in geostationary orbit. (Along with the EU’s Copernicus Sentinel-4 mission, expected to launch in 2024, these three missions form a global geostationary constellation for monitoring air quality on spatial and temporal scales that will help scientists better understand the causes, movement, and effects of air pollution across some of the world’s most populated areas.)
Jerrald Ziemke [Morgan State University] explained that tropospheric column O3 is measured over the disk of Earth every 1–2 hours. These measurements are derived by combining EPIC observations with Modern-Era Retrospective Analysis for Research and Applications (MERRA2) assimilated O3 and tropopause fields. These hourly maps are available to the public from the Langley ASDC and extend over eight years from June 2015 to present. The EPIC tropospheric O3 is now indicating post-COVID anomalous decreases of ~3 DU in the Northern Hemisphere for three consecutive years (2020–2022). Similar decreases are present in other satellite tropospheric O3 products as well as OMI tropospheric nitrogen dioxide (NO2), a tropospheric O3 precursor.
Algorithm Improvement for Ozone and Sulfur Dioxide Products
Kai Yang [UMD] presented the algorithm for retrieving tropospheric O3 from EPIC by estimating the stratosphere–troposphere separation of retrieved O3 profiles. This approach contrasts with the traditional residual method, which relies on the stratospheric O3 fields from independent sources. Validated against the near-coincident O3 sonde measurements, EPIC data biased low by a few DU (up to 5 DU), consistent with EPIC’s reduced sensitivity to O3 in the troposphere. Comparisons with seasonal means of TROPOMI tropospheric O3 show consistent spatial and temporal distributions, with lows and highs from atmospheric motion, pollution, lightning, and biomass burning. Yang also showed EPIC measurements of sulfur dioxide (SO2) from recent volcanic eruptions, including Mauna Loa and Kilauea (Hawaii, U.S., 2022–2023), Sheveluch (Kamchatka, Russia, 2023), Etna (Italy, 2023), Fuego (Guatemala, 2023), Popocatépetl (Mexico, 2023), and Pavlof and Shishaldin (Aleutian Islands, U.S., 2023). Yang reported the maximum SO2 mass loadings detected by EPIC are 430 kt from the 2022 Mauna Loa and Kilauea eruptions and 351 kt from the 2023 Sheveluch eruption.
Simon Carn [University of Michigan] showed EPIC observations of major volcanic eruptions in 2022–2023 using the EPIC L2 volcanic SO2 and UV Aerosol Index (UVAI) products to track SO2 and ash emissions. EPIC SO2 and UVAI measurements during the 2023 Sheveluch eruption show the coincident transport of volcanic SO2, ash, and Asian dust across the North Pacific. The high-cadence EPIC UVAI can be used to track the fallout of volcanic ash from eruption clouds, with implications for volcanic hazards. EPIC SO2 measurements during the November 2022 eruption of Mauna Loa volcano are being analyzed in collaboration with the U.S. Geological Survey, who monitored SO2 emissions using ground-based instruments during the eruption. Carn finished by mentioning that EPIC volcanic SO2 algorithm developments are underway including the simultaneous retrieval of volcanic SO2 and ash.
Aerosols
Myungje Choi [UMD, Baltimore County (UMBC)] presented an update on the EPIC V3 Multi-Angle Implementation of Atmospheric Correction (MAIAC) algorithm to optimize smoke aerosol models and the inversion process. The retrieved smoke/dust properties showed an improved agreement with long-term, ground-based Aerosol Robotic Network (AERONET) measurements of solar spectral absorption (SSA) and with aerosol layer height (ALH) measurements from the Cloud–Aerosol Lidar with Orthogonal Projection (CALIOP) on the Cloud–Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) mission. (Update: As of the publication of this summary, both CALIPSO and CloudSat have ended operations.) Choi reported that between 60–90% of EPIC SSA retrievals are within ±0.03 of AERONET SSA measurements, and between 56–88% of EPIC ALH retrievals are within ±1km of CALIOP ALH retrievals. He explained that the improved algorithm effectively captures distinct smoke characteristics, e.g., the higher brown carbon (BrC) fraction from Canadian wildfires in 2023 and the higher black carbon (BC) fraction from agricultural fires over Mexico in June 2023.
Sujung Go [UMBC] presented a global climatology analysis of major absorbing aerosol species, represented by BC and BrC in biomass burning smoke as well as hematite and goethite in mineral dust. The analysis is based on the V3 MAIAC EPIC dataset. Observed regional differences in BC vs. BrC concentrations have strong associations with known distributions of fuels and types of biomass burning (e.g., forest wildfire vs. agricultural burning) and with ALH retrievals linking injection heights with fire radiative power. Regional distributions of the mineral dust components have strong seasonality and agree well with known dust properties from published ground soil samples.
Omar Torres [GSFC] reported on the upgrades of the EPIC near-UV aerosol (EPICAERUV) algorithm. The EPICAERUV algorithm’s diurnal cycle of aerosol optical depth compared to the time and space collocated AERONET observations at multiple sites around the world. The analysis shows remarkably close agreement between the two datasets. In addition, Torres presented the first results of an improved UV-VIS inversion algorithm that simultaneously retrieves aerosol layer height, optical depth, and single scattering albedo.
Hiren Jethva [Morgan State University] discussed the unique product of absorbing aerosols above clouds (AAC) retrieved from EPIC near-UV observations between 340 and 388 nm. The validation analysis of the retrieved aerosol optical depth over clouds against airborne direct measurements from the NASA ObseRvations of Aerosols above CLouds and their intEractionS (ORACLES) campaign revealed a robust agreement. EPIC’s unique capability of providing near-hourly observations offered an insight into the diurnal variations of regional cloud fraction and AAC over “hotspot” regions. A new and simple method of estimating direct radiative effects of absorbing aerosols above clouds provided a multiyear timeseries dataset, which is consistent with similar estimations from Aura–OMI.
