NASA Marshall Names Roger Baird Associate Director

NASA Marshall Names Roger Baird Associate Director

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Roger Baird has been selected as associate director of NASA’s Marshall Space Flight Center in Huntsville, Alabama.

In this role, Baird will lead execution and integration of the center’s business operations, mission support enterprise functions, and budget management. In addition, he will be a senior adviser in advancing the direction of the center’s future.

Baird will also help manage the center’s 7,000 civil service and contract employees and help oversee an annual budget of approximately $5 billion. He will provide executive leadership across Marshall’s mission support areas as well as the center’s diverse portfolio of human spaceflight, science, and technology efforts, which touch nearly every mission NASA pursues.

A headshot of an older white male in a grey suit
Roger Baird, associate director, NASA Marshall Space Flight Center
NASA

“I know Roger will make an excellent addition to Marshall’s leadership team,” said Center Director Joseph Pelfrey. “His dedication to NASA’s missions has helped shape Marshall into a powerful technical solutions provider for the agency and our industry partners. Roger’s leadership will be invaluable in this new era of space exploration.”

Baird previously served as associate director for operations of Marshall’s Engineering Directorate from 2020-2024, after being detailed to the position in 2019. Named to the Senior Executive Service position in March 2020, he provided senior management and leadership expertise for the evaluation of spacecraft, payloads and launch vehicle systems, and the integration of the associated budgets and resources authority for these efforts. He was responsible for planning, directing, and coordinating engineering project management and integration activities in support of Marshall’s programs and projects, and oversaw an annual budget of approximately $550 million, including management of a highly technical workforce of more than 2,500 civil service and contractor employees. 

In 2018, Baird was selected as manager of the Engineering Resource Management Office, where he was responsible for advising, coordinating, monitoring, directing and performing work associated with planning, programming, budgeting and managing the Engineering Directorate’s financial, human and infrastructure resources. 

Baird brings a wealth of expertise to the role, with 34 years of NASA experience in the areas of engineering design, development, testing, facility and budget management, and strategic workforce acquisition and development. He joined NASA in 1990 as an avionics engineer in Marshall’s Astrionics Laboratory and served in multiple technical leadership positions within the Engineering Directorate’s Space Systems Department, Spacecraft and Vehicle Systems Department, and Propulsion Systems Department.

A native of Birmingham, Alabama, Baird earned a bachelor’s degree in electrical engineering from the University of Alabama in Birmingham. 

Learn more about Marshall’s work to support the nation’s mission in space at:

https://www.nasa.gov/marshall

Lance D. Davis
Marshall Space Flight Center, Huntsville, Ala.
256-640-9065
lance.d.davis @nasa.gov

Hannah Maginot
Marshall Space Flight Center, Huntsville, Ala.
256-932-1937
hannah.l.maginot @nasa.gov

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Beth Ridgeway

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2025 Gateways to Blue Skies Competition

2025 Gateways to Blue Skies Competition

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A collage depicting agriculture, including a cow, a vineyard, freshly picked grapes, and a drone watering a field, with the 2025 Blue Skies Logo in the center.
Credit from left to right: Stijn Te Strake/Unsplash, Yamaha Motor Corp USA, Maja Petric/Unsplash, Adele Payman/Unsplash

The agriculture industry faces several challenges, including limited resources and growing demands to reduce agriculture’s environmental impact while increasing its climate resilience. NASA Aeronautics is dedicated to expanding its efforts to assist commercial, industry, and government partners in advancing aviation systems that could modernize capabilities in agriculture.

In NASA’s 2025 Gateways to Blue Skies Competition: AgAir (Aviation Solutions for Agriculture) collegiate student teams will conceptualize novel aviation systems that can be applied to agriculture by 2035 or sooner with the goal of improving production, efficiency, environmental impact, and extreme weather/climate resilience. 

