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Hera takes flight: Didymos, here we come
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By NASA
Dr. Natasha Schatzman Receives Vertical Flight Society (VFS) Award
The Forum 81 award was presented to Natasha Schatzman (center), with the award given by the parents of Alex Stoll, Mark and Lyn Stoll, and flanked by VFS Chair of the Board Harry Nahatis (left) and VFS Executive Director Angelo Collins (right). Source: https://gallery.vtol.org/image/AloOB. Photo Credit: Warren Liebmann In May 2025, Dr. Natasha Schatzman, aerospace engineer in the Aeromechanics Office at NASA Ames Research Center, received the inaugural Alex M. Stoll Award from the Vertical Flight Society (VFS). This award honors a professional in the field of vertical flight who “demonstrates an exceptional commitment to advancing not only the mission of their organization but makes extraordinary contributions to enhancing the well-being and happiness of their colleagues.” Dr. Schatzman began her career at Ames in 2008 as a student intern while simultaneously completing her undergraduate studies at the Georgia Institute of Technology (Georgia Tech). She stayed at Georgia Tech through graduate school and finished her Ph.D. dissertation in 2018 in the Aeronautical and Astronautical Engineering Department. Currently, Dr. Schatzman is focusing on assessments of rotorcraft performance and aeroacoustics through experimentation and modeling at Ames Research Center. The Alex M. Stoll Award is the second time she has been honored by the VFS. In 2023, Dr. Schatzman received the François-Xavier Bagnoud Vertical Flight Award which is given to a member “who is 35 years old or younger for their career-to-date outstanding contributions to vertical flight technology.” More information on Dr. Schatzman’s 2025 award is at: https://vtol.org/awards-and-contests/vertical-flight-society-award-winners?awardID=28
About the Author
Osvaldo R. Sosa Valle
Osvaldo Sosa is a dedicated and detail-oriented project coordinator at NASA Ames Research Center, where he supports operations for the Aeronautics Directorate. He is part of the Strategic Communications Team and serves as managing editor for the Aeronautics topic on the NASA website. With experience in event coordination, logistics, and stakeholder engagement, Osvaldo brings strong organizational and communication skills to every project. He is passionate about driving innovation, fostering strong leadership, and streamlining operations to enhance team collaboration and organizational impact.
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Last Updated Jun 06, 2025 Related Terms
Ames Research Center View the full article
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By NASA
Megan Harvey is a utilization flight lead and capsule communicator, or capcom, in the Research Integration Office at NASA’s Johnson Space Center in Houston. She integrates science payload constraints related to vehicles’ launch and landing schedules. She is also working to coordinate logistics for the return of SpaceX vehicles to West Coast landing sites.
Read on to learn about Harvey’s career with NASA and more!
Megan Harvey talking to a flight director from the Remote Interface Officer console in the Mission Control Center at NASA’s Johnson Space Center in Houston. NASA/Mark Sowa Johnson Space Center is home to the best teams, both on and off the planet!
Megan Harvey
Utilization Flight Lead and Capsule Communicator
Where are you from?
I am from Long Valley, New Jersey.
How would you describe your job to family or friends who may not be familiar with NASA?
Many biological experiments conducted on the space station have specific time constraints, including preparation on the ground and when crew interacts with them on orbit. I help coordinate and communicate those kinds of constraints within the International Space Station Program and with the scientific community. This is especially important because launch dates seldom stay where they are originally planned! I am also currently working in a cross-program team coordinating the logistics for the return to West Coast landings of SpaceX vehicles.
As a capcom, I’m the position in the Mission Control Center in Houston that talks to the crew. That would be me responding to someone saying, “Houston, we have a problem!”
I’ve worked in the Research Integration Office since the beginning of 2024 and have really enjoyed the change of pace after 11 years in the Flight Operations Directorate, where I supported several different consoles for the International Space Station. I’ve kept my capcom certification since 2021, and it is an absolute dream come true every time I get to sit in the International Space Station Flight Control Room. Johnson Space Center is home to the best teams, both on and off the planet!
How long have you been working for NASA?
I have been working for the agency for 13 years.
What advice would you give to young individuals aspiring to work in the space industry or at NASA?
Some things that I have found that helped me excel are:
1. Practice: I am surprised over and over again how simply practicing things makes you better at them, but it works!
2. Preparation: Don’t wing things!
3. Curiosity: Keep questioning!
4. Enthusiasm!
Megan Harvey and friends after biking 25 miles to work. What was your path to NASA?