Jun Wang [University of Iowa] reported on the development and status of V1 of the L2 EPIC aerosol optical centroid height (AOCH) product – which is now publicly available through ASDC – and on improvements to the AOCH algorithm – which focus on the treatment of surface reflectance and aerosols models. He presented applications of this data product for both climate studies of Sahara dust layer height and air quality studies of surface particulate matter with diameter of 2.5 µm or less (PM2.5). In addition, Wang showed the comparisons of EPIC AOCH data product with those retrieved from TROPOMI and GEMS and discussed ongoing progress to reduce the AOCH data uncertainty that is estimated to be 0.5 km (0.3 mi) over the ocean and 0.8 km (0.5 mi) over land.
Clouds
Yuekui Yang [GSFC] explained the physical meaning of EPIC cloud effective pressure (CEP) in an “apples-to-apples” comparison with CEP measurements from the Global Ozone Monitoring Experiment 2 (GOME-2) on the European Operational Meteorology (MetOp) satellites. The results showed that the two products agreed well.
Yaping Zhou [UMBC] showed how current EPIC O2 A-band and B-band use Moon calibrations due to lack of in-flight calibration and other comparable in-space instruments for absolute calibration. This approach is ineffective at detecting small changes in instrument response function (IRF). This study examined the O2 band’s calibration and stability using a unique South Pole location and Radiative Transfer Model (RTM) simulations with in situ soundings and surface spectral albedo and bidirectional reflectance distribution function (BRDF) measurements as input. The results indicate EPIC simulations are within 1% of observations for non-absorption bands, but large discrepancies exist for the O2 A-band (15.63%) and O2 B-band (5.76%). Sensitivity studies show the large discrepancies are unlikely caused by uncertainties in various input, but a small shift (-0.2–0.3 nm) of IRF could account for the model observation discrepancy. On the other hand, observed multiyear trends in O2 band ratios in the South Pole can be explained with orbital shift – which means the instrument is stable.
Alfonso Delgado Bonal [UMBC] used the EPIC L2 cloud data to characterize the diurnal cycles of cloud optical thickness. To fully exploit the uniqueness of DSCOVR data, all clouds were separated in three groups depending on their optical thickness: thin (0–3), medium (3–10), and thick (3–25). Bonal explained that there is a predictable pattern for different latitudinal zones that reaches a maximum around noon local time – see Figure 2. It was also shown that that the median is a better measure of central tendency when describing cloud optical thickness.
Figure 2. Daytime variability of the median liquid cloud optical thickness over the ocean for different seasons of the year derived using EPIC L2 data. The various colored curves represent data collected in different seasons of the year. The black curve represents the annual average – which is most useful for calculations of cloud optical thickness. Figure credit: Alfonso Delgado BonalElizabeth Berry [Atmospheric and Environmental Research (AER)] reported on how coincident observations from EPIC and the Cloud Profiling Radar (CPR) on CloudSat have been used to train a machine learning model to predict cloud vertical structure. A XGBoost decision tree model used input (e.g., EPIC L1B reflectance, L2 Cloud products, and background meteorology) to predict a binary cloud mask on 25 vertical levels. Berry discussed model performance, feature importance, and future improvements.
Ocean
Robert Frouin [Scripps Institution of Oceanography, University of California] discussed ocean surface radiation products from EPIC data. He reported that surface radiation products were developed to address science questions pertaining to biogeochemical cycling of carbon, nutrients, and oxygen as well as mixed-layer dynamics and circulation. These products include daily averaged downward planar and scalar irradiance and average cosine for total light just below the surface in the EPIC spectral bands centered on 317.5, 325, 340, 388, 443, 551, and 680 nm and integrated values over the photosynthetically active radiation (PAR) and UV-A spectral ranges. The PAR-integrated quantities were evaluated against in situ data collected at sites in the North Atlantic Ocean and Mediterranean Sea. Frouin and his colleagues have also developed, tested, and evaluated an autonomous system for collecting and transmitting continuously spectral UV and visible downward fluxes.
Vegetation
Yuri Knyazikhin [Boston University] reported on the status of the Vegetation Earth System Data Record (VESDR) and discussed science with vegetation parameters. A new version of the VESDR software was delivered to NCCS and implemented for operational generation of the VESDR product. The new version passed tests of physics (e.g., various relationships between vegetation indices and vegetation parameters derived from the VESDR) and follow regularities reported in literature. Analysis of hotspot signatures derived from EPIC and from the Multiangle Imaging Spectroradiometer (MISR) on Terra over forests in southeastern Democratic Republic of the Congo reaffirms that long-term precipitation decline has had minimal impact on leaf area and leaf optical properties.
Jan Pisek [University of Tartu/Tartu Observatory, Estonia] reported on the verification of the previously modeled link between the directional area scattering factor (DASF) from the EPIC VESDR product and foliage clumping with empirical data. The results suggest that DASF can be accurately derived from satellite observations and provide new evidence that the photon recollision probability theory concepts can be successfully applied even at a fairly coarse spatial resolution.
Sun Glint
Tamás Várnai [UMBC] discussed the EPIC Glint Product as well as impacts of sun glint off ice clouds on other EPIC data products – see Figure 3. The cloud glints come mostly from horizontally oriented ice crystals and have strong impact in EPIC cloud retrievals. Glints increase retrieved cloud fraction, the retrieved cloud optical depth, and cloud height. Várnai also reported that the EPIC glint product is now available at the ASDC. It is expected that glints yield additional new insights about the microphysical and radiative properties of ice clouds.
Figure 3. EPIC image taken over Mexico on July 4, 2018. The red, white and blue spot over central Mexico is the result of Sun glint reflecting off high clouds containing ice crystals. EPIC is particularly well suited for studies of ice clouds that cause Sun glint, because unlike most other instruments, it uses a filter wheel to take images at multiple wavelengths, which means the image for each wavelength is obtained at a slightly different time. For example, it takes four minutes to cycle from red to blue. During that time, Earth moves by ~100 km (~62 mi) meaning each image will capture a slightly different scene. Brightness contrasts between images can be used to identify glint signals. Image credit: Tamas VanaiAlexander Kostinski [Michigan Technology University] reported on long-term changes and semi-permanent features, e.g., ocean glitter. They introduced pixel-pinned temporally and conditionally averaged reflectance images, uniquely suited to the EPIC observational circumstances. The preliminary resulting images (maps), averaged over months and conditioned on cover type (land, ocean, or clouds), show seasonal dependence at a glance (e.g., by an apparent extent of polar caps).
