Astronauts’ Perspectives on NESC Contributions to Mission Safety and Success 

Astronauts’ Perspectives on NESC Contributions to Mission Safety and Success 

Mark Vande Hei outside of ISS (October 10, 2017). 
Mark Vande Hei outside of ISS (October 10, 2017). 

This article is from the 2025 Technical Update.

The exact date when the crew of Space Shuttle Columbia was lost is readily recalled by Patrick Forrester, as it likely would be for any NASA employee in service that Saturday morning when the Shuttle broke up during reentry. Forrester had flown to ISS for the first time in 2001 aboard Discovery in support of the STS-105 mission. He was scheduled to fly again shortly after Columbia’s February 1, 2003 return. That date is now a somber anniversary etched in his memory.  

“I had three classmates on Columbia,” Forrester said. “As an astronaut class, you are even closer because you are selected together and go through that initial training together.” That was the reason he said yes when asked to join the NESC in 2009 as the NESC Chief Astronaut—the liaison between the NESC and the Astronaut Office. “The NESC was started after the Columbia accident, and it was really just an honor to be part of that organization where the focus was to make sure that didn’t happen again.” 

The NESC has had an astronaut liaison for most of its 22-year history. “It stands to reason that the individuals the NESC works so hard to protect should have a seat at the table,” said NESC Director Tim Wilson.

“The Chief Astronaut gives them direct access to the NESC for insight into technical activities that might affect them and a forum for voicing concerns that otherwise might not have surfaced. The interface gives us access to them as well; astronauts have lent their expertise and unique perspectives to many NESC assessments over the years. As the agency’s front-line risk takers, they are by definition our primary stakeholders, and much of what we do revolves around ensuring the risks they take are well-understood and mitigated.”  The current and some of the former Chief Astronauts shared their perspectives on how they feel about the NESC and whether this organization—designed to increase the overall safety of their jobs—was  accomplishing that mission.    

Patrick Forrester 
NESC Chief Astronaut 2009-2016 

It would be four years after Columbia that Forrester would fly again. That was June 2007 aboard Space Shuttle Atlantis as part of STS-117, where he helped deliver the second starboard truss and third set of solar arrays to ISS.  During his years with the NESC, Forrester assisted in NESC assessments or arranged for others from the Astronaut Office to participate. He recalled being a part of an NESC review of the astronaut pre-breathe protocol used before extravehicular activities, and he also worked with fellow astronaut Dr. Nancy Currie, who at that time was a principal engineer for the NESC, to assess the procedures and plans to ensure alternative means of return for STS-135 in the event Atlantis could not provide it. Since the other Space Shuttle orbiters had retired, rescue capability via Space Shuttle was not an option for this mission, he said. “We came up with the plan of how they could stay on the space station and use a Russian Soyuz to get them back.” 

Patrick Forrester, STS-128 mission specialist, watches his spacewalking crewmates through an overhead window on the aft flight deck of Space Shuttle Discovery while docked with the ISS (September 3, 2009)
Patrick Forrester, STS-128 mission specialist, watches his spacewalking crewmates through an overhead window on the aft flight deck of Space Shuttle Discovery while docked with the ISS (September 3, 2009)

Forrester always felt, however, that his primary mission was to educate others about the NESC, which was a relatively new organization at that time. “I tried to help them understand that the NESC was engineering. This is what we do. This is what we need. It was one of my goals when I served: to help people understand what the NESC did.”  

After leaving his NESC post to become chief of the Astronaut Office, he continued to call on the NESC during the lead-up to the launch of SpaceX Crew Dragon Demonstration Mission-2, the first SpaceX flight with crew aboard. “I was feeling the weight and the responsibility as the chief of putting Bob Behnken and Doug Hurley on that rocket for the first time. I took a lot of comfort in knowing how involved the NESC was in those decisions.” 