I had a very circuitous path to NASA. Since going to Space Camp in Huntsville, Alabama, when I was 10 years old, I wanted to be a capcom and work for NASA. I also traveled to Russia in high school and loved it. I thought working on coordination between the Russian and U.S. space programs would be awesome. In pursuit of those dreams, I earned a bachelor’s degree in physics with a minor in Russian language from Kenyon College in Gambier, Ohio, but I had so much fun also participating in music extracurriculars that my grades were not quite up to the standards of working at NASA. After graduation, I worked at a technology camp for a summer and then received a research assistant position in a neuroscience lab at Princeton University in New Jersey.
After a year or so, I realized that independent research was not for me. I then worked in retail for a year before moving to California to be an instructor at Astrocamp, a year-round outdoor education camp. I taught a number of science classes, including astronomy, and had the opportunity to see the Perseverance Mars rover being put together at NASA’s Jet Propulsion Laboratory in Southern California. It dawned on me that I should start looking into aerospace-related graduate programs. After three years at Embry-Riddle in Daytona Beach, Florida, I received a master’s degree in engineering physics and a job offer for a flight control position, initially working for a subcontractor of United Space Alliance. I started in mission control as an attitude determination and control officer in 2012 and kept that certification until the end of 2023. Along the way, I was a Motion Control Group instructor; a Russian systems specialist and operations lead for the Houston Support Group working regularly in Moscow; a Remote Interface Officer (RIO); and supported capcom and the Vehicle Integrator team in a multipurpose support room for integration and systems engineers. I have to pinch myself when I think about how I somehow made my childhood dreams come true.
Is there someone in the space, aerospace, or science industry that has motivated or inspired you to work for the space program? Or someone you discovered while working for NASA who inspires you?
After I switched offices to Houston Support Group/RIO, most of my training was led by Sergey Sverdlin. He was a real character. Despite his gruffness, he and I got along really well. We were very different people, but we truly respected each other. I was always impressed with him and sought out his approval.
Megan Harvey in Red Square in Moscow, Russia. What is your favorite NASA memory?
The most impactful experience I’ve had at NASA was working together with the Increment 68 leads during the days and months following the Soyuz coolant leak. I was increment lead RIO and just happened to be in the Increment Management Center the day of a planned Russian spacewalk. The increment lead RIO is not typically based in the Increment Management Center, but that day, things were not going well. All of our Russian colleagues had lost access to a critical network, and I was troubleshooting with the Increment Manager and the International Space Station Mission Management Team chair.
I was explaining to International Space Station Deputy Program Manager Dina Contella the plan for getting our colleagues access before their off-hours spacewalk when we saw a snowstorm of flakes coming out of the Soyuz on the downlink video on her office’s wall. Those flakes were the coolant. It was incredible watching Dina switch from winding down for the day to making phone call after phone call saying, “I am calling you in.” The Increment Management Center filled up and I didn’t leave until close to midnight that day. The rest of December was a flurry (no pun intended) of intense and meaningful work with the sharpest and most caring people I know.
What do you love sharing about station? What’s important to get across to general audiences to help them understand the benefits to life on Earth?
There is so much to talk about! I love giving insight into the complexities of not only the space station systems themselves, but also the international collaboration of all the teams working to keep the systems and the science running.
If you could have dinner with any astronaut, past or present, who would it be?
I would have dinner with Mae Jemison or Sally Ride. It’s too hard to pick!
Do you have a favorite space-related memory or moment that stands out to you?
I was selected by my management a few years ago to visit a Navy aircraft carrier with the SpaceX Crew-1 crew and some of the Crew-1 team leads. We did a trap landing on the deck and were launched off to go home, both via a C-2 Greyhound aircraft. It was mind blowing! I am also very lucky that I saw the last space shuttle launch from Florida when I was in graduate school.
Megan Harvey and NASA colleagues on the Nimitz aircraft carrier. What are some of the key projects you’ve worked on during your time at NASA? What have been your favorite?
My first increment lead role was RIO for Increment 59 and there was a major effort to update all our products in case of needing to decrew the space station. It was eye-opening to work with the entire increment team in this effort. I really enjoyed all the work and learning and getting to know my fellow increment leads better, including Flight Director Royce Renfrew.
Also, in 2021 I was assigned as the Integration Systems Engineer (ISE) lead for the Nanorack Airlock. I had never worked on a project with so many stakeholders before. I worked close to 100 revisions of the initial activation and checkout flowchart, coordinating with the entire flight control team. It was very cool to see the airlock extracted from NASA’s SpaceX Dragon trunk and installed, but it paled in comparison to the shift when we did the first airlock trash deploy. I supported as lead ISE, lead RIO, and capcom all from the capcom console, sitting next to the lead Flight Director TJ Creamer. I gave a countdown to the robotics operations systems officer commanding the deploy on the S/G loop so that the crew and flight control team could hear, “3, 2, 1, Engage!”
