NASA’s SpaceX Crew-9 Members Pose for Portrait

NASA astronauts Butch Wilmore, Nick Hague, and Suni Williams, and Roscosmos cosmonaut Aleksandr Gorbunov – the members of NASA’s SpaceX Crew-9 mission – smile at the camera in this Feb. 19, 2025, photo. While aboard the International Space Station, Hague, Williams, and Wilmore completed more than 900 hours of research between more than 150 unique scientific experiments and technology demonstrations during their stay aboard the orbiting laboratory.

Wilmore, Hague, Williams, and Gorbunov are set to return to Earth on Tuesday, March 18, with splashdown set for approximately 5:57 p.m. EDT.

Watch NASA’s Crew-9 return coverage at 4:45 p.m. EDT Tuesday on NASA+.

Image credit: NASA/Nick Hague

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Monika Luabeya

NASA Invites Media to View Wildland Fire Technology Flight Test

NASA will conduct a live flight test of aircraft performing simulated wildland fire response operations using a newly developed airspace management system at 9 a.m. PDT on Tuesday, March 25, in Salinas, California.

NASA’s new portable airspace management system, part of the agency’s Advanced Capabilities for Emergency Response Operations (ACERO) project, aims to significantly expand the window of time crews have to respond to wildland fires. The system provides the air traffic awareness needed to safely send aircraft – including drones and remotely piloted helicopters – into wildland fire operations, even during low-visibility conditions. Current aerial firefighting operations are limited to times when pilots have clear visibility, which lowers the risk of flying into the surrounding terrain or colliding with other aircraft. This restriction grounds most aircraft at night and during periods of heavy smoke.

During this inaugural flight test, researchers will use the airspace management system to coordinate the flight operations of two small drones, an electric vertical takeoff and landing aircraft, and a remotely piloted aircraft that will have a backup pilot aboard. The drones and aircraft will execute examples of critical tasks for wildland fire management, including weather data sharing, simulated aerial ignition flights, and communications relay.

Media interested in viewing the ACERO flight testing must RSVP by 4 p.m. Friday, March 21, to the NASA Ames Office of Communications by email at: arc-dl-newsroom@mail.nasa.gov or by phone at 650-604-4789. NASA will release additional details, including address and arrival logistics, to media credentialed for the event. A copy of NASA’s media accreditation policy is online.

NASA’s ACERO researchers will use data from the flight test to refine the airspace management system. The project aims to eventually provide this technology to wildland fire crews for use in the field, helping to save lives and property. This project is managed at NASA’s Ames Research Center in California’s Silicon Valley.

For more information on ACERO, visit:

https://go.nasa.gov/4bYEzsD

-end-

Rob Margetta
Headquarters, Washington
202-358-1600
robert.j.margetta@nasa.gov

Hillary Smith
Ames Research Center, Silicon Valley
650-604-4789
hillary.smith@nasa.gov

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Jessica Taveau

NASA Invites Media to 62nd Annual Goddard Space Science Symposium

Media are invited to meet leaders in the space community during the 62nd annual Goddard Space Science Symposium, taking place from Wednesday, March 19, to Friday, March 21, at Martin’s Crosswinds in Greenbelt, Maryland. The symposium will also be streamed online.

Hosted by the American Astronautical Society (AAS) in conjunction with NASA’s Goddard Space Flight Center in Greenbelt, the symposium examines the current state and future of space science and space exploration at large by convening leading minds across NASA, other government agencies, policy, academia, and industry – collectively navigating a path forward by identifying the opportunities and challenges ahead.

This year’s theme, “Pathways and Partnerships for U.S. Leadership in Earth and Space Science,” highlights the evolving collaborative landscape between the public and private sectors, as well as how it is helping the United States remain and grow as a leading space power. 

“Earth and space science are complex by nature, with a growing list of public and private enterprises carving out their space,” said Christa Peters-Lidard, co-chair of the symposium planning committee and Goddard’s director of sciences and exploration. “It’s an exciting time as we work to determine the future trajectory of space exploration in this new era, and the Goddard Space Science Symposium is an instrumental tool for gathering the insights of leading experts across a broad spectrum.”