Barry “Butch” Wilmore 
NESC Chief Astronaut 2018-2020 

Following Forrester’s tenure, Butch Wilmore served as the NESC Chief Astronaut for two years.  A former Navy test pilot, Wilmore joined NASA in 2000, flying three missions to the ISS, including his most recent as commander of the Boeing Starliner’s first crewed flight. He took on the NESC liaison role already well acquainted with the NESC’s mission.  

Boeing Crew Flight Test Commander Butch Wilmore performs spacesuit maintenance inside ISS's Quest airlock (July 11, 2024).
Boeing Crew Flight Test Commander Butch Wilmore performs spacesuit maintenance inside ISS’s Quest airlock (July 11, 2024).

“I’m very familiar with the certification, flight readiness, the flight readiness reviews, and how the NESC is used to validate some of the assumptions and the engineering that takes place. And I wasn’t just aware of the organization, but knew exactly what it did and what benefit it was,” Wilmore said.  “When I worked with the NESC, it gave me knowledge to understand more of what and how they went about doing things—that deep engineering analysis. And as an operator, I don’t dig into the engineering analysis. I just see big picture. So, when I would see something that wasn’t right, I knew the NESC could work on it and figure out why it didn’t look right to me.” 

Wilmore ended his NESC tenure when he was chosen as the Starliner commander, but continued to reach back whenever he needed answers to the multitude of questions that arise in flying a spacecraft for the first time. “Certainly when I became the commander of Starliner, there were things that I knew I wanted the NESC to have purview over.” In its support of the Commercial Crew Program, the NESC not only assisted in the lead-up to the flight, but helped troubleshoot propulsion issues it experienced on its way to ISS and with the plans to bring the crew home. “The NESC obviously has been a big help in all organizations,” Wilmore added. “I think that the role it plays is vital, and I wish it was larger.” 

Scott Tingle 
NESC Chief Astronaut 2020-2022 

Scott Tingle was selected in June 2009 to the astronaut corps, serving as a flight engineer and U.S. Operational Segment Lead for Expedition 54/55, where he spent 168 days aboard the ISS. His training for spaceflight involved many discussions about the Columbia accident.  “We debriefed it 100 times,” he said. “When we’re talking safety issues—Apollo, Challenger, Columbia—they always come up, and there are always really good lessons learned.” 

With his naval aviation and engineering background, Tingle said it didn’t take him long to get a feel for how the NESC worked. “They really get their fingers on the pulse of operations, which is what I think is one of the high value things they do.” When it came to filling in engineering gaps, Tingle liked having the NESC to lean on, “not only because of their engineering perspective, but because it’s independent. They’re not involved in the politics and everything that goes with it. And they have the end user and the operators in their heart and soul,” said Tingle. “This is the product that you get out of the NESC. It’s just a huge value because of that.”  

“Having folks able to dive into the technicals, it really helps us. And it doesn’t just help us, it helps the crew, it helps the program, it helps the contractors, it helps our technical authorities. It helps everybody just to have people with that capability.” 

Scott Tingle wears a U.S. spacesuit inside the Quest Airlock preparing for his first spacewalk (January 18, 2018).
Scott Tingle wears a U.S. spacesuit inside the Quest Airlock preparing for his first spacewalk (January 18, 2018).  

He remembers when the NESC ramped up material testing to address an issue the astronaut corps was working. “They were able to get results very quickly. They really do fill the gap when it needs to be filled. They help us catch the things that we can’t catch.” 

Being an astronaut was always on Tingle’s career agenda, and that obsession was deeply rooted at an early age. “I remember watching on TV Neil Armstrong stepping out onto the moon. I was four years old at the time, and me and my mom were watching in our living room.”  

In a way, that is part of what he thinks makes the NESC so valuable. “They have not forgotten their roots. They haven’t forgotten the users who actually use this equipment and the value of the overall human spaceflight community.” 

