Citizen Scientists Use NASA Open Science Data to Research Life in Space

Citizen Scientists Use NASA Open Science Data to Research Life in Space

2 min read

Citizen Scientists Use NASA Open Science Data to Research Life in Space

Large group photo of attendees at a NASA Analysis Working Group meeting, gathered in a conference room with round tables and chandeliers. A presentation screen is visible in the background.
2023 Workshop of Analysis Working Group members, Washington, D.C., November 14, 2023. Now, you are invited to join their quest to understand how life can thrive in deep space! Want to learn more first? Join our live virtual event April 17 at 3pm Eastern Time to hear an overview of the OSDR AWG’s operations.
Photo: NASA OSDR Team

How can life thrive in deep space? The Open Science Data Repository Analysis Working Groups invite volunteers from all backgrounds to help answer this question. Request to join these citizen science groups to help investigate how life adapts to space environments, exploring topics like radiation effects, microgravity’s impact on human and plant health, and how microbes change in orbit.

Currently, nine Analysis Working Groups (AWGs) hold monthly meetings to advance their specific focus areas. Participants collaborate using an online platform, the AWG “Forum-Space”, where they connect with peers and experts, join discussions, and contribute to over 20 active projects

The AWGs work with data primarily from the NASA Open Science Data Repository (OSDR), a treasure trove of spaceflight data on physiology, molecular biology, bioimaging, and much more. For newcomers, there are tutorials and a comprehensive paper covering all aspects of the repository and the AWG community. You can explore 500+ studies, an omics multi-study visualization portal, the environmental data app, and RadLab, a portal for radiation telemetry data. (“Omics” refers to fields of biology that end in “omics,” like “genomics”.)   

Each of the nine AWGs has a Lead who organizes their group and holds monthly virtual meetings. Once you join, make sure to connect with the Lead and get on the agenda so you can introduce yourself. Learn more about the AWGs here.

Have an idea for a new project? Propose a new project and help lead it! From data analysis and visualization to shaping data standards and conducting literature meta-analyses, there’s a place for everyone to contribute. Request to join, and together, we can address a great challenge for humanity: understanding and enabling life to thrive in deep space! 

Want to learn more?

On April 17 at 3pm Eastern Time, the NASA Citizen Science Leaders Series is hosting an virtual event with Ryan Scott about these Analysis Working Groups and their work. Ryan is the Science Lead for the Ames Life Sciences Data Archive and the liaison between the Open Data Science Repository and the Analysis Working Groups. Click here to register for this event!

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Apr 02, 2025

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Exercise Research Main Focus Aboard Station on Tuesday

Exercise Research Main Focus Aboard Station on Tuesday

NASA astronaut and Expedition 72 Flight Engineer Nick Hague exercises on the advanced resistive exercise device (ARED) aboard the International Space Station's Tranquility module. The ARED mimics the inertial forces of lifting free weights on Earth to maintain muscle health during long-term space missions. During his exercise session, Hague wore Bio-Monitor, a garment and headband set outfitted with sensors to collect physiological data and minimally interfere with space station life. Hague wore the garment 48 hours as part of Vascular Aging, a study that monitors an astronaut’s cardiovascular health in space.
Astronaut Nick Hague exercises on Oct. 29, 2024, on the advanced resistive exercise device that mimics the inertial forces of lifting free weights on Earth to maintain muscle health during long-term space missions.
NASA

Exercise research was back on the science schedule for the Expedition 72 crew on Tuesday ensuring astronauts stay healthy and in shape while living and working in weightlessness. The International Space Station residents also continued a host of other microgravity research exploring robotics, combustion, and more.

Space-caused muscle and bone loss are key concerns for NASA and its international partners planning long-duration crew missions to the Moon, Mars, and beyond. Scientists know that exercising two hours a day, seven days a week aboard the orbital outpost helps offset the effects of long-term weightlessness. However, continuous research is underway to learn how muscles and bones, including the heart and lungs, respond to a variety of space workouts to maximize the benefits of exercising in microgravity as crews spend more time off the Earth.