AAS President Ron Birk and Goddard Deputy Center Director Cynthia Simmons will deliver the symposium’s opening remarks on March 19, followed by panels on enabling science and exploration from the Moon to Mars and navigating space science and exploration policy. Greg Autry, associate provost for space commercialization and strategy at the University of Central Florida, will deliver the keynote address. The first day will conclude with an industry night reception.

The second day of the symposium on Thursday, March 20, will feature panels on enhancing U.S. economic leadership through science, the Habitable Worlds Observatory, and the confluence of public science and the private sector. Gillian Bussey, deputy chief science officer for the U.S. Space Force, will serve as the luncheon speaker.

Panels on the third and final day, March 21, will discuss integrating multi-sector data to advance Earth and space science, the Heliophysics Decadal Survey, and the space weather enterprise. Mark Clampin, acting deputy associate administrator for the NASA Science Mission Directorate, will provide the luncheon address.

Media interested in arranging interviews with NASA speakers should contact Jacob Richmond, Goddard acting news chief.

For more information on the Goddard Space Science Symposium and the updated program, or to register as a media representative, visit https://astronautical.org/events/goddard.

For more information on NASA’s Goddard Space Flight Center, visit https://www.nasa.gov/goddard.

Media Contact:
Jacob Richmond
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Jamie Adkins

Observing Storms from Skylab

Skylab 3 astronauts witnessed many spectacular sights during their 858 orbital trips around the Earth in the summer of 1973. One involved watching powerful Hurricane Ellen take shape off the West African coast. “There’s a nice storm down there. She looks pretty big. She’s got a lot of clouds,” said astronaut Alan L. Bean upon viewing the storm from Skylab’s low-Earth orbit.

Knowing they were witnessing something of interest to meteorologists on Earth, Bean and his fellow Skylab crew members captured stereo photographs of the storm using cameras aboard the space station. Meteorologists later used these images, which provided three-dimensional data, to help them understand how the clouds in tropical systems formed and functioned.

Like the Skylab 3 crew’s photographs of Hurricane Ellen, the lightning observations of Skylab 4 astronaut Edward G. Gibson were also used by meteorologists to understand regional weather phenomena. While gazing down at a storm over South America’s Andes Mountains, Gibson noted that the thunderstorm he observed generated recognizable lightning patterns over a 500-square-mile region.

“A few things impressed me here: one is the fact that they could go off simultaneously or near simultaneously over a large distance—sympathetic lightning bolts, if you will, analogous to sympathetic flares on the sun. And that we do get periods of calm between periods of very high activity. Some sort of collective phenomenon appears to be at work,” Gibson recalled.

The photographs of Hurricane Ellen and Gibson’s notes about lightning patterns are just two of many valuable meteorological observations and recordings astronauts made during Skylab’s three crewed missions. All told, astronaut-conducted Earth studies provided important regional, also known as mesoscale, weather data that improved storm forecasting.

Along with providing valuable data to meteorologists, the notable findings of the Skylab astronauts supported the argument of the era’s scientists and mission planners who insisted that there was no adequate replacement for intelligent human observers in space.

Perhaps the authors of Living and Working in Space: A History of Skylab  put it best when they wrote: “Man’s ability to discriminate, to select the important features of a wide vista, and to respond effectively to unexpected events constituted his greatest contribution to orbital investigations.”

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Atomic Layer Processing Coating Techniques Enable Missions to See Further into the Ultraviolet

Astrophysics observations at ultraviolet (UV) wavelengths often probe the most dynamic aspects of the universe. However, the high energy of ultraviolet photons means that their interaction with the materials that make up an observing instrument are less efficient, resulting in low overall throughput. New approaches in the development of thin film coatings are addressing this shortcoming by engineering the coatings of instrument structures at the atomic scale.

Researchers at the NASA Jet Propulsion Laboratory (JPL) are employing atomic layer deposition (ALD) and atomic layer etching (ALE) to enable new coating technologies for instruments measuring ultraviolet light. Conventional optical coatings largely rely on physical vapor deposition (PVD) methods like evaporation, where the coating layer is formed by vaporizing the source material and then condensing it onto the intended substrate. In contrast, ALD and ALE rely on a cyclic series of self-limiting chemical reactions that result in the deposition (or removal) of material one atomic layer at a time. This self-limiting characteristic results in a coating or etchings that are conformal over arbitrary shapes with precisely controlled layer thickness determined by the number of ALD or ALE cycles performed.