Sometimes that value is only seen in hindsight. “When we finally get up and running with all of these vehicles, I think you’re going to be able to go back and list all of these actions the NESC supported and how they helped provide critical information. You’re going to end up seeing that, ‘Wow, this was really transformational. This really helped us with our overall direction. It helped us be successful,’ ” Tingle said. “I’m honored to have been a part of it.” 

Mark Vande Hei 
NESC Chief Astronaut 2023-present 

“I think the fact that NASA’s been willing to invest the talent and the resources to have an organization that can do a really deep dive with a second, third, fifth set of eyes, with the best technical experts and the perspective of knowing what’s going on across NASA, is a hugely beneficial thing,” said Mark Vande Hei, the current NESC Chief Astronaut.  

Expedition 65 Flight Engineer Mark Vande Hei works inside the U.S. Destiny laboratory module's Microgravity Science Glovebox for the Ring Sheared Drop fluid physics study (August 16, 2021)
Expedition 65 Flight Engineer Mark Vande Hei works inside the U.S. Destiny laboratory module’s Microgravity Science Glovebox for the Ring Sheared Drop fluid physics study (August 16, 2021)

Relatively new to the organization, he’s been getting up to speed. “I’ve already seen programs like the ISS repeatedly pull in NESC expertise to help out.” In his own experience, he sought NESC advice to help understand the risk posture associated with batteries. “I knew it was something we could fix, but it was going to cost money. And so the emphasis was on ‘how risky is this? Can we accept this risk?’ ” Help from the NASA Technical Fellow for Electrical Power helped him make decisions on what avenues to pursue.  

He also asked the NESC to convey the risks associated with leaks in the Russian PrK module. “I wanted to have both sides hear directly what the other’s perspective was. I was  impressed with the NESC’s professionalism,” said Vande Hei, in discussing a topic that has been controversial at times. “In addition to their technical skills, there’s an impressive interpersonal skill set that comes along with the folks on the NESC, too.” 

Having already spent more than 500 days in space, Vande Hei is focused on the next generation. “There are a lot of other people who haven’t flown yet, and we need to get them to space because they’ll still be around when we’re doing much more challenging missions to the Moon and Mars. And they need to get the experience to be ready for those things much more than I do.” Even today, Vande Hei said the emotions he goes through when he watches astronauts launch, “I’m a mess. It’s rough, but it’s great. I call it ‘horribly amazing.’” 

____________________ 

Today, 22 years in and with nearly 1,400 assessments behind it, the NESC has won the respect of the programs and projects it supports, and some of it was earned with the help of its astronaut liaisons. “They helped us prove we could add value to NASA missions and bring new perspectives to their technical problems,” said Wilson. “We keep a photograph of the Columbia crew in the NESC office, but our astronaut liaisons are living, breathing reminders of why we do this work.”      

Pat Forrester, now retired from NASA, considers his time with the NESC well spent. “You always want to be able, if there is an accident, to look at the remaining family and let them know you did everything that could be done. The amount of involvement the NESC has is limited only by funds and people, so I know how hard everyone works on those assessments,” he said. “I appreciated it so much when I was in that role where I felt like I was carrying a lot of the burden.”  

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Meagan Chappell

Eruption at Mayon

Eruption at Mayon

The upper slopes of Mayon volcano appear brown, with several narrow channels radiating from the crater. A red infrared heat signature appears near the summit, with red streaks extending east and southeast. The lower slopes are green and forested. Farmland and towns are visible in the lower part of the image.
February 26, 2026

At any given moment, about 20 volcanoes on Earth are actively erupting. Often among them is Mayon—the most active volcano in the Philippines. The nearly symmetrical stratovolcano, on Luzon Island near the Albay and Lagonoy gulfs, rises more than 2,400 meters (8,000 feet) above sea level.