  • Action Required: Teams of 2 to 6 students to submit a 5-7-page Proposal and 2-minute Video summarizing the team’s proposal concept. 
  • Deadline: Proposal and Video Submissions are due February 17, 2025.  
  • Forum & Award: We’ll pay you to travel! Up to 8 finalist teams will be selected by a panel of NASA and industry subject matter experts to receive an $8,000 stipend to facilitate full participation in the Gateways to Blue Skies Competition & Forum, held at NASA’s Armstrong Flight Research Center in Mountain View, CA, in May 2025. Winners are offered internships within NASA Aeronautics during the academic year following the competition. 
  • Contact: blueskies@nianet.org 

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Bailey G. Light

Tortoise Takes a Leisurely Stroll

Tortoise Takes a Leisurely Stroll

A gopher tortoise walks toward the camera along a gravelly road with one front leg and one hind leg in the air. The scales on its legs are in sharp detail, while the immediate foreground and background are blurry.
NASA/Daniel Casper

A NASA photographer captured this gopher tortoise walking on the Launch Pad 39B beach road at NASA’s Kennedy Space Center in Florida on June 4, 2014.

The undeveloped property on Kennedy Space Center is managed by the U.S. Fish and Wildlife Service through the Merritt Island National Wildlife Refuge. The refuge provides a habitat for 14 species federally listed as threatened or endangered, including the leatherback, green, Kemps Ridley, loggerhead and Atlantic hawksbill turtles.

Image Credit: NASA/Daniel Casper

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Monika Luabeya

Tyler Parsotan Takes a Long Look at the Transient Universe with NASA’s Swift

Tyler Parsotan Takes a Long Look at the Transient Universe with NASA’s Swift

Through a nonlinear path to success, research astrophysicist Tyler Parsotan discovers transformational science using Swift’s observations. 

Name: Tyler Parsotan
Formal Job Classification: Research astrophysicist
Organization: Astroparticle Physics Laboratory (Code 661), Astrophysics Science Division, Sciences and Exploration Directorate 

Headshot against a black background. Tyler Parsotan wears a wears a white shirt with a black tie.
Dr. Tyler Parsotan is a research astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Md. He helps operate the Bust Alert Telescope on board the Neil Gehrels Swift Observatory.
Courtesy of Tyler Parsotan

What do you do and what is most interesting about your role here at Goddard? 

I help operate the Burst Alert Telescope on board the Neil Gehrels Swift Observatory to study some of the most powerful astrophysical processes in the universe. What is most interesting is the engineering capabilities that have gone into the spacecraft to make it nimble and robust, allowing it to conduct a wide range of transformative science. 

Why did you become an astrophysicist?

Ever since I was young, I was fascinated with the stars and how the world worked. All of this led me to physics with a focus on astrophysics. That is how I got into what I am doing now.

What is your educational background?

In 2015, I got a Bachelor of Science in space physics from Embry Riddle Aeronautical University in Daytona Beach, Florida. In 2019, I got a master’s in physics from Oregon State University, Corvallis, and in 2020 I got a master’s in mechanical engineering also from Oregon State University. In 2021, I got a doctorate in physics from Oregon State University. 

When I first applied to graduate school, I did not get into any. I was fortunate enough to learn about Oregon State University though a program geared towards allowing underrepresented students in STEM fields to get graduate degrees. This program, known as the Ronald E. McNair Post-baccalaureate Achievement Program, played a pivotal role in me being able to attend graduate school . 

Are you also a pilot?

Yes, I am. While I was in Oregon as a graduate student, I was able to save up enough money to get my private pilot’s license over the course of one summer from the local Corvallis airport. I would bike to the airport and get in a plane to fly all over Oregon from the coast to the Cascade Mountains. It was a very cool experience. 

How did you come to Goddard?

I did a post-doctorate fellowship starting the fall of 2021 through May 2023. My doctoral research was related to one of Swift’s many science focuses, so I wanted to continue my work at Goddard. 

What transformational science have you been involved with using Swift’s observations?

Some of the science that Swift focuses on is related to the transient universe, meaning that we primarily look at astrophysical events that come and go very quickly and typically produce a ton of energy. Swift examines the light energy produced from black holes, the majority of which are eating mass from black stars. 

While at Oregon State University, I studied the most energetic events in the universe known as gamma-ray bursts. I am now studying gamma-ray bursts at Goddard. One of the big discoveries made by Swift is that these gamma ray bursts can be seen out to early times in the universe. Some of these explosions occurred when the universe was very young, only 100,000 years old or so. Because the universe is expanding, it takes that light some time to travel to us. With Swift, we detect that light and can make some measurements about the gamma-ray bursts, such as when they occurred, how much energy they produced in these massive explosions, and some of the properties of the early universe. 

