NASA

The Progress 85 cargo craft is seen shortly after undocking from International Space Station on Feb. 12 as it was orbiting 260 miles above the Pacific Ocean.

NASA will provide live launch and docking coverage of a Roscosmos cargo spacecraft carrying about three tons of food, fuel, and supplies for the Expedition 71 crew aboard the International Space Station.

The unpiloted Progress 88 spacecraft is scheduled to launch at 5:43 a.m. EDT (2:43 p.m. Baikonur time) Thursday, May 30, on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.

Live launch coverage will begin at 5:15 a.m. on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.

After a two-day in-orbit journey to the station, the spacecraft will automatically dock to the space-facing port of orbiting laboratory’s Poisk module at 7:47 a.m., Saturday, June 1. NASA coverage of rendezvous and docking will begin at 7 a.m. on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website.
The spacecraft will remain docked at the station for almost six months before departing in late November for a re-entry into Earth’s atmosphere to dispose of trash loaded by the crew.

The International Space Station is a convergence of science, technology, and human innovation that enables research not possible on Earth. For more than 23 years, NASA has supported a continuous U.S. human presence aboard the orbiting laboratory, through which astronauts have learned to live and work in space for extended periods of time. The space station is a springboard for the development of a low Earth economy and NASA’s next great leaps in exploration, including missions to the Moon under Artemis and ultimately, human exploration of Mars.

Learn more about the space station, its research, and crew, at:

https://www.nasa.gov/station

-end-

Julian Coltre
Headquarters, Washington
202-358-1100
julian.n.coltre@nasa.gov

Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov

4 min read

NASA’s OSIRIS-APEX Unscathed After Searing Pass of Sun

Mission engineers were confident NASA’s OSIRIS-APEX (Origins, Spectral Interpretation, Resource Identification – Apophis Explorer) spacecraft could weather its closest ever pass of the Sun on Jan. 2, 2024. Their models had predicted that, despite traveling 25 million miles closer to the heat of the Sun than it was originally designed to, OSIRIS-APEX and its components would remain safe.

The mission team confirmed that the spacecraft indeed had come out of the experience unscathed after downloading stored telemetry data in mid-March. The team also tested OSIRIS-APEX’s instruments in early April, once the spacecraft was far enough from the Sun to return to normal operations. Between December 2023 and March, OSIRIS-APEX was inactive, with only limited telemetry data available to the team on Earth.

Both these images from a camera called StowCam aboard OSIRIS-APEX show the same view taken six months apart, before (left) and after (right) the Jan. 2, 2024, perihelion. Notably, there is no observable difference on spacecraft surfaces, a good indication that the higher temperatures faced during perihelion didn’t alter the spacecraft. Another insight gleaned from the identical view in the two images is that the camera’s performance was also not affected by perihelion. StowCam, a color imager, is one of three cameras comprising TAGCAMS (the Touch-and-Go Camera System), which is part of OSIRIS-APEX’s guidance, navigation, and control system. TAGCAMS was designed, built and tested by Malin Space Science Systems; Lockheed Martin integrated TAGCAMS to the OSIRIS-APEX spacecraft and operates TAGCAMS.

The spacecraft’s clean bill of health was due to creative engineering. Engineers placed OSIRIS-APEX in a fixed orientation with respect to the Sun and repositioned one of its two solar arrays to shade the spacecraft’s most sensitive components during the pass.

The spacecraft is in an elliptical orbit around the Sun that brings it to a point closest to the Sun, called a perihelion, about every nine months. To get on a path that will allow it to meet up with its new target Apophis in 2029, the spacecraft’s trajectory includes several perihelions that are closer to the Sun than the spacecraft’s components were originally designed to withstand.

“It’s phenomenal how well our spacecraft configuration protected OSIRIS-APEX, so I’m really encouraged by this first close perihelion pass,” said Ron Mink, mission systems engineer for OSIRIS-APEX, based at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Besides confirming that the January perihelion worked out according to predictions, engineers found surprises while testing spacecraft components. A couple of instruments came out better than expected after exposure to higher temperatures.

A camera that helped map asteroid Bennu and will do the same at Apophis, saw a 70% reduction in “hot pixels” since April 13, 2023, the last time it was tested. Hot pixels, which are common in well-used cameras in space, show up as white spots in images when detectors accumulate exposure to high-energy radiation, mostly from our Sun.

“We think the heat from the Sun reset the pixels through annealing,” said Amy Simon, OSIRIS-APEX project scientist, based at NASA Goddard. Annealing is a heat process that can restore function of instruments and is often done intentionally through built-in heaters on some spacecraft.

Captured on Oct. 20, 2020, as NASA’s OSIRIS-REx spacecraft collected a sample from the surface of asteroid Bennu, this series of 82 images shows the SamCam imager’s field of view as the spacecraft approached and touched Bennu’s surface. OSIRIS-REx’s sampling head touched Bennu’s surface for approximately 6 seconds, after which the spacecraft performed a back-away burn. Credit: NASA/Goddard/University of Arizona

Another welcome surprise, said Simon, came from the spacecraft’s visible and near-infrared spectrometer. Before perihelion, the spectrometer, which mapped the surface composition of Bennu, and will do the same at Apophis, seemed to have a rock from Bennu stuck inside its calibration port. Scientist suspected that some sunlight was blocked from filtering through the instrument after the spacecraft, then called OSIRIS-REx, grabbed a sample from asteroid Bennu on Oct. 20, 2020. By picking up the sample and then firing its engines to back away from Bennu, the spacecraft stirred up dust and pebbles that clung to it.

“But, with enough spacecraft maneuvers and engine burns after sample collection,” Simon said, the rock in the calibration port appears to have been dislodged. Scientists will check the spectrometer again when OSIRIS-APEX swings by Earth on Sept. 25, 2025, for a gravitational boost.

OSIRIS-APEX is now operating normally as it continues its journey toward asteroid Apophis for a 2029 rendezvous. Its better-than-expected performance during the first close perihelion is welcome news. But engineers caution that it doesn’t mean it’s time to relax. OSIRIS-APEX needs to execute five more exceptionally close passes of the Sun — along with three Earth gravity assists — to get to its destination. It’s unclear how the cumulative effect of six perihelions at a closer distance than designed will impact the spacecraft and its components.