Historical records indicate Mayon has erupted 65 times in the past 5,000 years, with the latest episode beginning in January 2026. The Philippine Institute of Volcanology and Seismology (PHIVOLCS) first reported increased rockfalls near the volcano’s summit and inflation of the mountain’s upper slopes. On January 6, the alert level was increased to three on a five-level scale after lava began flowing from the crater and hot clouds of ash and debris called pyroclastic flows (also called pyroclastic density currents) moved down one side of the mountain.

The volcano was still puffing and lava flowing on February 26, when the OLI (Operational Land Imager) on Landsat 8 acquired this rare, relatively clear image. The natural-color scene is overlaid with infrared observations to highlight the lava’s heat signature. On that day, PHIVOLCS reported volcanic earthquakes, rockfalls, and pyroclastic flows. The longest pyroclastic flow had traveled about 4 kilometers (3 miles) through the Mi-isi Gully on the southeast flank. 

The level-three alert, which remained in place in March, prompted evacuations within a 6-kilometer (4-mile) radius of the crater, displacing hundreds of families from communities including Tabaco City, Malilpot, and Camalig. Past pyroclastic flows have proven extremely destructive, leading to more than 1,000 deaths in 1814, at least 400 deaths in 1897, and 77 deaths in 1993. More than 73,000 people were evacuated during an eruption in 1984.

Sulfur dioxide (SO2) emissions during the current eruption have averaged 2,466 tons per day, with a peak of 6,569 metric tons measured on February 4, 2026. That is the highest SO2 emission level for one day in 15 years, the PHIVOLCS announced in early February. That was later exceeded on March 6, when SO2 emissions reached as high as 7,633 metric tons

Multiple NASA satellites have also monitored the volcano’s sulfur dioxide emissions, showing sizable plumes of the gas drifting southwest on February 4 and March 6. The Philippine volcanology institute reported a peak in other activity on February 8 and 9, with 469 rockfalls, 12 major pyroclastic flows, and ashfall in the municipalities of Camalig and Guinobatan.

NASA Earth Observatory image by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Adam Voiland.

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About Low Boom Flight Demonstrator (LBFD) Project

About Low Boom Flight Demonstrator (LBFD) Project

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

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NASA’s X-59 quiet supersonic research aircraft cruises above Palmdale and Edwards, California, during its first flight, Tuesday, Oct. 28, 2025. The aircraft traveled to NASA’s Armstrong Flight Research Center in Edwards, California.
NASA/Lori Losey

The Low Boom Flight Demonstrator project (LBFD) is part of NASA’s effort to help enable new aircraft noise standards that are required to open the market to commercial supersonic flight over land.

The federal government banned all civilian supersonic flights over land more than fifty years ago due to sonic boom noise. If new standards are established, the U.S. aviation industry can position itself to lead the commercial supersonic market, and passengers will benefit from significantly shorter travel times.

Over the past decade, fundamental research and experimentation have demonstrated the possibility of supersonic flight with greatly reduced sonic boom noise – one of several key areas needed to transform commercial supersonic flight.  

NASA’s X-59, part of the LBFD project, sits on the ramp of Lockheed Martin’s Skunk Works facility, facing toward the site’s main hangar during sunset.
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The LBFD project will demonstrate a reduced sonic boom by utilizing a purpose-built experimental aircraft designated the X-59.

The LBFD project supports a multi-phase effort aimed at demonstrating the X-59’s ability to fly supersonic without generating loud sonic booms. The LBFD project leads Phase 1 of the Quesst mission, involving the design, fabrication, ground tests, and checkout flights of the X-59.

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Mar 12, 2026

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Jim Banke
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Lillian Gipson

NASA to Cover Upcoming US Spacewalks 94, 95 Outside Space Station

NASA to Cover Upcoming US Spacewalks 94, 95 Outside Space Station

NASA astronaut and Expedition 72 Flight Engineer Anne McClain is pictured near one of the International Space Station's main solar arrays during a spacewalk to upgrade the orbital outpost's power generation system and relocate a communications antenna.
NASA astronaut Anne McClain works near one of the International Space Station’s main solar arrays during a May 1, 2025, spacewalk to upgrade the station’s power system and relocate a communications antenna.
Credit: NASA

NASA astronauts will conduct a pair of spacewalks beginning Wednesday, March 18, outside of the International Space Station to prepare for the installation of two roll-out solar arrays. Experts from NASA will preview the spacewalks during a news conference at 2 p.m. EDT, Monday, March 16, at the agency’s Johnson Space Center in Houston.