More EPIC Science Results
Guoyong Wen [Morgan State University] discussed spectral properties of the EPIC observations near backscattering, including four cases when the scattering angle reaches about 178° (only 2° from perfect backscattering). The enhancement addresses changes in scattering angle observed in 2020. (Scattering angle is a function of wavelength, because according to Mie scattering theory, the cloud scattering phase function in the glory region is wavelength dependent.) Radiative transfer calculations showed that the change in scattering angles has the largest impact on reflectance in the red and NIR channels at 680 nm and 780 nm and the smallest influence on reflectance in the UV channel at 388 nm – consistent with EPIC observations. The change of global average cloud amount also plays an important role in the reflectance enhancement.
Nick Gorkavyi [SSAI] talked about future plans to deploy a wide-angle camera and a multislit spectrometer on the Moon’s surface for whole-Earth observations to complement EPIC observations. Gorkavyi explained that the apparent vibrational movement of Earth in the Moon’s sky complicates observations of Earth. This causes the center of Earth to move in the Moon’s sky in a rectangle, measuring 13.4° × 15.8° with a period of 6 years.
Jay Herman [UMBC] reported on EPIC O3 and trends from combining Nimbus 7/Solar Backscatter Ultraviolet (SBUV), the SBUV-2 series, and OMPS–Nadir Mapper (NM) data. (OMPS is made up of three instruments: a Nadir Mapper (NM), Nadir Profiler, and Limb Profiler. OMPS NM is a total ozone sensor). Herman compared EPIC O3 data to OMPS NM data, which showed good agreement (especially summer values) for moderate solar zenith angle (SZA). Comparison with long-term O3 time series (1978–2021) revealed that there were trends and latitude dependent O3 turn-around dates (1994–1998). Herman emphasized that global O3 models do not show this effect but rather have only a single turn-around date around 2000.
Alexander Radkevich [LaRC] presented a poster that showed a comparative analysis of air quality monitoring by orbital and suborbital NASA missions using the DSCOVR EPIC O3 product as well as Pandora total O3 column retrievals. Comparison of the June 2023 total column O3 from EPIC data to the same periods in previous years revealed a significant – around 50 DU – increase of total O3 column in the areas impacted by the plume from 2023 Canadian wildfires.
Conclusion
At the end of the meeting Alexander Marshak, Jay Herman, and Adam Szabo discussed how to make the EPIC and NISTAR instruments more visible in the community. The EPIC website now allows visitors to observe daily fluctuations of aerosol index, cloud fraction, and the ocean surface – as observed from the “L1” point, nearly one million miles away from Earth! More daily products, (e.g., cloud and aerosol height, total leaf area index, and sunlit leaf area index) will be added soon.
The 2023 DSCOVR EPIC and NISTAR Science Team Meeting provided an opportunity to learn the status of DSCOVR’s Earth-observing instruments, EPIC and NISTAR, the status of recently released L2 data products, and the science results being achieved from the “L1” point. As more people use DSCOVR data worldwide, the ST hopes to hear from users and team members at its next meeting. The latest updates from the mission are found on the EPIC website. (UPDATE: The next DSCOVR EPIC and NISTAR STM will be held on October 16–18, 2024. Check the website for more details as the date approaches.)
Alexander Marshak
NASA’s Goddard Space Flight Center
alexander.marshak@nasa.gov
Adam Szabo
NASA’s Goddard Space Flight Center
adam.szabo@nasa.gov
NASA’s Hubble Restarts Science in New Pointing Mode
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NASA’s Hubble Restarts Science in New Pointing Mode This image of NASA’s Hubble Space Telescope was taken on May 19, 2009 after deployment during Servicing Mission 4. NASANASA successfully transitioned operations for the agency’s Hubble Space Telescope to an alternate operating mode that uses one gyro, returning the spacecraft to daily science operations Friday. The telescope and its instruments are stable and functioning normally.
Hubble went into safe mode May 24 due to an ongoing issue with one of its gyroscopes (gyros), which measure the telescope’s slew rates and are part of the system that determines and controls the direction the telescope is pointed. The gyro had been increasingly returning faulty readings over the past six months, suspending science operations multiple times. This led the Hubble team to transition from a three-gyro operating mode to observing with only one gyro, enabling more consistent science observations and keeping another operational gyro available for future use. The agency discussed this transition in detail during a media teleconference June 4.
The team will continue monitoring the problematic gyro to see if it stabilizes and can be used again in the future. Although there are some minor limitations to observing in one-gyro mode, Hubble can continue doing most of its science observations. Further refinements to optimize operations are anticipated as the team gains more experience with the one-gyro mode.
Launched in 1990, Hubble has more than doubled its expected design lifetime, and has been observing the universe for more than three decades, recently celebrating its 34th anniversary. Read more about some of Hubble’s greatest scientific discoveries.
NASA’s Hubble Temporarily Pauses ScienceOriginally Published May 31, 2024
NASA’s Hubble Space Telescope entered safe mode May 24 due to an ongoing gyroscope (gyro) issue, suspending science operations. Hubble’s instruments are stable, and the telescope is in good health.
The telescope automatically entered safe mode when one of its three gyroscopes gave faulty telemetry readings. Hubble’s gyros measure the telescope’s slew rates and are part of the system that determines and controls precisely the direction the telescope is pointed. NASA will provide more information early the first week of June.
NASA anticipates Hubble will continue making discoveries throughout this decade and possibly into the next, working with other observatories, such as the agency’s James Webb Space Telescope for the benefit of humanity.
Launched in 1990, Hubble has been observing the universe for more than three decades and recently celebrated its 34th anniversary. Read more about some of Hubble’s greatest scientific discoveries.