The second OSIRIS-APEX perihelion is scheduled for Sept. 1, 2024. The spacecraft will be 46.5 million miles away from the Sun, which is roughly half the distance between Earth and the Sun, and well inside the orbit of Venus.

Learn more about the OSIRIS-APEX mission to Apophis

By Lonnie Shekhtman

NASA’s Goddard Space Flight Center, Greenbelt, Md.

It was bright and green and stretched across the sky.

2 min read

Sols 4195-4198: Feels Like Summer Navcam Right image of Fascination Turret to the north from sol 4193 NASA/JPL-Caltech

Earth planning date: Friday, May 24, 2024

The first sol of this weekend includes an extremely long, 6-hour DAN activity to measure the amount of hydrogen near the surface, in parallel with a standard midday remote science block including: ChemCam LIBS on a smooth, dark rock named “Shadow Lake,” an RMI 7-frame mosaic of the Gediz Vallis ridge base, and two small Mastcam mosaics to document the rock diversity in this area. Since we have so much power to play with, we’re actually staying awake until beginning a custom afternoon Mastcam imaging block to capture the low-sun-angle lighting on Kukenan butte and Milestone Peak ridge in front of us. Should be a butte-iful view. 

On the second sol, it’s time to stretch the old arm! After another standard midday block with more ChemCam and Mastcam remote sensing, the arm will get ready for a full evening of contact science on the workspace blocks we have reachable. There’s no DRT-able rocks here, so MAHLI has two dusty targets named “Second Lake” and “Josephine Lake,” the latter of which will include a 5-frame MAHLI mosaic on the dusty layers. APXS finishes off the evening with two integrations on both Josephine Lake and Second Lake. 

The third sol includes one last midday remote sensing block and an hour-long drive, which is proving tricky to plan. There’s sand, spikey rocks, float rocks, you name it we’re driving over it. If we make it all 38.41 meters, we’ll have crossed a major transition in the bedrock and gotten closer to the white stones to the west. I don’t camp much these days, but if I could go anywhere this holiday weekend it’d be where Curiosity is! Except, you know, the radioactive power source…A fourth sol is included this weekend since Curiosity is on a California holiday schedule, but we make it easy on ourselves by using it as a “REMS-only” sol where the only measurements come from REMS (our local Gale weather station). Enjoy the holiday, US-based earthlings!

Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems

Share

• 
  
  
• 
  
  
• 
  
  
• 
  
  

Details

Last Updated

May 28, 2024

Related Terms

• Blogs

Explore More

4 min read Sols 4193-4194: Stay Overnight? No, Touch-and-Go!

Article


6 days ago

2 min read Sols 1151-1152: Rocky Roads in the Margin Unit

Article


6 days ago

2 min read Sols 4191-4192: Communication

Article


6 days ago

Keep Exploring Discover More Topics From NASA

Mars

Mars is no place for the faint-hearted. It’s dry, rocky, and bitter cold. The fourth planet from the Sun, Mars…

All Mars Resources

Rover Basics

Mars Exploration Science Goals

From May 29 to July 17, 2009, for the first time in its history, each of the five partner agencies participating in the International Space Station Program had a crew member living and working aboard the orbiting facility at the same time. The period also marked the beginning of six-person crew habitation, greatly increasing the time available for utilization. The addition of the international partner elements and life support systems to enable the larger crew size made this 49-day event possible. Although international partner crew members routinely live and work aboard the station, its crew size now expanded to seven, having all the partners represented at the same time remains a unique event in the space station’s history.

Left: Plaque commemorating the signing of the 1988 Inter-Governmental Agreement (IGA) governing the International Space Station partnership. Middle: Signatories of the 1998 IGA visit the Space Station Processing Facility at NASA’s Kennedy Space Center in Florida, posing in front of the Unity Node 1 module being prepared for launch. Right: Joint NASA-Roscosmos crew of STS-88, the first space station assembly mission.

The International Space Station as we know it came into existence in 1993 with the merging of Space Station Freedom, a partnership among the United States, Canada, Japan, and the European Space Agency (ESA), with Russia’s planned Mir-2 space station. In January 1998, representatives of these space agencies met at NASA’s Kennedy Space Center in Florida and signed the Intergovernmental Agreement (IGA) that established the framework for use of the orbiting laboratory. The IGA stipulated the contributions of each agency to the program that entitled them commensurate utilization of the research facility as well as long-duration crew member flight opportunities, beginning when their elements had reached the station. Separate agreements covered the flights of International Partner astronauts on space shuttle assembly flights, usually to accompany elements from their agencies. In orbit construction of the space station began 11 months after the signing of the IGA. From the first assembly mission in December 1998 to March 2001, all components belonged to either NASA or Roscosmos, a fact reflected in the makeup of early space shuttle and expedition crews. The crew of the STS-88, the first space shuttle assembly mission, included five NASA astronauts and cosmonaut Sergei K. Krikalev representing Roscosmos.

Left: STS-96 included Julie Payette, third from left, the first Canadian Space Agency astronaut to visit the space station. Middle: STS-92 included Koichi Wakata, right, the first astronaut from the Japan Aerospace Exploration Agency to visit the space station. Right: The joint NASA-Roscosmos space station Expedition 1 crew.

As early assembly continued, select space shuttle missions included International Partner crew members. The Canadian Space Agency’s (CSA) first astronaut to visit the space station, Julie Payette, flew as one of the seven crew members on the second assembly flight, STS-96 in May-June 1999. The first astronaut from the Japan Aerospace Exploration Agency (JAXA) to visit the station, Koichi Wakata, flew on the fifth assembly flight, STS-92 in October 2000. When the Expedition 1 crew arrived to begin permanent habitation of the space station in November 2000, the crew consisted of NASA astronaut William M. Shepherd, and Roscosmos cosmonauts Krikalev  and Yuri P. Gidenzko. The next six expeditions maintained the two-and-one crew composition, alternating between expeditions, until the impacts from the Columbia accident reduced crew size to two until Expedition 13. During this time, NASA and Roscosmos each had one crew member on board.