Watch NASA’s live coverage of the news conference on the agency’s YouTube channel. Learn how to stream NASA content through a variety of online platforms, including social media.

NASA participants include:

  • Bill Spetch, operations integration manager, International Space Station Program
  • Diana Trujillo, spacewalk flight director, Flight Operations Directorate
  • Ronak Dave, spacewalk flight director, Flight Operations Directorate

Media interested in participating in person or by phone must contact the NASA Johnson newsroom no later than 10 a.m. on March 16 by calling 281-483-5111 or emailing jsccommu@mail.nasa.gov. To ask questions by phone, reporters must dial into the news conference no later than 15 minutes prior to the start of the call. Questions also may be submitted on social media using #AskNASA. NASA’s media accreditation policy is available online.

On March 18, NASA astronauts Jessica Meir and Chris Williams will conduct U.S. spacewalk 94, exiting the orbiting laboratory’s Quest airlock to prepare the 2A power channel for the future International Space Station Roll-Out Solar Arrays (IROSA) installation. It will be Meir’s fourth spacewalk and Williams’ first.

Watch NASA’s live coverage beginning at 6:30 a.m. on NASA+, Amazon Prime, and the agency’s YouTube channel. U.S. spacewalk 94 will begin at approximately 8 a.m. and is expected to last about six and a half hours.

For U.S. spacewalk 95, two NASA astronauts will prepare the station’s 3B power channel for a future IROSA installation. NASA will provide more information on the date and time of the spacewalk, the crew members assigned to the activity, and coverage details closer to the operation.

The spacewalks will be the 278th and 279th supporting space station assembly, maintenance and upgrades. They also are the first two station spacewalks of 2026 and the first for Expedition 74. Spacewalks 94 and 95 originally were scheduled for January, but the target dates were adjusted after the early departure of NASA’s SpaceX Crew‑11 mission.

Learn more about International Space Station research and operations at:

https://www.nasa.gov/station

-end-

Josh Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov

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

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Jessica Taveau

Tiny NASA Spacecraft Delivers Exoplanet Mission’s First Images

Tiny NASA Spacecraft Delivers Exoplanet Mission’s First Images

This pair of images shows stars observed Feb. 6, 2026, by the SPARCS space telescope simultaneously in the near-ultraviolet, left, and far-ultraviolet, right. The fact that one star is seen in the far-UV while multiple are seen in near-UV offers insights into the temperatures of these stars, with the one visible in both colors being the hottest.
NASA/JPL-Caltech/ASU

With the first images from the spacecraft now in hand, the team behind NASA’s Star-Planet Activity Research CubeSat, or SPARCS, is ready to begin charting the energetic lives of the galaxy’s most common stars to help answer one of humanity’s most profound questions: Which distant worlds beyond our solar system might be habitable? 

Initial, or “first light,” images mark the moment a mission proves its instruments are functioning in space and ready to transition to full science operations. This milestone is especially important for SPARCS, whose observations depend on highly precise ultraviolet (UV) measurements, making the demonstration of the camera’s performance critical to achieving its science goals. The spacecraft launched Jan. 11; the images came down Feb. 6 and were subsequently processed. 

Roughly the size of a large cereal box, SPARCS will monitor flares and sunspot activity on low-mass stars — objects only 30% to 70% the mass of the Sun. These stars are among the most common in the Milky Way and host the majority of the galaxy’s roughly 50 billion habitable-zone terrestrial planets, which are rocky worlds close enough to their stars for temperatures that could allow liquid water and potentially support life. 