I’ll never forget the satisfaction of working through all the complications with that stellar team and getting to a successful result while also having so much fun.
Megan Harvey at a bouldering gym. What are your hobbies/things you enjoy outside of work?
I love biking, rock climbing, cooking, board games, and singing.
Day launch or night launch?
Night launch!
Favorite space movie?
Space Camp. It’s so silly. And it was the first DVD I ever bought!
NASA “worm” or “meatball” logo?
Worm
Every day, we’re conducting exciting research aboard our orbiting laboratory that will help us explore further into space and bring benefits back to people on Earth. You can keep up with the latest news, videos, and pictures about space station science on the Station Research & Technology news page. It’s a curated hub of space station research digital media from Johnson and other centers and space agencies.
Sign up for our weekly email newsletter to get the updates delivered directly to you.
Follow updates on social media at @ISS_Research on Twitter, and on the space station accounts on Facebook and Instagram.
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By NASA
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s X-59 quiet supersonic research aircraft is seen during its “aluminum bird” systems testing at Lockheed Martin’s Skunk Works facility in Palmdale, California. The test verified how the aircraft’s hardware and software work together, responding to pilot inputs and handling injected system failures. Lockheed Martin / Garry Tice NASA’s X-59 quiet supersonic research aircraft successfully completed a critical series of tests in which the airplane was put through its paces for cruising high above the California desert – all without ever leaving the ground.
“The idea behind these tests is to command the airplane’s subsystems and flight computer to function as if it is flying,” said Yohan Lin, the X-59’s lead avionics engineer at NASA’s Armstrong Flight Research Center in Edwards, California.
The goal of ground-based simulation testing was to make sure the hardware and software that will allow the X-59 to fly safely are properly working together and able to handle any unexpected problems.
Any new aircraft is a combination of systems, and identifying the little adjustments required to optimize performance is an important step in a disciplined approach toward flight.
“We thought we might find a few things during the tests that would prompt us to go back and tweak them to work better, especially with some of the software, and that’s what we wound up experiencing. So, these tests were very helpful,” Lin said.
Completing the tests marks another milestone off the checklist of things to do before the X-59 makes its first flight this year, continuing NASA’s Quesst mission to help enable commercial supersonic air travel over land.
Simulating the Sky
During the testing, engineers from NASA and contractor Lockheed Martin turned on most of the X-59’s systems, leaving the engine off. For example, if the pilot moved the control stick a certain way, the flight computer moved the aircraft’s rudder or other control surfaces, just as it would in flight.
At the same time, the airplane was electronically connected to a ground computer that sends simulated signals – which the X-59 interpreted as real – such as changes in altitude, speed, temperature, or the health of various systems.
Sitting in the cockpit, the pilot “flew” the aircraft to see how the airplane would respond.
“These were simple maneuvers, nothing too crazy,” Lin said. “We would then inject failures into the airplane to see how it would respond. Would the system compensate for the failure? Was the pilot able to recover?”
Unlike in typical astronaut training simulations, where flight crews do not know what scenarios they might encounter, the X-59 pilots mostly knew what the aircraft would experience during every test and even helped plan them to better focus on the aircraft systems’ response.
NASA test pilot James Less sits in the cockpit of the X-59 quiet supersonic research aircraft as he participates in a series of “aluminum bird” systems tests at Lockheed Martin’s Skunk Works facility in Palmdale, California.Lockheed Martin / Garry Tice Aluminum vs. Iron
In aircraft development, this work is known as “iron bird” testing, named for a simple metal frame on which representations of the aircraft’s subsystems are installed, connected, and checked out.
Building such a testbed is a common practice for development programs in which many aircraft will be manufactured. But since the X-59 is a one-of-a-kind airplane, officials decided it was better and less expensive to use the aircraft itself.
As a result, engineers dubbed this series of exercises “aluminum bird” testing, since that’s the metal the X-59 is mostly made of.
So, instead of testing an “iron bird” with copies of an aircraft’s systems on a non-descript frame, the “aluminum bird” used the actual aircraft and its systems, which in turn meant the test results gave everyone higher confidence in the design,
“It’s a perfect example of the old tried and true adage in aviation that says ‘Test what you fly. Fly what you test,’” Lin said.
Still Ahead for the X-59
With aluminum bird testing in the rearview mirror, the next milestone on the X-59’s path to first flight is take the airplane out on the taxiways at the airport adjacent to Lockheed Martin’s Skunk Works facility in Palmdale, California, where the X-59 was built. First flight would follow those taxi tests.