Left: STS-100 included Umberto Guidoni, center, the first European Space Agency (ESA) astronaut to visit the space station. Middle: Expedition 13 included Thomas A. Reiter, left, the first ESA astronaut to serve as a long-duration crew member on the space station. Right: STS-119 delivered Koichi Wakata, right, the first astronaut from the Japanese Aerospace Exploration Agency to serve as a long-duration crewmember on the space station.

The first ESA astronaut to visit the space station, Umberto Guidoni from Italy, served as a mission specialist on STS-100 in April 2001. The seven-member crew also included CSA’s Christopher A. Hadfield, who accompanied and helped install the Canadian Space Station Remote Manipulator System, and Yuri V. Lonchakov from Roscosmos, making the STS-100 crew the most internationally diverse shuttle assembly crew. Thomas A. Reiter from Germany arrived at the station aboard STS-121 in July 2006, joining Expedition 13 as ESA’s first long-duration resident crew member, and also returning the onboard crew size back to three. Wakata arrived at the station on STS-119 in March 2009 as JAXA’s first long-duration crew member, joining Expedition 19’s Lonchakov and E. Michael Fincke. Wakata’s arrival set in motion the steps leading to the unique occasion of having each of the five partners with a crew member living and working aboard the space station at the same time.

Left: Expedition 19 crew of Koichi Wakata of the Japan Aerospace Exploration Agency, left, NASA astronaut E. Michael Fincke, and Yuri V. Lonchakov of Roscosmos. Middle: Gennadi I. Padalka of Roscosmos, left, and NASA astronaut Michael M. Barratt of Expedition 19. Right: Canadian Space Agency astronaut Robert B. Thirsk, left, Roman Y. Romanenko of Roscosmos, and European Space Agency astronaut Frank L. DeWinne of Expedition 20.

Eleven days after Wakata’s arrival, Soyuz TMA-14 delivered replacement Expedition 19 crew members NASA astronaut Michael M. Barratt and Gennadi I. Padalka of Roscosmos. On May 29, ESA’s Frank L. DeWinne and CSA’s Robert B. Thirsk, along with Roman Y. Romanenko of Roscosmos arrived aboard Soyuz TMA-15, and all five space station partners had representatives on board. Their arrival began Expedition 20 and the first period of six-person crew residency.

Left: Preflight crew photo of Expedition 20, the first six-person crew on the space station – Michael M. Barratt (NASA), Frank L. DeWinne (ESA), Robert B. Thirsk (CSA), Koichi Wakata (JAXA), Gennadi I. Padalka (Roscosmos), and Roman Y. Romanenko (Roscosmos). Middle: Inflight photo of the Expedition 20 crew. Right: The Expedition 20 crew members put their heads together.

The period of full international representation proved brief, however, lasting just 49 days, and remains unique to this day. Wakata broke up the party on July 17 when he exchanged places with NASA astronaut Timothy L. Kopra who arrived aboard STS-127. Barratt and Padalka left on Oct. 11, replaced by another NASA-Roscosmos crew. Finally, Romanenko, DeWinne, and Thirsk left on Dec. 1, replaced after a brief gap by a crew consisting of a NASA astronaut, a JAXA astronaut, and a representative of Roscosmos.

Explore More 18 min read 40 Years Ago: NASA Selects its 10th Group of Astronauts Article 5 days ago 21 min read 55 Years Ago: Two Months Until the Moon Landing Article 1 week ago 16 min read 15 Years Ago: STS-125, the Final Hubble Servicing Mission Article 2 weeks ago

While NASA promotes the availability of EAP counselors at each Center, there may be reasons when, during a mental health crisis, employees do not think about EAP or cannot remember how to access.

Now, the Suicide and Crises Lifeline (https://988lifeline.org/) is available to anyone, anytime nationwide by calling or texting three numbers from your cell phone “988”. Please check out their link for more information about the Lifeline and additional mental health resources.

For  MAF Employee Assistance Program Office  support contact Porter Pryor at porter.j.pryor@nasa.gov or call or text 228-363-4910.  If you need support grieving a recent or past death of a friend or family member, consider joining the monthly Grief Support Group for SSC/NSSC/MAF/MSFC employees (via NASA Teams) by contacting Porter Pryor.

Additional resources and education available through NASA Occupational Health’s Health4Life link:

Mission: HEALTH / Health 4 Life – Home (sharepoint.com)

When you think about personal property, your home, clothes, and electronic devices probably come to mind. For NASA, personal property comprises government-owned government-held assets ranging from laptops to spacecraft and space station components. Managing the financial records for these assets is the responsibility of the Property Accounting Team, which includes Personal Property Accountant Britney Tang.

Tang sits within the Accounting Services Office of Johnson Space Center’s Office of the Chief Financial Services Officer (OCFO). She works with her colleagues to determine which NASA-held assets must be tracked over time versus expensed, and to ensure those assets are reported appropriately on Johnson’s financial statements.

Official portrait of Britney Tang.NASA/Josh Valcarcel

While she has only held her civil servant position for a few months, Tang is no stranger to Johnson or the OCFO. She completed five rotations with NASA’s Pathways Program between 2021 and 2023, including two stints as a property accounting intern for her current office. “I jumped around a bit as an intern because I really wanted to have a full understanding of NASA’s whole business,” she said. “It made things click to see the entire process of how funds are being used and recorded throughout the agency.” Tang particularly enjoyed her rotations with the Property Accounting Team and feels lucky to rejoin them as a full-time employee.

As an accounting major at the University of Houston’s C.T. Bauer College of Business, Tang planned to work for a public accounting firm or a private company when she graduated, until she stumbled upon a Pathways internship opportunity. “It was in a newsletter that my school put out, which I rarely opened, but one day I did, and I saw the call for applications,” she said. “I thought I might as well throw my hat into the ring and see where it got me.”