“Seeing SPARCS’ first ultraviolet images from orbit is incredibly exciting. They tell us the spacecraft, the telescope, and the detectors are performing as tested on the ground and we are ready to begin the science we built this mission to do,” says SPARCS Principal Investigator Evgenya Shkolnik, professor of Astrophysics at the School of Earth and Space Exploration at Arizona State University, which leads the mission. 

The SPARCS spacecraft is the first dedicated to continuously and simultaneously monitoring the far-ultraviolet and near-ultraviolet radiation from low-mass stars for extended periods. Over its one-year mission, SPARCS will target approximately 20 low-mass stars and observe them over durations of five to 45 days.  

Although such stars are small, dim, and cool compared to the Sun, they are also known to flare far more frequently than our solar system’s star. The flares can dramatically affect the atmospheres of the planets they host. Understanding the host star is key to understanding a planet’s habitability.

Future focused  

“I am so excited that we are on the brink of learning about exoplanets’ host stars and the effect of their activities on the planets’ potential habitability,” said Shouleh Nikzad, the lead developer of the SPARCS camera (dubbed SPARCam) and the chief technologist at NASA’s Jet Propulsion Laboratory in Southern California. “I’m doubly excited that we are contributing to this mission with detector and filter technologies we developed at JPL’s Microdevices Laboratory.” Created in 1989, the facility is where inventors harness physics, chemistry, and material science, including quantum, to deliver first-of-their-kind devices and capabilities for the nation. 

The filters were made using a technique that improves sensitivity and performance by enabling them to be directly deposited onto the specially developed UV-sensitive “delta-doped” detectors. The approach of detector-integrated filters eliminated the need for a separate filter element, resulting in a system that is among the most sensitive of its kind ever flown in space.  

“We took silicon-based detectors — the same technology as in your smartphone camera — and we created a high-sensitivity UV imager. Then we integrated filters into the detector to reject the unwanted light. That is a huge leap forward to doing big science in small packages,” Nikzad said, “and SPARCS serves to demonstrate their long-term performance in space.” 

This technology paves the way for future missions like NASA’s next potential UV-capable flagship mission, the Habitable Worlds Observatory mission concept, as well as smaller interim missions, such as the agency’s forthcoming UVEX (UltraViolet EXplorer), which is led by Caltech in Pasadena.  

The mission takes advantage of advances in computational processing as well, with an onboard computer that can perform data processing and intelligently adjust the observation parameters to better sample the development of flares as they happen.  

“The SPARCS mission brings all of these pieces together — focused science, cutting-edge detectors, and intelligent onboard processing — to deepen our understanding of the stars that most planets in the galaxy call home,” said David Ardila, SPARCS instrument scientist at JPL. “By watching these stars in ultraviolet light in a way we’ve never done before, we’re not just studying flares. These observations will sharpen our picture of stellar environments and help future missions interpret the habitability of distant worlds.”

More about SPARCS 

Funded by NASA and led by Arizona State University, SPARCS is managed under the agency’s Astrophysics Research and Analysis program. The agency’s CubeSat Launch Initiative (CSLI) selected SPARCS in 2022 for a ride to orbit. The initiative is a low-cost pathway for conducting scientific investigations and technology demonstrations in space, enabling students and faculty to gain hands-on experience with flight hardware design, development, and building.  

Blue Canyon Technologies fabricated the spacecraft bus.

News Media Contact

Matthew Segal
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-8307
matthew.j.segal@jpl.nasa.gov

Alise Fisher / Karen Fox
NASA Headquarters, Washington
202-358-2546 / 202-385-1287
alise.m.fisher@nasa.gov / karen.c.fox@nasa.gov

Kim Baptista  
Arizona State University, School of Earth and Space Exploration  
480-727-4662
Kim.Baptista@asu.edu 

2026-016

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Naomi Hartono