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Hubble Pointing and Control
Operating Hubble with Only One Gyroscope
Hubble Science Highlights
Hubble Images
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Media Contact:
Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
NASA’s LRO Spots China’s Chang’e 6 Spacecraft on Lunar Far Side
NASA’s LRO (Lunar Reconnaissance Orbiter) imaged China’s Chang’e 6 sample return spacecraft on the far side of the Moon on June 7. Chang’e 6 landed on June 1, and when LRO passed over the landing site almost a week later, it acquired an image showing the lander on the rim of an eroded, 55-yard-diameter (about 50 meters) crater.
The LRO Camera team computed the landing site coordinates as about 42 degrees south latitude, 206 degrees east longitude, at an elevation of about minus 3.27 miles (minus 5,256 meters).
This before and after animation of LRO images shows the appearance of the Chang’e 6 lander. The increased brightness of the terrain surrounding the lander is due to disturbance from the lander’s engines and is similar to the blast zone seen around other lunar landers. The before image is from March 3, 2022, and the after image is from June 7, 2024.Credit: NASA/Goddard/Arizona State UniversityThe Chang’e 6 landing site is situated toward the southern edge of the Apollo basin (about 306 miles or 492 km in diameter, centered at 36.1 degrees south latitude, 208.3 degrees east longitude). Basaltic lava erupted south of Chaffee S crater about 3.1 billion years ago and flowed downhill to the west until it encountered a local topographic high, likely related to a fault. Several wrinkle ridges in this region have deformed and raised the mare surface. The landing site sits about halfway between two of these prominent ridges. This basaltic flow also overlaps a slightly older flow (about 3.3 billion years old), visible further west, but the younger flow is distinct because it has higher iron oxide and titanium dioxide abundances.
A regional context map of the Chang’e 6 landing site. Color differences have been enhanced for clarity. The dark area is a basaltic mare deposit; bluer areas of the mare are higher-titanium flows. Contour lines marking 100-meter (about 328 feet) elevation intervals are overlaid to provide a sense of the topography. Image is about 118 miles (190 km) across. Credit: NASA/Goddard/Arizona State UniversityLRO is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the Science Mission Directorate at NASA Headquarters in Washington. Launched on June 18, 2009, LRO has collected a treasure trove of data with its seven powerful instruments, making an invaluable contribution to our knowledge about the Moon. NASA is returning to the Moon with commercial and international partners to expand human presence in space and bring back new knowledge and opportunities.
More on this story from Arizona State University's LRO Camera websiteMedia Contact:
Nancy N. Jones
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Johnson Celebrates LGBTQI+ Pride Month: Meet Michael Chandler
Michael Chandler has provided configuration and data management support at Houston’s Johnson Space Center for the last 13 years. After roughly seven years supporting the Exploration Systems Development Division, Chandler transitioned to the Moon to Mars Program Office in 2019. He and his team work to ensure that the baseline for Moon to Mars products, like agreements and documents, is appropriately controlled and that configuration and data management processes are integrated across the office’s six programs – Orion, Gateway, EHP, Space Launch System, Human Landing system, and Exploration Ground Systems.
“The most rewarding part of my job is not only the magnitude of what I have the privilege of working on every day, returning humans to the surface of the Moon, but also the experience I get in working with such a diverse group of members of the aerospace community,” said Chandler, a contractor with The Aerospace Corporation. “It’s also so rewarding to work as a team on a common goal and to look forward to the work I do every day!”
Portrait of Michael Chandler onsite at Johnson Space Center. NASA/Noah MoranChandler has been an active member of the Out & Allied Employee Resource Group (OAERG) since 2018 and says his involvement with the group led to some groundbreaking life events. “I was very shy and reticent about revealing who I was until I got involved with Out & Allied,” he said. “I now believe that being ‘out’ is a way to support and encourage others to be themselves.”
Chandler learned about OAERG while attending a training about how to be an ally for the LGBTQ+ community. In his first year with the group, he helped organize a panel discussion on allyship and creating safe workplaces. He then became co-chair of OAERG’s Pride Committee, working with ERG colleagues and others to plan the group’s LGBTQ+ Pride Month events and participation in Houston’s annual Pride Parade. “I had a wonderful experience managing events and bringing everyone together for Pride,” he said – efforts that earned him a Trailblazer Award.
Chandler said he has grown personally and professionally through his involvement with OAERG. “I was very shy and kind of uptight at the first meeting that I went to, but everyone was so kind and accepting, and I slowly started taking on responsibilities and planning events,” he said. “These activities helped me grow as a communicator and a leader in my regular work and personal life.”
Michael Chandler (left) stands with fellow Out & Allied Employee Resource Group members, waiting for the Houston Pride Parade to begin. Image courtesy of Michael ChandlerChandler belongs to other employee resource groups (ERGs) at Johnson to support different communities and find opportunities to collaboratively promote diversity, equity, and inclusion (DEI) at the center, and he encourages others to do the same. “Even if you only participate when you have time, it can lead to knowledge and ways to support other communities that have the same challenges in this world,” he said.
Chandler has been impressed with agency and center leadership’s involvement in DEI efforts and support for ERGs to date. He suggested that increased communication around DEI initiatives may help to quell anxieties about the political landscape and developments outside of NASA by reassuring team members that their employer supports them for who they are. He believes that every person at Johnson can help create an inclusive environment by being respectful, listening with an open heart, and joining the fight to ensure that everyone can be themselves.
“The most important thing is that everyone needs to be their true self,” he said. “It’s so rewarding and makes life so much more fun!”
Human Factors Researcher Garrett Sadler
“I graduated in 2008, so that job market was not super great, and I ended up with this very unusual job working for this guy who thought that he had some new theory of physics that he wanted to work on. And so I was responsible for creating little computer simulations, trying to resemble some version of his ideas. His whole thing was like a quasi-spiritual tool, looking toward science as a rationalization of different spiritual beliefs that he had about a collective consciousness and the interconnectedness of things.
“As I worked for him longer and met a bunch of other people who were trying to put various spiritual beliefs on scientific footing, I got interested [and thought] maybe this could be studied as a cultural thing. What’s going on here with the desire to scientifically explain spiritual beliefs that they have? What’s the dynamic going on there? That’s what led me into eventually going to grad school for anthropology. I studied the way that science gets conceptualized and interpreted to rationalize spiritual and religious beliefs.