Britney Tang tries on a spacesuit glove and attempts basic astronaut tasks, like latching and unlatching tethers, during Johnson Space Center’s Intern, Innovation, and Industry Day on July 13, 2023.Image courtesy of Britney Tang

Tang believes her experience highlights an important opportunity for NASA to attract more diverse talent by reaching out to students enrolled in a wider variety of schools and academic fields. “When you think of NASA, you think of engineers and rockets. I think that’s why a lot of people in business specifically do not consider NASA as a career option, because they forget that we do need mission support operations to keep things running,” she said. “I’m really passionate about telling people about the opportunities at NASA, especially on the business side.”

That passion prompted Tang to work with ASIA ERG to host a virtual event with the University of Houston’s Asian Business Student Association last year. At the time, she was participating in the group’s education and outreach and social cohorts as a Pathways intern. Tang developed a presentation for the event that provided overviews of Johnson’s business organizations, describing each organization’s work and related career opportunities for students. She also recruited several employees from those organizations to participate in the presentation and a brief panel discussion that followed.

Britney Tang participates in a payload-capture simulation from a mockup of the International Space Station’s cupola during an intern tour of Johnson’s systems engineering simulators in March 2023. Image courtesy of Britney Tang

Tang said that she has never felt like a minority on the teams she has been a part of, noting that her current team is almost entirely female and includes several people of color, but she knows this may not be every Johnson employee’s experience. During one intern orientation session, Tang observed that she was one of five or six women in a room of 30 people. “I did not like that feeling and I expressed that to the Pathways coordinators,” she said. “I think if people don’t see someone similar to them, or someone they can relate to, it’s harder for them to feel like they can apply.”

A self-described foodie, Tang said that showing openness and acceptance of teammates’ ethnic foods is one way that every Johnson employee can promote cultural understanding and inclusivity. Asian American families often share stories about bringing Asian food to school for lunch as kids and getting teased by other students because it smelled different, she said, adding that she hopes the growing popularity of ethnic cuisines will help put an end to those experiences. Telling her fellow Pathways interns that she enjoys trying different foods around Houston helped her build connections with them, and many approached her with questions about where they should go and what they should try. “The easiest way to start a conversation is to talk about food, and food is very integral to a culture,” she said.

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) This computer-generated 3D model of Venus’ surface shows the volcano Sif Mons, which is exhibiting signs of ongoing activity. Using data from NASA’s Magellan mission, Italian researchers detected evidence of an eruption while the spacecraft orbited the planet in the early 1990s.NASA/JPL-Caltech

An analysis of data from Magellan’s radar finds two volcanoes erupted in the early 1990s. This adds to the 2023 discovery of a different active volcano in Magellan data.

Direct geological evidence of recent volcanic activity on Venus has been observed for a second time. Scientists in Italy analyzed archival data from NASA’s Magellan mission to reveal surface changes indicating the formation of new rock from lava flows linked to volcanoes that erupted while the spacecraft orbited the planet. Managed by NASA’s Jet Propulsion Laboratory in Southern California, Magellan mapped 98% of the planet’s surface from 1990 to 1992, and the images it generated remain the most detailed of Venus to date.

“Using these maps as a guide, our results show that Venus may be far more volcanically active than previously thought,” said Davide Sulcanese of d’Annunzio University in Pescara, Italy, who led the study. “By analyzing the lava flows we observed in two locations on the planet, we have discovered that the volcanic activity on Venus could be comparable to that on Earth.”

This latest discovery builds on the historic 2023 discovery of images from Magellan’s synthetic aperture radar that revealed changes to a vent associated with the volcano Maat Mons near Venus’ equator. The radar images proved to be the first direct evidence of a recent volcanic eruption on the planet. By comparing Magellan radar images over time, the authors of the 2023 study spotted changes caused by the outflow of molten rock from Venus’ subsurface filling the vent’s crater and spilling down the vent’s slopes.

Scientists study active volcanoes to understand how a planet’s interior can shape its crust, drive its evolution, and affect its habitability. The discovery of recent volcanism on Venus provides a valuable insight to the planet’s history and why it took a different evolutionary path than Earth.

Before starting its journey to Venus, NASA’s Magellan spacecraft was released while in Earth orbit by Space Shuttle Atlantis’ STS-30 mission. Captured in this May 4, 1989, photo, Magellan was the first planetary spacecraft to be launched from the shuttle.NASA Radar Backscatter

For the new study, published in the journal Nature Astronomy, the researchers likewise focused on archival data from Magellan’s synthetic aperture radar. Radio waves sent by the radar traveled through Venus’ thick cloud cover, then bounced off the planet’s surface and back to the spacecraft. Called backscatter, these reflected radar signals carried information about the rocky surface material they encountered.

The two locations studied were the volcano Sif Mons in Eistla Regio and the western part of Niobe Planitia, which is home to numerous volcanic features. By analyzing the backscatter data received from both locations in 1990 and again in 1992, the researchers found that radar signal strength increased along certain paths during the later orbits. These changes suggested the formation of new rock, most likely solidified lava from volcanic activity that occurred during that two-year period. But they also considered other possibilities, such as the presence of micro-dunes (formed from windblown sand) and atmospheric effects that could interfere with the radar signal.

To help confirm new rock, the researchers analyzed Magellan’s altimetry (surface height) data to determine slope of the topography and locate obstacles that lava would flow around.

“We interpret these signals as flows along slopes or volcanic plains that can deviate around obstacles such as shield volcanoes like a fluid,” said study co-author Marco Mastrogiuseppe of Sapienza University of Rome. “After ruling out other possibilities, we confirmed our best interpretation is that these are new lava flows.”

Using flows on Earth as a comparison, the researchers estimate new rock that was emplaced in both locations to be between 10 and 66 feet (3 and 20 meters) deep, on average. They also estimate that the Sif Mons eruption produced about 12 square miles (30 square kilometers) of rock — enough to fill at least 36,000 Olympic-size swimming pools. The Niobe Planitia eruption produced about 17 square miles (45 square kilometers) of rock, which would fill 54,000 Olympic swimming pools. As a comparison, the 2022 eruption of Mauna Loa in Hawaii, Earth’s largest active volcano, produced a lava flow with enough material to fill 100,000 Olympic pools.