Already in the X-59’s logbook since the fully assembled and painted airplane made its public debut in January 2024:
A Flight Readiness Review in which a board of independent experts from across NASA completed a study of the X-59 project team’s approach to safety for the public and staff during ground and flight testing. A trio of important structural tests and critical inspections that included “shaking” the airplane to make sure there were no unexpected problems from the vibrations. Firing up the GE Aerospace jet engine for the first time after installation into the X-59, including a series of tests of the engine running with full afterburner. Checking the wiring that ties together the X-59’s flight computer, electronic systems, and other hardware to be sure there were no concerns about electromagnetic interference. Testing the aircraft’s ability to maintain a certain speed while flying, essentially a check of the X-59’s version of cruise control. The X-59 Tests in 59
Watch this video about the X-59 aluminum bird testing. It only takes a minute. Well, 59 seconds to be precise. About the Author
Jim Banke
Managing Editor/Senior WriterJim Banke is a veteran aviation and aerospace communicator with more than 40 years of experience as a writer, producer, consultant, and project manager based at Cape Canaveral, Florida. He is part of NASA Aeronautics' Strategic Communications Team and is Managing Editor for the Aeronautics topic on the NASA website.
Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASA_es Instagram logo @NASA@NASAaero@NASA_es Linkedin logo @NASA Explore More
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Last Updated May 15, 2025 EditorJim BankeContactMatt Kamletmatthew.r.kamlet@nasa.gov Related Terms
Aeronautics Advanced Air Vehicles Program Aeronautics Research Mission Directorate Ames Research Center Armstrong Flight Research Center Commercial Supersonic Technology Glenn Research Center Integrated Aviation Systems Program Langley Research Center Low Boom Flight Demonstrator Quesst (X-59) Quesst: The Vehicle Supersonic Flight View the full article
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By USH
What would you do if you suddenly felt an unseen presence, turned around—and found yourself face to face with a seven-foot-tall, insect-like entity? Since 2006, anglers along New Jersey’s Musconetcong River have reported startling encounters with just such a being: a towering, humanoid creature that closely resembles a praying mantis.
But these aren’t just fleeting sightings. Witnesses frequently describe deeply unsettling experiences: telepathic communication, a sense of their thoughts or memories being accessed, and profound physiological effects. Consistent patterns emerge—electronic devices glitch, the surrounding forest falls unnaturally silent, and a strange, low-frequency hum seems to vibrate through the air.
More intriguingly, these mantis-like figures aren’t limited to modern encounters. Strikingly similar forms appear in ancient art across the globe, from 8,000-year-old cave paintings to references in Egyptian iconography. Could these entities have been with us since the dawn of civilization?
Theories vary widely. Some suggest these beings are an advanced species of insectoid extraterrestrials, possibly master geneticists overseeing hybridization programs involving humanity. Others propose a more Earth-bound origin, perhaps they’re a secret lineage of evolved terrestrial insects, hiding in the shadows of time.
And then there’s the interdimensional hypothesis: that these creatures aren’t physical in the way we understand, but exist in a parallel state of reality, occasionally phasing into ours.
Some researchers have even speculated that geological fault lines, like those beneath the Musconetcong River, could serve as energetic gateways, allowing these entities to cross between dimensions.
One thing is clear: the Mantis beings are watching and they may have been here far longer than we’ve dared to imagine.
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By NASA
This artist’s concept depicts a magnetar – a type of neutron star with a strong magnetic field – losing material into space. Shown as thin green lines, the magnetic field lines influence the movement of charged material around the magnetar. NASA/JPL-Caltech Since the big bang, the early universe had hydrogen, helium, and a scant amount of lithium. Later, some heavier elements, including iron, were forged in stars. But one of the biggest mysteries in astrophysics is: How did the first elements heavier than iron, such as gold, get created and distributed throughout the universe?
“It’s a pretty fundamental question in terms of the origin of complex matter in the universe,” said Anirudh Patel, a doctoral student at Columbia University in New York. “It’s a fun puzzle that hasn’t actually been solved.”
Patel led a study using 20-year-old archival data from NASA and ESA telescopes that finds evidence for a surprising source of a large amount of these heavy elements: flares from highly magnetized neutron stars, called magnetars. The study is published in The Astrophysical Journal Letters.
Study authors estimate that magnetar giant flares could contribute up to 10% of the total abundance of elements heavier than iron in the galaxy. Since magnetars existed relatively early in the history of the universe, the first gold could have been made this way.
“It’s answering one of the questions of the century and solving a mystery using archival data that had been nearly forgotten,” said Eric Burns, study co-author and astrophysicist at Louisiana State University in Baton Rouge.