Flight Engineers Don Pettit and Takuya Onishi, during the first half of their shift, took turns pedaling on an exercise cycle while wearing breathing gear and electrodes attached to their chest inside the Destiny laboratory module. The data collected from the hardware measures the astronauts’ heart and breathing rate to evaluate aerobic capacity, or the bodies’ ability to deliver and use oxygen during strenuous physical activity, in space.

Afterward, Pettit from NASA activated an Astrobee robotic free-flyer and tested its abilities to recognize and respond to hand gestures ahead of a student competition to control the device using computer code. Onishi from JAXA (Japan Aerospace Exploration Agency) opened up Destiny’s Combustion Integrated Rack, adjusted fire safety research gear, and photographed the final configuration for analysis.

NASA Flight Engineer Anne McClain worked out on the advanced resistive exercise device (ARED), located in the Tranquility module, for the CIPHER suite of 14 human research investigations. She performed squats on the ARED that mimics free weights on Earth for the portion of the study assessing any changes to her cardiorespiratory fitness, muscle strength, and endurance due to living in weightlessness.

Next, McClain put on an experimental wearable dosimeter that measures radiation dosages crews are exposed to in real time. Finally, McClain joined NASA Flight Engineer Nichole Ayers and replaced power distribution hardware inside Tranquility at the end of their shift.

Roscosmos cosmonauts Alexey Ovchinin and Ivan Vagner tested the lower body negative pressure suit for its ability to reverse the space-caused flow of body fluids toward a crew member’s head. Results may prevent microgravity-induced head and eye pressure and help crews adjust quicker to the return to Earth’s gravity. Roscosmos Flight Engineer Kirill Peskov spent his shift cleaning ventilation systems, checking radiation detectors, and adjusting oxygen sensors on gas analyzers.

Learn more about station activities by following the space station blog, @space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia

NASA Receives 10 Nominations for the 29th Annual Webby Awards

NASA Receives 10 Nominations for the 29th Annual Webby Awards

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

This ultra high-definition video featuring an orange tabby cat named Taters, was streamed from nearly 19 million miles away via laser by NASA’s Deep Space Optical Communications (DSOC) experiment, marking a historic milestone for space communications.
Jet Propulsion Laboratory

Since it began in 1958, NASA has been charged by law with spreading the word about its work to the widest extent practicable. From typewritten press releases to analog photos and film, the agency has effectively moved into social media and other online communications. NASA’s broad reach across digital platforms has been recognized by the International Academy of Digital Arts and Sciences (IADAS), with 10 nominations across multiple categories for the academy’s 29th annual Webby Awards.

The 2025 Webby nominations demonstrate NASA’s dedication to sharing the wonders of space through digital platforms. We believe in the power of digital storytelling to inspire the next generation of explorers.

Michelle R. Jones

Michelle R. Jones

Deputy Associate Administrator for Communications

Public Voting Opportunities

Voting for the Webby People’s Voice Awards—chosen by the public—is open now through Thursday, April 17. Voting links for each category are listed below.

29th Annual Webby Award Nominees

AI, Immersive & Games

NASA’s Snap It! An Eclipse Photo Adventure
NASA
Kids and Family

Social

NASA Instagram
NASA
Education and Science

Matt Dominick’s X Account: A Visual Journey from Space
NASA
Best Photography & Design

NASA’s 2024 Total Solar Eclipse Campaign
NASA
Events and Livestreams

NASA’s Webb Telescope: Unfolding a Universe of Wonders
NASA Goddard
Education and Science

Video & Film

2024 Total Solar Eclipse: Through the Eyes of NASA
NASA
Events and Live

NASA Streams Historic Cat Video From Deep Space
NASA’s Jet Propulsion Laboratory
Events and Livestreams

Websites & Mobile Sites

NASA Website
NASA
Government & Associations

NASA+ Streaming Service
NASA
Television, Film & Streaming

NASA Newsletter
NASA
Business, News and Technology

About the Webby Awards

Established in 1996 during the web’s infancy, The Webbys is presented by the IADAS—a 3000+ member judging body. The Academy is comprised of Executive Members—leading Internet experts, business figures, luminaries, visionaries, and creative celebrities—and associate members who are former Webby winners, nominees and other internet professionals.