“This exciting work provides another example of volcanic change on Venus from new lava flows that augments the vent change Dr. Robert Herrick and I reported last year,” said Scott Hensley, senior research scientist at JPL and co-author of the 2023 study. “This result, in tandem with the earlier discovery of present-day geologic activity, increases the excitement in the planetary science community for future missions to Venus.”

Figuring Out Volcanoes

Hensley is the project scientist for NASA’s upcoming VERITAS mission, and Mastrogiuseppe is a member of its science team. Short for Venus Emissivity, Radio science, InSAR, Topography, And Spectroscopy, VERITAS is slated to launch early next decade, using a state-of-the-art synthetic aperture radar to create 3D global maps and a near-infrared spectrometer to figure out what Venus’ surface is made of while also tracking volcanic activity. In addition, the spacecraft will measure the planet’s gravitational field to determine its internal structure.

“These new discoveries of recent volcanic activity on Venus by our international colleagues provide compelling evidence of the kinds of regions we should target with VERITAS when it arrives at Venus,” said Suzanne Smrekar, a senior scientist at JPL and principal investigator for VERITAS. “Our spacecraft will have a suite of approaches for identifying surface changes that are far more comprehensive and higher resolution than Magellan images. Evidence for activity, even in the lower-resolution Magellan data, supercharges the potential to revolutionize our understanding of this enigmatic world.”

More About the Mission

NASA’s VERITAS mission was selected in 2021 under NASA’s Discovery Program. Mission partners include Lockheed Martin Space, the Italian Space Agency, the German Aerospace Center, and Centre National d’Études Spatiales in France. The Discovery Program is managed by the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the Planetary Science Division of NASA’s Science Mission Directorate in Washington.

News Media Contacts

Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov

Karen Fox / Charles Blue
NASA Headquarters
202-358-1600 / 202-802-5345
karen.c.fox@nasa.gov / charles.e.blue@nasa.gov

Giuseppina Piccirilli
Agenzia Spaziale Italiana
+39 06 85 67 431 / 887 / 655
stampa@asi.it

2024-073      

Share

Details Last Updated May 27, 2024 Related Terms

• Jet Propulsion Laboratory
• Magellan
• Planetary Geosciences & Geophysics
• Planetary Science
• Planetary Science Division
• Venus
• VERITAS (Venus Emissivity, Radio Science, InSAR, Topography & Spectroscopy)
• Volcanoes

Explore More 6 min read New Images From Euclid Mission Reveal Wide View of the Dark Universe Article 5 days ago 4 min read NASA’s Psyche Fires Up Its Sci-Fi-Worthy Thrusters Article 6 days ago 7 min read NASA Tool Gets Ready to Image Faraway Planets Article 7 days ago Keep Exploring Discover Related Topics

Missions

Humans in Space

Climate Change

Solar System

Can a gas cloud eat a galaxy?

It seemed like night, but part of the sky glowed purple.

Rocket Lab’s Electron rocket lifted off from Launch Complex 1 at Māhia, New Zealand at 7:41 p.m. NZST May 25, 2024 (3:41 a.m. EDT) carrying a small satellite for NASA’s PREFIRE (Polar Radiant Energy in the Far-InfraRed Experiment) mission.Rocket Lab

The first of a pair of climate satellites designed to study heat emissions at Earth’s poles for NASA is in orbit after lifting off atop Rocket Lab’s Electron rocket from the company’s Launch Complex 1 in Māhia, New Zealand at 7:41 p.m. NZST (3:41 a.m. EDT) on Saturday.

The agency’s PREFIRE (Polar Radiant Energy in the Far-InfraRed Experiment) mission consists of two shoebox-size cube satellites, or CubeSats, that will measure the amount of heat Earth radiates into space from two of the coldest, most remote regions on the planet. Data from the PREFIRE mission will help researchers better predict how Earth’s ice, seas, and weather will change in a warming world.

“NASA’s innovative PREFIRE mission will fill a gap in our understanding of the Earth system – providing our scientists a detailed picture of how Earth’s polar regions influence how much energy our planet absorbs and releases,” said Karen St. Germain, director of NASA’s Earth Science Division in Washington. “This will improve prediction of sea ice loss, ice sheet melt, and sea level rise, creating a better understanding of how our planet’s system will change in the coming years — crucial information to farmers tracking changes in weather and water, fishing fleets working in changing seas, and coastal communities building resilience.”

Ground controllers successfully established communications with the CubeSat at 8:48 EDT. The second PREFIRE CubeSat will set off on its own Electron rocket from Launch Complex 1 in the coming days. Following a 30-day checkout period during which engineers and scientists will make sure both CubeSats are working normally, the mission is expected to operate for 10 months.

At the heart of the PREFIRE mission is Earth’s energy budget – the balance between incoming heat energy from the Sun and the outgoing heat given off by the planet. The difference between the two is what determines the planet’s temperature and climate. A lot of the heat radiated from the Arctic and Antarctica is emitted as far-infrared radiation, but there is currently no detailed measurement of this type of energy.

The water vapor content of the atmosphere, along with the presence, structure, and composition of clouds, influences the amount of far-infrared radiation that escapes into space from Earth’s poles. Data collected from PREFIRE will give researchers information on where and when far-infrared energy radiates from the Arctic and Antarctic environments into space.

“The PREFIRE CubeSats may be small, but they’re going to close a big gap in our knowledge about Earth’s energy budget,” said Laurie Leshin, director, NASA’s Jet Propulsion Laboratory in Southern California. “Their observations will help us understand the fundamentals of Earth’s heat balance, allowing us to better predict how our ice, seas, and weather will change in the face of global warming.”

The mission’s CubeSats each carry an instrument called a thermal infrared spectrometer, which use specially shaped mirrors and sensors to measure infrared wavelengths. Miniaturizing the instruments to fit on CubeSats necessitated downsizing some parts while scaling up other components.

“Our planet is changing quickly, and in places like the Arctic, in ways that people have never experienced before,” said Tristan L’Ecuyer, PREFIRE’s principal investigator, University of Wisconsin, Madison. “NASA’s PREFIRE will give us new measurements of the far-infrared wavelengths being emitted from Earth’s poles, which we can use to improve climate and weather models and help people around the world deal with the consequences of climate change.”