“I had this sort of unconventional trajectory [to NASA]. I didn’t really set a target on something to pursue it. The other thing that might be surprising is that I’ve been insecure about it at every single stage. You know, there’s the whole impostor syndrome thing, and I didn’t feel like I was qualified to be here because I didn’t have some sort of traditional path or because my educational background looks different than that of most of my colleagues. But I’m now at a place where I’ve come to understand that’s true for everyone.”
– Garrett Sadler, Human Factors Researcher, NASA’s Ames Research Center
Image Credit: NASA/Bradon Torres
Interviewer: NASA/Tahira Allen
Hubble Captures a Cosmic Fossil
This NASA/ESA Hubble Space Telescope image features the globular cluster NGC 2005. It’s not an unusual globular cluster in and of itself, but it is a peculiarity when compared to its surroundings. NGC 2005 is located about 750 light-years from the heart of the Large Magellanic Cloud (LMC), which is the Milky Way’s largest satellite galaxy some 162,000 light-years from Earth. Globular clusters are densely-packed groups of stars that can hold tens of thousands or millions of stars. Their density means they are tightly bound by gravity and therefore very stable. This stability contributes to their longevity: globular clusters can be billions of years old, and are often comprised of very old stars. Studying globular clusters in space can be a little like studying fossils on Earth: where fossils give insights into the characteristics of ancient plants and animals, globular clusters illuminate the characteristics of ancient stars.
Current theories of galaxy evolution predict that galaxies merge with one another. Astronomers think the relatively large galaxies we observe in the modern universe formed when smaller galaxies merged. If this is correct, then we would expect to see evidence that the most ancient stars in nearby galaxies originated in different galactic environments. Because globular clusters hold ancient stars, and because of their stability, they are an excellent laboratory to test this hypothesis.
NGC 2005 is such a globular cluster, and its very existence provides evidence that supports the theory of galaxy evolution via mergers. Indeed, what makes NGC 2005 a bit peculiar from its surroundings, is the fact that its stars have a chemical composition that is distinct from the stars around it in the LMC. This suggests that the LMC underwent a merger with another galaxy somewhere in its history. That other galaxy has long-since merged and otherwise dispersed, but NGC 2005 remains behind as an ancient witness to the long-past merger.
Text Credit: European Space Agency (ESA)
The Next Full Moon is the Strawberry Moon
NASA/Joel Kowsky
The Next Full Moon is the Strawberry Moon; the Flower, Hot, Hoe, or Planting Moon; the Mead or Honey Moon; the Rose Moon; Vat Purnima; Poson Poya; and the LRO Moon.
The next full Moon will be Friday evening, June 21, 2024, appearing opposite the Sun (in Earth-based longitude) at 9:08 PM EDT. This will be Saturday from Greenland and Cape Verde time eastward across Eurasia, Africa, and Australia to the International Date Line in the mid-Pacific. Most commercial calendars will show this full Moon on Saturday, June 22, the date in Coordinated Universal Time (UTC). The Moon will appear full for about three days around this time, from Thursday evening through Sunday morning.
In the 1930s the Maine Farmer’s Almanac began publishing “Indian” names for full Moons and these names are now widely known and used. According to this Almanac, as the full Moon in June this is the Strawberry Moon, a name that comes from the relatively short season for harvesting strawberries in the north-eastern United States. Other seasonal names that I have found in various sources (sometimes with conflicting information about whether they are of European or Native American origin) are the Flower Moon, Hot Moon, Hoe Moon, and Planting Moon.
An old European name for this full Moon is the Mead or Honey Moon. Mead is a drink created by fermenting honey mixed with water and sometimes fruits, spices, grains, or hops. In some countries Mead is also called Honey Wine (though in others Honey Wine is made differently). Some writings suggest the time around the end of June was when honey was ready for harvesting, which made this the “sweetest” Moon. The word “honeymoon” traces back to at least the 1500s in Europe. The tradition of calling the first month of marriage the “honeymoon” may be tied to this full Moon because of the custom of marrying in June or because the “Honey Moon” is the “sweetest” Moon of the year. There doesn’t appear to be enough evidence to support a 19th century theory that the word entered English from the custom of gifting newlyweds mead for their first month of marriage.
Another European name for this full Moon is the Rose Moon. Some sources indicate “Rose Moon” comes from the roses that bloom this time of year. Others indicate that the name comes from the color of the full Moon. The orbit of the Moon around the Earth is in almost the same plane as the orbit of the Earth around the Sun (only about 5 degrees off). On the summer solstice the Sun appears highest in the sky for the year. Full Moons are opposite the Sun, so a full Moon near the summer solstice will be low in the sky. Particularly for Europe’s higher latitudes, when the full Moon is low it shines through more atmosphere, making it more likely to have a reddish color (for the same reasons that sunrises and sunsets are red). For the Washington, DC area, the full Moon on the night from the evening of June 21 to the morning of June 22 will have the lowest full Moon of the year, reaching only 21.9 degrees above the southern horizon at 1:20 AM EDT.
For Hindus this is Vat Purnima. During the 3 days of this full Moon married women will show their love for their husbands by tying a ceremonial thread around a banyan tree. The celebration is based on the legend of Savitri and Satyavan.
For Buddhists this full Moon is Poson Poya. The Poson holiday in Sri Lanka celebrates the introduction of Buddhism in 236 BCE.
Another tribe has also given a name to this full Moon. This tribe is now scattered but mostly lived in the mid-Atlantic region of the United States. This tribe’s language is primarily English, but with a liberal smattering of acronyms, arcane scientific and engineering terms, and Hawaiian phrases (cheerfully contributed by the former Deputy Project Manager). Comprised of people from all backgrounds, many of whom have gone on to join other tribes, this tribe was devoted to the study of the Moon. This tribe calls June’s full Moon the LRO Moon, in honor of the spacecraft they launched towards the Moon 15 years ago, on June 18, 2009. NASA’s Lunar Reconnaissance Orbiter is still orbiting the Moon providing insights about our nearest celestial neighbor, some of which help us understand our own planet. See https://www.nasa.gov/mission_pages/LRO/main/index.html for more information.