Man stands next to spacecraft model and his Robert H. Goddard Award for Exceptional Achievement for Science. He wears a blue button-down shirt and black pants.
“There are no linear paths to success,” said Tyler. “Keep looking for a way to be successful. This advice applies to life overall.”
Courtesy of Tyler Parsotan

What is the biggest discovery you have been involved with and what do you love most about working on Swift?

We are simulating the gamma-ray bursts, which was a focus of my doctorate. We cannot yet actually see these explosions, so we have to simulate them using the physics that we now know. I have been able to connect some of the large simulations to the Swift observations and measurements. This helps us better understand the underlying physics of these powerful explosions. 

The amount of energy produced in a typical gamma-ray burst is enough to blow up the Sun a few times over.

Lots of people know about Hubble, which observes the light that we can see with our eyes. The light that I deal with, gamma rays, has much higher energy and cannot be seen with our eyes. We have to use different techniques to measure this light. Designing detectors to measure this light is challenging technically but means that this area of physics is ripe for discovery. I love being part of this. 

Swift will be 20 years old in November 2024. As a relative newcomer to Swift, what are your thoughts?

I think Swift is a great observatory because it has conducted lots of transformational science, drastically expanding our knowledge of the cosmos. Even though it is getting older, it is still able to push science forward in new and exciting ways. I am looking forward to helping the Swift mission celebrate 20 years of amazing science. 

What is your advice to anyone starting and continuing a career?

There are no linear paths to success. Keep looking for a way to be successful. This advice applies to life overall. 

Are you involved in any of Goddard’s extracurricular activities?

I recently joined Goddard’s soccer league. Everyone at Goddard self organizes into teams that play each other after work during the week. We play about a game a week. The winning team gets bragging rights. I mostly play defense. Being on a team is a good way to meet people at Goddard and to stay active. 

In addition to soccer, what are your hobbies?

I enjoy hiking, mountain biking, and generally being outdoors. 

Where do you see yourself in five years?

I hope to still be at Goddard. I enjoy the type of work and the overall work environment. If Swift continues another five years, hopefully I’ll be working on it and also helping to create the next generation of gamma-ray observatories to help push science forward. We are making the science that will be in the next textbooks. 

Who do you want to thank?

My doctoral supervisor Davide Lazzati was an extremely supportive mentor and pushed me to be the best scientist that I can be. Since I arrived at Goddard, we have been good colleagues. 

My former mentor and supervisor at Goddard is Brad Cenko, the Swift principal investigator. I am grateful that he hired me and allowed me to grow as a post-doctoral researcher.

I also want to thank my entire family for being extremely supportive and understanding even though they may not fully understand what I really do. 

Who is your science hero?

Copernicus. He put forward the theory that our solar system orbits the Sun. He was obviously very instrumental in changing the way we think about the cosmos. He got into a lot of trouble with his theory, which makes his accomplishments all the more important. 

By Elizabeth M. Jarrell
NASA’s Goddard Space Flight Center, Greenbelt, Md.

A banner graphic with a group of people smiling and the text "Conversations with Goddard" on the right. The people represent many genders, ethnicities, and ages, and all pose in front of a soft blue background image of space and stars.

Conversations With Goddard is a collection of Q&A profiles highlighting the breadth and depth of NASA’s Goddard Space Flight Center’s talented and diverse workforce. The Conversations have been published twice a month on average since May 2011. Read past editions on Goddard’s “Our People” webpage.

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Madison Olson

Danish Instrument Helps NASA’s Juno Spacecraft See Radiation

Danish Instrument Helps NASA’s Juno Spacecraft See Radiation

Using cameras designed for navigation, scientists count ‘fireflies’ to determine the amount of radiation the spacecraft receives during each orbit of Jupiter.

Scientists with NASA’s Juno mission have developed the first complete 3D radiation map of the Jupiter system. Along with characterizing the intensity of the high-energy particles near the orbit of the icy moon Europa, the map shows how the radiation environment is sculpted by the smaller moons orbiting near Jupiter’s rings.

The work relies on data collected by Juno’s Advanced Stellar Compass (ASC), which was designed and built by the Technical University of Denmark, and the spacecraft’s Stellar Reference Unit (SRU), which was built by Leonardo SpA in Florence, Italy. The two datasets complement each other, helping Juno scientists characterize the radiation environment at different energies.