The ALD and ALE techniques are common in the semiconductor industry where they are used to fabricate high-performance transistors. Their use as an optical coating method is less common, particularly at ultraviolet wavelengths where the choice of optical coating material is largely restricted to metal fluorides instead of more common metal oxides, due to the larger optical band energy of fluoride materials, which minimizes absorption losses in the coatings. Using an approach based on co-reaction with hydrogen fluoride, the team at JPL has developed a variety of fluoride-based ALD and ALE processes.

In addition to these metal-fluoride materials, layers of aluminum are often used to construct structures like reflective mirrors and bandpass filters for instruments operating in the UV.  Although aluminum has high intrinsic UV reflectance, it also readily forms a surface oxide that strongly absorbs UV light. The role of the metal fluoride coating is then to protect the aluminum surface from oxidation while maintaining enough transparency to create a mirror with high reflectance.

The use of ALD in this context has initially been pursued in the development of telescope optics for two SmallSat astrophysics missions that will operate in the UV: the Supernova remnants and Proxies for ReIonization Testbed Experiment (SPRITE) CubeSat mission led by Brian Fleming at the University of Colorado Boulder, and the Aspera mission led by Carlos Vargas at the University of Arizona. The mirrors for SPRITE and Aspera have reflective coatings that utilize aluminum protected by lithium fluoride using a novel PVD processes developed at NASA Goddard Space Flight Center, and an additional very thin top coating of magnesium fluoride deposited via ALD.

The use of lithium fluoride enables SPRITE and Aspera to “see” further into the UV than other missions like NASA’s Hubble Space Telescope, which uses only magnesium fluoride to protect its aluminum mirror surfaces. However, a drawback of lithium fluoride is its sensitivity to moisture, which in some cases can cause the performance of these mirror coatings to degrade on the ground prior to launch. To circumvent this issue, very thin layers (~1.5 nanometers) of magnesium fluoride were deposited by ALD on top of the lithium fluoride on the SPRITE and Aspera mirrors. The magnesium fluoride layers are thin enough to not strongly impact the performance of the mirror at the shortest wavelengths, but thick enough to enhance the stability against humidity during ground phases of the missions. Similar approaches are being considered for the mirror coatings of the future NASA flagship Habitable Worlds Observatory (HWO).

Multilayer structures of aluminum and metal fluorides can also function as bandpass filters (filters that allow only signals within a selected range of wavelengths to pass through to be recorded) in the UV. Here, ALD is an attractive option due to the inherent repeatability and precise thickness control of the process. There is currently no suitable ALD process to deposit aluminum, and so additional work by the JPL team has explored the development of a custom vacuum coating chamber that combines the PVD aluminum and ALD fluoride processes described above. This system has been used to develop UV bandpass filters that can be deposited directly onto imaging sensors like silicon (Si) CCDs. These coatings can enable such sensors to operate with high UV efficiency, but low sensitivity to longer wavelength visible photons that would otherwise add background noise to the UV observations.

Structures composed of multilayer aluminum and metal fluoride coatings have recently been delivered as part of a UV camera to the Star-Planet Activity Research CubeSat (SPARCS) mission led by Evgenya Shkolnik at Arizona State University. The JPL-developed camera incorporates a delta-doped Si CCD with the ALD/PVD filter coating on the far ultraviolet channel, yielding a sensor with high efficiency in a band centered near 160 nm with low response to out-of-band light.

Next, the JPL team that developed these coating processes plans to focus on implementing a similar bandpass filter on an array of larger-format Si Complementary Metal-Oxide-Semiconductor (CMOS) sensors for the recently selected NASA Medium-Class Explorer (MIDEX) UltraViolet EXplorer (UVEX) mission led by Fiona Harrison at the California Institute of Technology, which is targeted to launch in the early 2030s. 

For additional details, see the entry for this project on NASA TechPort

Project Lead: Dr. John Hennessy, Jet Propulsion Laboratory (JPL)

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