Many lunar and lunisolar calendars start the months on or just after the new Moon and the full Moon is near the middle of the month. This full Moon is near the middle of the fifth month of the Chinese year of the Dragon, Sivan in the Hebrew calendar, and Dhu al-Hijjah, the final month of the Islamic year and one of the four sacred months during which fighting is forbidden.
As usual, the wearing of suitably celebratory celestial attire is encouraged in honor of the full Moon. If you’re not allergic, enjoy the strawberries, flowers, and honey during this “sweetest” month of the year, and take note of how low in the sky this full Moon will be.
As for other celestial events between now and the full Moon after next (with specific times and angles based on the location of NASA Headquarters in Washington, DC):
As summer begins the daily periods of sunlight start to gradually shorten, having been at their longest on the summer solstice on the day before this full Moon. On Friday, June 21, 2024 (the day of the full Moon), morning twilight will begin at 4:30 AM, sunrise will be at 5:43 AM, solar noon at 1:10 PM when the Sun will reach its maximum altitude of 74.6 degrees, sunset will be at 8:37 PM, and evening twilight will end at 9:49 PM. The period of daylight will be 1.2 seconds shorter than on the summer solstice the previous day.
The solar days (as measured, for example, from solar noon to solar noon on a sundial) are longer than 24 hours near the solstices, so the earliest sunrises of the year occur before the summer solstice and the latest sunsets occur after the solstice. For the Washington, DC area and similar latitudes at least (I’ve not checked for other latitudes), Thursday, June 27, will have the latest sunset of the year, with sunset at 8:37:30 PM EDT.
By Sunday, July 21, (the day of the full Moon after next), morning twilight will begin at 4:52 AM, sunrise will be at 6:00 AM, solar noon at 1:15 PM when the Sun will reach its maximum altitude of 71.4 degrees, sunset will be at 8:28 PM, and evening twilight will end at 9:37 PM.
The comet 13P/Olbers is expected to peak at magnitude 7.5 in early July, too dim to see with the naked eye. The two meteor showers expected to peak this lunar cycle will be difficult to see. The full Moon will interfere with the peak of the June Bootids (170 JBO) on June 27. The July Pegasids (175 JPE), peaking on July 10, is only expected to show 3 meteors per hour (under ideal conditions).
Evening Sky Highlights:On the evening of Friday, June 21, 2024 (the evening of the day of the full Moon), as twilight ends (at 9:49 PM EDT), the rising Moon will be 7 degrees above the southeastern horizon. The bright planets Venus and Mercury will be below the horizon, with Venus setting 21 minutes and Mercury setting 43 minutes after sunset. Mercury may be visible from about 30 minutes after sunset until it sets 13 minutes later. The bright object appearing closest to overhead will be the star Arcturus at 69 degrees above the south-southwestern horizon. Arcturus is the brightest star in the constellation Boötes the herdsman or plowman. It is the 4th brightest star in our night sky and is 36.7 light years from us. While it has about the same mass as our Sun, it is about 2.6 billion years older and has used up its core hydrogen, becoming a red giant 25 times the size and 170 times the brightness of our Sun.
As this lunar cycle progresses the background of stars will appear to shift westward each evening (as the Earth moves around the Sun). June 30 will be the first evening that the bright planet Mercury will be above the west-northwestern horizon as evening twilight ends and the first evening that the bright planet Venus will be above the horizon 30 minutes after sunset (an approximation of when Venus will start emerging from the glow of dusk. Mercury will shift to the left low along the horizon, reaching its highest above the horizon (just 2 degrees as twilight ends) on July 13. The waxing Moon will pass by Regulus on July 8 and 9, Spica on July 13, and Antares on July 17.
By the evening of Sunday, July 21 (the evening of the day of the full Moon after next), as twilight ends (at 9:37 PM EDT), the rising Moon will be 3 degrees above the east-southeastern horizon. The bright planet Mercury will be 1 degree above the west-northwestern horizon and 6 minutes away from setting. The planet Venus will set 22 minutes before twilight ends, but will be bright enough to see in the glow of dusk low on the west-northwestern horizon before it sets. The bright object appearing closest to overhead will be Vega, the brightest star in the constellation Lyra the lyre, at 65 degrees above the eastern horizon. Vega is one of the three bright stars in the Summer Triangle along with Deneb, and Altair. Vega is the 5th brightest star in our night sky, about 25 light-years from Earth, has twice the mass of our Sun, and shines 40 times brighter than our Sun.
Morning Sky Highlights:On the morning of Friday, June 21, 2024 (the morning of the day of the full Moon), as twilight begins (at 4:31 AM EDT), the setting full Moon will be 2 degrees above the southwestern horizon. The brightest planet in the sky will be Jupiter at just 3 degrees above the east-northeastern horizon. The planet Mars will be 19 degrees above the eastern horizon and the planet Saturn (almost as bright as Mars) will be 37 degrees above the southeastern horizon. The bright object appearing closest to overhead will be the star Deneb at 80 degrees above the northwestern horizon. Deneb is the 19th brightest star in our night sky and is the brightest star in the constellation Cygnus the swan. Deneb is one of the three bright stars of the “Summer Triangle” (along with Vega and Altair). Deneb is about 20 times more massive than our Sun but has used up its hydrogen, becoming a blue-white supergiant about 200 times the diameter of the Sun. If Deneb were where our Sun is, it would extend to about the orbit of the Earth. Deneb is about 2,600 light years from us.
As this lunar cycle progresses, Jupiter, Saturn, and the background of stars will appear to shift westward each evening, with Mars shifting more slowly and to the left. The waning Moon will pass by Saturn on June 27, on Mars on July 1, the Pleiades star cluster on July 2, and Jupiter on July 3.
By the morning of Sunday, July 21 (the morning of the day of the full Moon after next), as twilight begins (at 4:52 AM EDT), the setting full Moon will be 7 degrees above the southwestern horizon. The brightest planet in the sky will be Jupiter at 25 degrees above the eastern horizon. Mars will be 33 degrees above the eastern horizon and Saturn 45 degrees above the southern horizon. The bright object appearing closest to overhead still will be the star Deneb at 56 degrees above the west-northwestern horizon.