NASA’s Launch Services Program, based out of the agency’s Kennedy Space Center in Florida, in partnership with NASA’s Earth System Science Pathfinder Program is providing the launch service as part of the agency’s Venture-class Acquisition of Dedicated and Rideshare (VADR) launch services contract.

The PREFIRE mission was jointly developed by NASA and the University of Wisconsin-Madison. NASA JPL manages the mission for the agency’s Science Mission Directorate and provided the spectrometers. Blue Canyon Technologies built the CubeSats and the University of Wisconsin-Madison will process the data the instruments collect. The launch services provider is Rocket Lab USA Inc. of Long Beach, California.

To learn more about PREFIRE, visit:

https://science.nasa.gov/mission/prefire/

-end-

Karen Fox / Elizabeth Vlock

Headquarters, Washington

202-358-1600 / 202-358-1600

karen.c.fox@nasa.gov / elizabeth.a.vlock@nasa.gov

Jane J. Lee / Andrew Wang

Jet Propulsion Laboratory, Pasadena, Calif.

818-354-0307 / 626-379-6874

jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov

Share

Details Last Updated May 25, 2024 EditorJennifer M. DoorenLocationNASA Headquarters Related Terms

• PREFIRE (Polar Radiant Energy in the Far-InfraRed Experiment)

North Celestial Aurora

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) Representatives of NASA’s Transformative Aeronautics Concepts Program (TACP) pose with students and faculty from the University of Central Florida (UCF) in Orlando who are participating in the agency’s University Leadership Initiative (ULI). From left: Ramees Khaleel Rahman; John Cavolowsky, NASA’s Transformative Aeronautics Concepts Program director; Marc Heinrich; Andrew Provenza, NASA’s University Innovation deputy project manager for tchnology; Connor Wall; Lucas Cavalcante; Andrew Menendez; Jayanta Kapat, principal investigator of UCF’s ULI project; Claire-Phonie Silaire; Koushik Datta, NASA’s University Innovation project manager; Marcel Otto, UCF’s ULI project manager.

Representatives of NASA’s Transformative Aeronautics Concepts Program (TACP) recently shared information about their work to develop innovation and advance aviation and space exploration with students at the University of Central Florida in Orlando.

Here are some images of the event showing NASA team members interacting with students and faculty during the April Town Hall.

TACP at UCF Image Carousel Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More 4 min read Aviary: A New NASA Software Platform for Aircraft Modelling Article 2 weeks ago 3 min read NASA Licenses 3D-Printable Superalloy to Benefit US Economy Article 3 weeks ago 2 min read ULI Round 7 Awards Article 3 months ago Keep Exploring Discover More Topics From NASA

Missions

Artemis

University Innovation Project

Aeronautics STEM

Share

Details Last Updated May 24, 2024 EditorJim BankeContactJim Bankejim.banke@nasa.gov Related Terms

• Transformative Aeronautics Concepts Program
• University Innovation
• University Leadership Initiative

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater) Composites Consortium team members gathered during May 2024 at NASA’s Langley Research Center in Virginia for a technical review of all tasks in progress for the Hi-Rate Composite Aircraft Manufacturing project.

NASA and its partners in the Advanced Composites Consortium gathered at the agency’s Langley Research Center in Hampton, Virginia, May 7-9.

Team members from 20 organizations across the country recently discussed progress on all technology development tasks underway in NASA’s Hi-Rate Composite Aircraft Manufacturing (HiCAM) project. The project is competing manufacturing approaches that reduce labor, equipment, and tooling costs without compromising strength or safety.

Results will help determine which technologies will have the greatest impact on the manufacturing rate and allow downselect for the demonstration phase of the project beginning this fall.

The HiCAM project addresses an aviation industry need for more rapid production of composite aircraft to meet increasing global demand for lightweight transport aircraft.

Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More 4 min read NASA, Industry to Start Designing More Sustainable Jet Engine Core Article 1 week ago 2 min read NASA Noise Prediction Tool Supports Users in Air Taxi Industry Article 2 months ago 4 min read NASA Instruments Will Listen for Supersonic X-59’s Quiet ‘Thump’ Article 3 months ago Keep Exploring Discover More Topics From NASA

Advanced Air Vehicles Program

Artemis

Missions

Aeronautics STEM

Share

Details Last Updated May 24, 2024 EditorJim BankeContactJim Bankejim.banke@nasa.gov Related Terms

• Advanced Air Vehicles Program
• Hi-Rate Composite Aircraft Manufacturing

Representatives from 24 of the Artemis Accords signatories met May 21-23, 2024, for a workshop hosted at the John H. Chapman Space Centre (CSA Headquarters) in Longueuil, Quebec.CSA (Canadian Space Agency)

NASA participated in the second international face-to-face workshop this week among Artemis Accords signatories, which featured space officials from two dozen nations focused on advancing the principles for the safe, peaceful, and responsible exploration of the Moon, Mars and beyond. This year’s workshop was hosted by CSA (Canadian Space Agency) at their headquarters in Montreal May 21-23.

Since the Artemis Accords were created nearly four years ago, 39 countries have joined the United States in a voluntary commitment to engage in transparent and responsible behavior in space. The accords are meant to push humanity’s reach farther safely and sustainably into space than ever before and build on more than 23 years of continuous human presence aboard the International Space Station.

“The Artemis Accords represent a shared vision for humanity’s exploration of space —one that transcends borders and fosters unity in our quest to expand our understanding of the cosmos,” said NASA Deputy Administrator Pam Melroy, who participated virtually to jointly kick-off the workshop with CSA President Lisa Campbell. “The days of going to space alone are long over. We are in a new age where nations globally go to space to both explore deeper and gain better understanding about our place in the universe.”

During workshop, participants from 24 countries engaged in robust discussions and conducted a tabletop exercise centered on further defining and implementing key tenets, including considering views on non-interference, interoperability, and scientific data sharing among nations.

“The Artemis Accords are an important part of humanity’s future in space and Canada is very much committed to these principles. As we explore beyond Earth, we must do so in ways that are safe and sustainable, for the benefit of humanity and future generations. It was an honour to welcome brilliant minds from around the world to discuss how to conduct present and future space exploration activities safely, sustainably, and transparently through the application of the Artemis Accords,” said Campbell.