How could gold be made at a magnetar?
Neutron stars are the collapsed cores of stars that have exploded. They are so dense that one teaspoon of neutron star material, on Earth, would weigh as much as a billion tons. A magnetar is a neutron star with an extremely powerful magnetic field.
On rare occasions, magnetars release an enormous amount of high-energy radiation when they undergo “starquakes,” which, like earthquakes, fracture the neutron star’s crust. Starquakes may also be associated with powerful bursts of radiation called magnetar giant flares, which can even affect Earth’s atmosphere. Only three magnetar giant flares have been observed in the Milky Way and the nearby Large Magellanic Cloud, and seven outside.
Patel and colleagues, including his advisor Brian Metzger, professor at Columbia University and senior research scientist at the Flatiron Institute in New York, have been thinking about how radiation from giant flares could correspond to heavy elements forming there. This would happen through a “rapid process” of neutrons forging lighter atomic nuclei into heavier ones.
Protons define the element’s identity on the periodic table: hydrogen has one proton, helium has two, lithium has three, and so on. Atoms also have neutrons which do not affect identity, but do add mass. Sometimes when an atom captures an extra neutron the atom becomes unstable and a nuclear decay process happens that converts a neutron into a proton, moving the atom forward on the periodic table. This is how, for example, a gold atom could take on an extra neutron and then transform into mercury.
In the unique environment of a disrupted neutron star, in which the density of neutrons is extremely high, something even stranger happens: single atoms can rapidly capture so many neutrons that they undergo multiple decays, leading to the creation of a much heavier element like uranium.
When astronomers observed the collision of two neutron stars in 2017 using NASA telescopes and the Laser Interferomete Gravitational wave Observatory (LIGO), and numerous telescopes on the ground and in space that followed up the initial discovery, they confirmed that this event could have created gold, platinum, and other heavy elements. But neutron star mergers happen too late in the universe’s history to explain the earliest gold and other heavy elements. Recent research by co-authors of the new study — Jakub Cehula of Charles University in Prague, Todd Thompson of The Ohio State University, and Metzger — has found that magnetar flares can heat and eject neutron star crustal material at high speeds, making them a potential source.
A rupture in the crust of a highly magnetized neutron star, shown here in an artist’s rendering, can trigger high-energy eruptions. Credit: NASA’s Goddard Space Flight Center/S. Wiessinger New clues in old data
At first, Metzger and colleagues thought that the signature from the creation and distribution of heavy elements at a magnetar would appear in the visible and ultraviolet light, and published their predictions. But Burns in Louisiana wondered if there could be a gamma-ray signal bright enough to be detected, too. He asked Metzger and Patel to check, and they found that there could be such a signature.
“At some point, we said, ‘OK, we should ask the observers if they had seen any,’” Metzger said.
Burns looked up the gamma ray data from the last giant flare that has been observed, which was in December 2004. He realized that while scientists had explained the beginning of the outburst, they had also identified a smaller signal from the magnetar, in data from ESA (European Space Agency)’s INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), a recently retired mission with NASA contributions. “It was noted at the time, but nobody had any conception of what it could be,” Burns said.
Metzger remembers that Burns thought he and Patel were “pulling his leg” because the prediction from their team’s model so closely matched the mystery signal in the 2004 data. In other words, the gamma ray signal detected over 20 years ago corresponded to what it should look like when heavy elements are created and then distributed in a magnetar giant flare.
Patel was so excited, “I wasn’t thinking about anything else for the next week or two. It was the only thing on my mind,” he said.
Researchers supported their conclusion using data from two NASA heliophysics missions: the retired RHESSI (Reuven Ramaty High Energy Solar Spectroscopic Imager) and the ongoing NASA’s Wind satellite, which had also observed the magnetar giant flare. Other collaborators on the new study included Jared Goldberg at the Flatiron Institute.
Next steps in the magnetar gold rush
NASA’s forthcoming COSI (Compton Spectrometer and Imager) mission can follow up on these results. A wide-field gamma ray telescope, COSI is expected to launch in 2027 and will study energetic phenomena in the cosmos, such as magnetar giant flares. COSI will be able to identify individual elements created in these events, providing a new advancement in understanding the origin of the elements. It is one of many telescopes that can work together to look for “transient” changes across the universe.
Researchers will also follow up on other archival data to see if other secrets are hiding in observations of other magnetar giant flares.
“It very cool to think about how some of the stuff in my phone or my laptop was forged in this extreme explosion of the course of our galaxy’s history,” Patel said.
Media Contact
Elizabeth Landau
Headquarters, Washington
202-358-0845
elandau@nasa.gov
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