Detailed Daily Guide:Here for your reference is a day-by-day listing of celestial events between now and the full Moon after next. The times and angles are based on the location of NASA Headquarters in Washington, DC, and some of these details may differ for where you are (I use parentheses to indicate times specific to the DC area).
Sunday morning, June 16, 2024, will be the first morning that the bright planet Jupiter will be above the east-northeastern horizon as morning twilight begins (at 4:30 AM EDT).
Sunday evening into early Monday morning, June 16 to 17, 2024, the bright star Spica will appear near the waxing gibbous Moon. As evening twilight ends (at 9:48 PM EDT) Spica will be 3.5 degrees to the right of the Moon. By the time Spica sets on the west-southwestern horizon 4.5 hours later (at 2:16 AM) it will be 5 degrees to the lower right of the Moon. Around the northern part of the boundary between Europe and Asia the Moon will actually block Spica from view.
Wednesday evening, June 19, 2024, will be the first evening the bright planet Mercury will be above the west-northwestern horizon 30 minutes after sunset, an approximation of when it will begin emerging from the glow of dusk. Each evening after this Mercury should become easier to spot and by the end of June will be above the horizon as evening twilight ends.
Wednesday evening into Thursday morning, June 19 to 20, 2024, the bright star Antares will appear near the waxing gibbous Moon. As evening twilight ends (at 9:49 PM EDT) Antares will be 5 degrees to the lower left of the Moon. The Moon will reach its highest in the sky 1.5 hours later (at 11:25 PM EDT) with Antares 4 degrees to the left of the Moon. The Moon will set first on the southwestern horizon (at 4:03 AM) with Antares 2 degrees to the upper left.
Thursday afternoon, June 20, 2024, at 4:51 PM EDT will be the summer solstice, the astronomical end of spring and start of summer. This will be the day with the longest period of sunlight (14 hours, 53 minutes, 42.5 seconds) but will not be the day with the earliest sunrise or the latest sunset.
As mentioned above, the full Moon will be Friday evening, June 21, 2024, at 9:08 PM EDT. This will be on Saturday from Greenland and Cape Verde time eastward across Eurasia, Africa, and Australia to the International Date Line in the mid-Pacific. Most commercial calendars will show this full Moon on Saturday, June 22. This will be the lowest full Moon of the year (reaching only 21.9 degrees above the southern horizon Saturday morning at 1:20 AM). The Moon will appear full for about three days around this time, from Thursday evening through Sunday morning.
Thursday morning, June 27, 2024, the planet Saturn will appear near the waning gibbous Moon. As Saturn rises on the eastern horizon (at 12:26 AM EDT) it will be 6 degrees to the lower left of the Moon. By the time morning twilight begins (at 4:33 AM) Saturn will be 4 degrees to the upper left of the Moon.
Thursday morning June 27, 2024, the Moon will be at perigee, its closest to the Earth for this orbit.
For the Washington, DC area and similar latitudes, at least, Thursday, June 27, 2024, will have the latest sunset of the year (with sunset at 8:37:30 PM EDT).
Friday afternoon, June 28, 2024, the waning Moon will appear half-full as it reaches its last quarter at 5:53 PM EDT (when the Moon will be below the horizon).
Sunday evening, June 30, 2024, will be the first evening that the bright planet Mercury will be above the west-northwestern horizon as evening twilight ends (at 9:49 PM EDT). It will also be the first evening that the bright planet Venus will be above the west-northwestern horizon (at 9:07 PM) 30 minutes after sunset, an approximation of when Venus will start emerging from the glow of dusk.
Monday morning, July 1, 2024, the planet Mars will appear 5 degrees to the lower left of the waning crescent Moon. Mars will rise last on the east-northeastern horizon (at 2:29 AM EDT) and morning twilight will begin a little more than 2 hours later (at 4:35 AM).
Tuesday morning, July 2, 2024, the Pleiades star cluster will appear 5 degrees to the lower left of the waning crescent Moon. The Pleiades will rise last on the east-northeastern horizon (around 2:46 AM EDT) and morning twilight will begin a little less than 2 hours later (at 4:35 AM).
Friday afternoon, July 5, 2024, the Earth will be at aphelion, its farthest away from the Sun in its orbit, 3.4% farther away than it was at perihelion in early January. Since the intensity of light drops off as the square of the distance, the sunlight reaching the Earth at aphelion is about 6.5% less bright than sunlight reaching the Earth at perihelion.
Friday evening, July 5, 2024, at 6:57 PM EDT, will be the new Moon, when the Moon passes between the Earth and the Sun and will not be visible from the Earth. The day of or the day after the New Moon marks the start of the new month for most lunisolar calendars. Saturday, July 6 will be the start of the sixth month of the Chinese year of the Dragon. Sundown on July 6 will mark the start of Tammuz in the Hebrew calendar. In the Islamic calendar the months traditionally start with the first sighting of the waxing crescent Moon. Many Muslim communities now follow the Umm al-Qura Calendar of Saudi Arabia, which uses astronomical calculations to start months in a more predictable way. Using this calendar, sundown on Saturday, July 6, will probably mark Al-Hijra, the Islamic New Year and the beginning of the month of Muharram, although Muharram is one of four months for which the calendar dates may be adjusted by the religious authorities of Saudi Arabia after actual sightings of the lunar crescent. Al-Hijra is a public holiday in many Muslim countries. Customs vary, but most include observing the day quietly and practicing gratitude. Muharram is one of the four sacred months during which warfare is forbidden.
Sunday evening, July 7, 2024, the planet Mercury will appear 3 degrees below the thin, waxing crescent Moon, with the Beehive cluster (visible with binoculars) 1.5 degrees to the lower right of Mercury. As evening twilight ends (at 9:47 PM EDT) the Moon will be 4 degrees above the west-northwestern horizon, with Mercury a little more than 1 degree and the Beehive cluster a little less than 1 degree above the horizon. The Beehive cluster will set first 7 minutes later (at 9:54 PM), followed by Mercury 4 minutes after that (at 9:58 PM) and the Moon 19 minutes after Mercury set (at 10:17 PM).