For example, during the workshop participants delved more deeply into topics such as non-interference and interoperability. These discussions build upon prior work such as an initial set of mission data parameters agreed to by the signatories last October. The data parameters identify necessary information about planned lunar surface missions including expected launch dates, the general nature of activities, and the landing location.

Sharing such information will support safer lunar operations by ensuring signatories respective missions do not inadvertently interfere with each other. Transparency and communication are keys to peaceful exploration, and the Artemis Accords signatories are committed to sharing information about their activities and outcomes through the United Nations of Committee on the Peaceful Uses of Outer Space (UNCOPUOS) and other appropriate channels.

The commitments undertaken under the Artemis Accords, and the significant efforts by the signatories to advance implementation of these principles, are essential to the success of the Artemis campaign for NASA and its partners, as well as for the success of the safe and sustainable exploration activities of the other Accords signatories.

As the Artemis Accords workshop concluded May 23, participants reaffirmed their commitment to upholding the principles outlined in the Artemis Accords and to continue working collaboratively. The first workshop was hosted by Poland in 2023. Additional countries are expected to sign the Artemis Accords in the weeks and months ahead. Signatory principals will gather again for face-to-face discussions on the margins of the International Astronautical Congress in October.

The United States and seven other nations were the first to sign the Artemis Accords in 2020, which identified an early set of principles that promote the beneficial use of space for all humanity, grounded in the Outer Space Treaty and other agreements including the Registration Convention, the Rescue and Return Agreement, as well as best practices and norms of responsible behavior that NASA and its partners have supported, including the public release of scientific data.

For more information about the Artemis Accords, visit:

https://www.nasa.gov/artemis-accords/

-end-

Amber Jacobson / Jennifer Dooren
Headquarters, Washington
202-358-1600
amber.c.jacobson@nasa.gov / jennifer.m.dooren@nasa.gov

Share

Details Last Updated May 24, 2024 EditorJennifer M. DoorenLocationNASA Headquarters Related Terms

• Office of International and Interagency Relations (OIIR)

Jennifer Scott Williams embodies leadership, innovation, and excitement for life. Her career has been a testament to her unwavering passion and versatility, navigating through various roles and significantly contributing to the agency’s milestones and evolution. In her 23 years at NASA, she has combined engineering, business, science communications, and leadership all into one.    

Currently in the Center Director’s Office, Williams serves as NASA Johnson Space Center Director Vanessa Wyche’s assistant for technical integration, supporting meetings such as readiness reviews for the International Space Station and Commercial Crew Programs. Her role also involves coordinating skip-level meetings for Dare | Unite | Explore and overseeing senior staff meetings to ensure that leadership remains informed about the activities happening across the center.  

Official portrait of Jennifer Scott Williams. Credit: NASA/Josh Valcarcel 

She also plays a role in the International Space Station Program’s Research Integration Office, ensuring crews aboard the space station have the tools they need to complete their research. 

“Like many of our laboratories where astronauts conduct their research, understanding the engineering components of the facilities we use on board is crucial,” said Williams. “Understanding the science is also critical,” she added. “It adds meaning to our work when we help execute the science onboard and communicate the creative insights and results from the experiments conducted. Being a good communicator is extremely important and creativity makes that message real and mean something to the public.” 

Jennifer Scott Williams (front) during a senior staff outreach event at the Remembering Columbia Museum in Hemphill, Texas.

Her journey also included groundbreaking work on the Boeing Starliner spacecraft, where she served as the instrumentation and communications officer on the Boeing Mission Operations Team. Her efforts established operational foundations that will shape its future space missions. Williams was instrumental in developing the vehicle communications systems, understanding its operations, creating simulations, coding, and comprehending the computer systems, addressing all the fundamental aspects necessary for the spacecraft. 

Beyond her technical contributions, Williams is deeply committed to inspiring the next generation of explorers. She also managed the Minority University Research and Education Project, encouraging students of color to engage in STEM fields.  

She led a team that collaborated with students, teachers, and educational institutions through the Pre-Service Teacher Program. Williams said that working in the Office of STEM Engagement was a new experience that became life-changing for her. “I really rediscovered a passion that I have for students and education,” she said. “I love being able to help interns navigate the NASA environment and help people of color be able to apply for NASA jobs. It takes all perspectives to accomplish our mission.” 

Williams earned dual bachelor’s degrees in mathematics and electrical engineering from Spelman College and the Georgia Institute of Technology. She later received a master’s degree in electrical engineering from the University of Houston. She belongs to the Spelman College National Alumni Association and holds a lifetime membership in the National Society of Black Engineers. 

Jennifer Scott Williams’ headshot in the 2024 International Space Station calendar.Credit: NASA/Bill Stafford  

Williams is an advocate for youth interested in pursuing STEM careers. Her advice is, “Come on and do it. We are out here,” she added “I love that we are embracing our differences instead of shunning differences because having people with different backgrounds, personalities, insights, and perspectives is what’s going to help us get back to the Moon.”     

“For the Artemis Generation, we need creative minds,” she said. “We need artists, scientists, engineers, technologists, physicians, attorneys, and financial connoisseurs. This next generation is going to have to be open-minded thought seekers. They need to be willing to do things that we have never done before and take the risks so that we can put boots on the Moon and Mars.” 

Jennifer Scott Williams with her family at Kennedy Space Center in Florida for the launch of NASA’s SpaceX Commercial Resupply Service mission to the International Space Station on March 15, 2023.

Williams also plays an integral role in Dare | Unite | Explore initiatives. She works with senior leadership to make sure the workforce has professional mobility and is able to get the training and resources for new opportunities. “We want to encourage employees to try new things, to learn, and to grow in different organizations,” she said. “Dare | Unite | Explore ensures that the Johnson workforce is fully supported in our efforts as we grow and develop and that our facilities and processes can support us and are in alignment with our future initiatives.”   

“I never really thought I would work at NASA, but when I came here to interview, they put me in the shuttle simulator and I was hooked,” she said. “I encourage my children to pursue careers in STEM because it has been so beneficial to me throughout my life. The people that I have come across in my time here have been phenomenal. It makes me want to keep coming to work.”  