Both the ASC and SRU are low-light cameras designed to assist with deep-space navigation. These types of instruments are on almost all spacecraft. But to get them to operate as radiation detectors, Juno’s science team had to look at the cameras in a whole new light.

“On Juno we try to innovate new ways to use our sensors to learn about nature, and we have used many of our science instruments in ways they were not designed for,” said Scott Bolton, Juno principal investigator from the Southwest Research Institute in San Antonio. “This is the first detailed radiation map of the region at these higher energies, which is a major step in understanding how Jupiter’s radiation environment works. This will help planning observations for the next generation of missions to the Jovian system.”

Counting Fireflies

Consisting of four star cameras on the spacecraft’s magnetometer boom, Juno’s ASC takes images of stars to determine the spacecraft’s orientation in space, which is vital to the success of the mission’s magnetic field experiment. But the instrument has also proved to be a valuable detector of high-energy particle fluxes in Jupiter’s magnetosphere. The cameras record “hard radiation,” or ionizing radiation that impacts a spacecraft with sufficient energy to pass through the ASC’s shielding.

“Every quarter-second, the ASC takes an image of the stars,” said Juno scientist John Leif Jørgensen of the Technical University of Denmark. “Very energetic electrons that penetrate its shielding leave a telltale signature in our images that looks like the trail of a firefly. The instrument is programmed to count the number of these fireflies, giving us an accurate calculation of the amount of radiation.”

Jupiter’s moon Europa was captured by the JunoCam instrument aboard NASA’s Juno spacecraft during the mission’s close flyby on Sept. 29, 2022.
Image data: NASA/JPL-Caltech/SwRI/MSSS. Image processing: Björn Jónsson (CC BY 3.0)

Because of Juno’s ever-changing orbit, the spacecraft has traversed practically all regions of space near Jupiter.

ASC data suggests that there is more very high-energy radiation relative to lower-energy radiation near Europa’s orbit than previously thought. The data also confirms that there are more high-energy electrons on the side of Europa facing its orbital direction of motion than on the moon’s trailing side. This is because most of the electrons in Jupiter’s magnetosphere overtake Europa from behind due to the planet’s rotation, whereas the very high-energy electrons drift backward, almost like fish swimming upstream, and slam into Europa’s front side.

Jovian radiation data is not the ASC’s first scientific contribution to the mission. Even before arriving at Jupiter, ASC data was used to determine a measurement of interstellar dust impacting Juno. The imager also discovered a previously uncharted comet using the same dust-detection technique, distinguishing small bits of the spacecraft ejected by microscopic dust impacting Juno at a high velocity.

Dust Rings

Like Juno’s ASC, the SRU has been used as a radiation detector and a low-light imager. Data from both instruments indicates that, like Europa, the small “shepherd moons” that orbit within or close to the edge of Jupiter’s rings (and help to hold the shape of the rings) also appear to interact with the planet’s radiation environment. When the spacecraft flies on magnetic field lines connected to ring moons or dense dust, the radiation count on both the ASC and SRU drops precipitously. The SRU is also collecting rare low-light images of the rings from Juno’s unique vantage point.

“There is still a lot of mystery about how Jupiter’s rings were formed, and very few images have been collected by prior spacecraft,” said Heidi Becker, lead co-investigator for the SRU and a scientist at NASA’s Jet Propulsion Laboratory in Southern California, which manages the mission. “Sometimes we’re lucky and one of the small shepherd moons can be captured in the shot. These images allow us to learn more precisely where the ring moons are currently located and see the distribution of dust relative to their distance from Jupiter.”

More About the Mission

NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. The Technical University of Denmark designed and built the Advanced Stellar Compass. The Stellar Reference Unit was built by Leonardo SpA in Florence, Italy. Lockheed Martin Space in Denver built and operates the spacecraft.

More information about Juno is available at:

https://www.nasa.gov/juno

News Media Contacts

DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov

Karen Fox / Alana Johnson
NASA Headquarters, Washington
202-385-1600
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

Simon Koefoed Toft
Technical University of Denmark, Copenhagen
+45 9137 0088 
sito@dtu.dk

Deb Schmid
Southwest Research Institute, San Antonio
210-522-2254
dschmid@swri.org

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Naomi Hartono