Friday morning, July 12, 2024, at 4:12 AM EDT (when we can’t see it), the Moon will be at apogee, its farthest from the Earth for this orbit.
Saturday evening, July 13, 2024, the Moon will appear half-full as it reaches its first quarter at 6:49 PM EDT.
Saturday evening, July 13, 2024, will be when the planet Mercury will reach its highest (2 degrees) above the west-northwestern horizon as evening twilight ends (at 9:43 PM EDT).
Saturday night, July 13, 2024, the bright star Spica will appear near the half-full Moon, so near that for part of the night the Moon will block Spica from view for much of North America (see http://lunar-occultations.com/iota/bstar/0714zc1925.htm for a map and information on the locations that will see this occultation). For the location of NASA Headquarters in Washington, DC (angles and times will be different for other locations), as evening twilight ends (at 9:43 PM EDT), Spica will be 1 degree to the left of the Moon. If you are in a location that will see this occultation, you should be able to see Spica vanish behind the dark half of the Moon (at 11:26 PM for the DC area). For the Washington, DC area the Moon will set (at 12:32 AM) before Spica reemerges. For locations farther west, the brightness of the lit half of the Moon will make it hard to see when Spica emerges.
Wednesday night into early Thursday morning, July 17 to 18, 2024, the bright star Antares will appear near the waxing gibbous Moon. As evening twilight ends (at 9:40 PM EDT) Antares will be 3 degrees to the upper right of the Moon. The Moon will reach its highest in the sky 27 minutes later (at 10:07 PM). As Antares sets (at 2:21 AM) it will be 5 degrees to the lower right of the Moon. For much of the southern part of Africa the Moon will pass in front of Antares earlier on Wednesday. See http://lunar-occultations.com/iota/bstar/0717zc2366.htm for a map and information on the locations that will see this occultation. The full Moon after next will be Sunday morning, July 21, 2024, at 6:17 AM EDT. This will be late Saturday night for the International Date Line West and the American Samoa and Midway time zones and early Monday morning for Line Islands Time. The Moon will appear full for about three days around this time, from Friday evening through Monday morning, making this a full Moon weekend.
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NASA Announces New System to Aid Disaster Response
In early May, widespread flooding and landslides occurred in the Brazilian state of Rio Grande do Sul, leaving thousands of people without food, water, or electricity. In the following days, NASA teams provided data and imagery to help on-the-ground responders understand the disaster’s impacts and deploy aid.
Building on this response and similar successes, on June 13, NASA announced a new system to support disaster response organizations in the U.S. and around the world.
Members of the Los Angeles County Fire Department’s Urban Search and Rescue team in Adiyaman, Turkey (Türkiye), conducting rescue efforts in the wake of powerful earthquakes that struck the region in February 2023. NASA provided maps and data to support USAID and other regional partners during these earthquakes. USAID“When disasters strike, NASA is here to help — at home and around the world,” said NASA Administrator Bill Nelson. “As challenges from extreme weather grow, so too does the value of NASA’s efforts to provide critical Earth observing data to disaster-response teams on the frontlines. We’ve done so for years. Now, through this system, we expand our capability to help power our U.S. government partners, international partners, and relief organizations across the globe as they take on disasters — and save lives.”
The team behind NASA’s Disaster Response Coordination System gathers science, technology, data, and expertise from across the agency and provides it to emergency managers. The new system will be able to provide up-to-date information on fires, earthquakes, landslides, floods, tornadoes, hurricanes, and other extreme events.
NASA Administrator Bill Nelson delivers remarks during an event launching a new Disaster Response Coordination System that will provide communities and organizations around the world with access to science and data to aid disaster response, Thursday, June 13, 2024, at the NASA Headquarters Mary W. Jackson Building in Washington. NASA/Bill Ingalls“The risk from climate-related hazards is increasing, making more people vulnerable to extreme events,” said Karen St. Germain, director of NASA’s Earth Science Division. “This is particularly true for the 10% of the global population living in low-lying coastal regions who are vulnerable to storm surges, waves and tsunamis, and rapid erosion. NASA’s disaster system is designed to deliver trusted, actionable Earth science in ways and means that can be used immediately, to enable effective response to disasters and ultimately help save lives.”
Agencies working with NASA include the Federal Emergency Management Agency, the National Oceanic and Atmospheric Administration (NOAA), the U.S. Geological Survey, and the U.S. Agency for International Development — as well as international organizations such as World Central Kitchen.
“With this deliberate and structured approach, we can be even more effective in putting Earth science into action,” said Josh Barnes, at NASA’s Langley Research Center in Hampton, Virginia. Barnes manages the Disaster Response Coordination System.
NASA Disasters Team Aiding BrazilWhen the floods and landslides ravaged parts of Brazil in May, officials from the U.S. Southern Command — working with the U.S. Space Force and Air Force, and regional partners — reached out to NASA for Earth-observing data.
Image Before/AfterNASA’s response included maps of potential power outages from the Black Marble project at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Disaster response coordinators at NASA Goddard also reviewed high-resolution optical data — from the Commercial Smallsat Data Acquisition Program — to map more than 4,000 landslides.
Response coordinators from NASA’s Jet Propulsion Laboratory and the California Institute of Technology, both in Southern California, produced flood extent maps using data from the NASA and U.S. Geological Survey Landsat mission and from ESA’s (the European Space Agency) Copernicus Sentinel-2 satellite. Response coordinators at NASA’s Johnson Space Center in Houston also provided photographs of the flooding taken by astronauts aboard the International Space Station.
Building on Previous WorkThe Brazil event is just one of hundreds of responses NASA has supported over the past decade. The team aids decision-making for a wide range of natural hazards and disasters, from hurricanes and earthquakes to tsunamis and oil spills.
“NASA’s Disasters Program advances science for disaster resilience and develops accessible resources to help communities around the world make informed decisions for disaster planning,” said Shanna McClain, manager of NASA’s Disasters Program. “The new Disaster Response Coordination System significantly expands our efforts to bring the power of Earth science when responding to disasters.”
For more information visit:
https://disasters.nasa.gov/response
By Jacob Reed
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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