As a member of the Mars Architecture Team, Clare Luckey is one of the people at the forefront of designing the first crewed mission to the Red Planet. Her current work involves helping to develop the vision for the initial segment of Mars exploration missions. She also has been named one of Forbes’ 30 under 30 Class of 2024 in the Science category. Her commitment extends beyond the cosmos as she is deeply involved in community outreach, inspiring students to aim for the stars in space careers and encouraging diversity in STEM.  

Starting her journey as an intern at NASA’s Johnson Space Center Operations in fall 2018, Luckey’s career trajectory has been nothing short of meteoric. She began her career as a contractor at Barrios Technology, focusing on cargo integration for the International Space Station Program, then transitioned to a civil servant position in Center Operations by late 2020. Currently serving in the Exploration Mission Planning Office, Luckey’s role is critical not just in Mars exploration but also in the Artemis missions, where she contributes to Lunar Mission Planning in the Mission Analysis and Integrated Assessments team. 

Official portrait of Clare Luckey. Credit: NASA/Josh Valcarcel

Luckey’s innovative thinking is especially crucial as she navigates the complexities of planning travel to Mars. Her ability to compare and adapt strategies from near-term missions like Artemis to the long-term objectives of Mars colonization highlights her unique insight and adaptability. “Mars missions are more open to change because they are far in the future,” said Luckey. “We are still in the process of figuring out not only how to make decisions, but what decisions to make.” 

Her influence extends far beyond engineering. Luckey’s engagement with global space leaders at the Space Symposium and her contributions as a panelist at the American Institute of Aeronautics and Astronautics Science and Technology Forum exemplify her as a thought leader in aerospace. She also participated in the Space Generation Advisory Council, a board that advises the United Nations on next-generation space exploration concepts. “All of these opportunities have given me different insights into the larger space industry and space economy,” she said. 

Clare Luckey, member of the Mars Architecture Team, shares her passion with NASA’s Johnson Space Center employees at the JSC Town Hall on Aug. 23, 2023.Credit: NASA/Riley McClenaghan 

Reflecting on her journey, Luckey attributes her passion for space exploration to a middle school project, “Future Cities,” where she and her friends designed a futuristic Mars city. The project ignited her imagination and inspired her to think critically and creatively about the future. “It’s important to build the foundations of mathematics and science at a young age,” she said. “I am really passionate about getting other people who look like me involved in the space industry.” 

Luckey’s involvement with the National Society of Black Engineers and her efforts to mentor and help students with school projects gives her great joy. “NASA can invest in the next generation by building a sustainable pipeline alongside sustainable space architecture,” she said. “You have to invest in communities and education so that kids grow up participating in a culmination of activities that make them want to be a part of NASA.” She believes that persistence, passion, and creativity are the top qualities for someone to excel in the space exploration industry.  

As a vocal advocate for diversity in the space industry, Luckey emphasizes the importance of community and mentorship within NASA and beyond. “I try to reach out to people and build that community because it is important,” she said. “That’s one of the things that keeps people coming to work – no matter where you work. It’s not the work, it’s the people that keep you coming back. I work with a lot of great people that have built that NASA community.” 

Clare Luckey at the NASA Human Research Program Investigators’ Workshop 2023, “To the Moon: The Next Golden Age of Human Spaceflight,” at the Galveston Island Convention Center on Feb. 8, 2023. Credit: NASA/Josh Valcarcel 

Luckey’s advice to aspiring space explorers is, “Just try. Even when you don’t think you’re capable or don’t think you know enough, you will learn as you go.” She also encourages students to search out opportunities and get involved at a young age. “There’s no wrong answer. Just do what you’re interested in, put effort into it, and you’ll end up where you want to go,” she said. 

Her favorite part about working at NASA is the outlandishness of it all, she said. “People at NASA are really trying to build the future. The work we do here is amazing and not to be overlooked.” She is looking forward to the Artemis missions because this time is a completely new paradigm. “With Artemis, we’re going to the Moon to stay and to build sustainable architecture,” said Luckey. “We’re going to push forward. I am really excited to see how it turns out, and the international collaboration will be amazing for us.” 

Her enthusiasm for the Artemis campaign and the future of international space collaboration shines through her work, envisioning a new era of lunar exploration and beyond. “I am grateful to be here,” she said. “The most important thing to me is to be humble and personable. I want to be someone that is approachable, helpful, and easy to learn from so that I can be a mentor to the next generation of students, in the same way that I had mentors.” 

Clare Luckey, an engineer at NASA’s Johnson Space Center in Houston.Credit: NASA/Bill Stafford 

Helen Ling was a supervisor for the computing group at NASA's Jet Propulsion Laboratory in the 1960s. She was influential in the inclusion of women in STEM positions at JPL. Ling encouraged women within the computing group to attend night school in order to obtain degrees that would allow them more professional opportunities within JPL. A pioneer for women's rights in the workplace, Helen Ling was so admired in the computing group that those who worked under her lovingly referred to themselves as "Helen's girls." Many of them went on to become computer scientists and engineers within JPL thanks to the mentorship and guidance of Helen Ling.

NASA/JPL-Caltech

Helen Ling, seen here in a photo from Feb. 16, 1973, was influential in the inclusion of women in STEM positions at NASA’s Jet Propulsion Laboratory. After majoring in Mathematics at the University of Notre Dame—the only woman to do so at the time—Ling joined her brother in working at JPL. She became a supervisor for the computing group in the 1960s, a team who was responsible for performing trajectory calculations.

Ling encouraged women within the computing group to attend night school to earn degrees that would allow them more professional opportunities within JPL. A pioneer for women’s rights in the workplace, Helen Ling was so admired in the computing group that those who worked under her lovingly referred to themselves as “Helen’s girls.” Many of “Helen’s girls” went on to become computer scientists and engineers within JPL thanks to the mentorship and guidance of Helen Ling.

Throughout her time at JPL, Ling developed software for the IRAS, Magellan, TOPEX/Poseidon, and Mars Observer missions, and retired in 1994.

Image Credit: NASA/JPL-Caltech