The Webby Awards presents two honors in every category—the Webby Award and the Webby People’s Voice Award. Members of the International Academy of Digital Arts and Sciences (IADAS) select the nominees for both awards in each category, as well as the winners of the Webby Awards. In the spirit of the open web, the Webby People’s Voice is chosen by the voting public, and garners millions of votes from all over the world.

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Dacia Massengill

NASA’s SPHEREx Takes First Images, Preps to Study Millions of Galaxies

NASA’s SPHEREx Takes First Images, Preps to Study Millions of Galaxies

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s SPHEREx, which will map millions of galaxies across the entire sky, captured one of its first exposures March 27. The observatory’s six detectors each captured one of these uncalibrated images, to which visible-light colors have been added to represent infrared wavelengths. SPHEREx’s complete field of view spans the top three images; the same area of the sky is also captured in the bottom three images.
NASA/JPL-Caltech

Processed with rainbow hues to represent a range of infrared wavelengths, the new pictures indicate the astrophysics space observatory is working as expected.

NASA’s SPHEREx (short for Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) has turned on its detectors for the first time in space. Initial images from the observatory, which launched March 11, confirm that all systems are working as expected.

Although the new images are uncalibrated and not yet ready to use for science, they give a tantalizing look at SPHEREx’s wide view of the sky. Each bright spot is a source of light, like a star or galaxy, and each image is expected to contain more than 100,000 detected sources.

There are six images in every SPHEREx exposure — one for each detector. The top three images show the same area of sky as the bottom three images. This is the observatory’s full field of view, a rectangular area about 20 times wider than the full Moon. When SPHEREx begins routine science operations in late April, it will take approximately 600 exposures every day.

Each image in this uncalibrated SPHEREx exposure contains about 100,000 light sources
Each image in this uncalibrated SPHEREx exposure contains about 100,000 light sources, including stars and galaxies. The two insets at right zoom in on sections of one image, showcasing the telescope’s ability to capture faint, distant galaxies. These sections are processed in grayscale rather than visible-light color for ease of viewing.
NASA/JPL-Caltech

“Our spacecraft has opened its eyes on the universe,” said Olivier Doré, SPHEREx project scientist at Caltech and NASA’s Jet Propulsion Laboratory, both in Southern California. “It’s performing just as it was designed to.”

The SPHEREx observatory detects infrared light, which is invisible to the human eye. To make these first images, science team members assigned a visible color to every infrared wavelength captured by the observatory. Each of the six SPHEREx detectors has 17 unique wavelength bands, for a total of 102 hues in every six-image exposure.

Breaking down color this way can reveal the composition of an object or the distance to a galaxy. With that data, scientists can study topics ranging from the physics that governed the universe less than a second after its birth to the origins of water in our galaxy.

“This is the high point of spacecraft checkout; it’s the thing we wait for,” said Beth Fabinsky, SPHEREx deputy project manager at JPL. “There’s still work to do, but this is the big payoff. And wow! Just wow!”

During the past two weeks, scientists and engineers at JPL, which manages the mission for NASA, have executed a series of spacecraft checks that show all is well so far. In addition, SPHEREx’s detectors and other hardware have been cooling down to their final temperature of around minus 350 degrees Fahrenheit (about minus 210 degrees Celsius). This is necessary because heat can overwhelm the telescope’s ability to detect infrared light, which is sometimes called heat radiation. The new images also show that the telescope is focused correctly. Focusing is done entirely before launch and cannot be adjusted in space.

“Based on the images we are seeing, we can now say that the instrument team nailed it,” said Jamie Bock, SPHEREx’s principal investigator at Caltech and JPL.

How It Works

Where telescopes like NASA’s Hubble and James Webb space telescopes were designed to target small areas of space in detail, SPHEREx is a survey telescope and takes a broad view. Combining its results with those of targeted telescopes will give scientists a more robust understanding of our universe.

The observatory will map the entire celestial sky four times during its two-year prime mission. Using a technique called spectroscopy, SPHEREx will collect the light from hundreds of millions of stars and galaxies in more wavelengths any other all-sky survey telescope.

When light enters SPHEREx’s telescope, it’s directed down two paths that each lead to a row of three detectors. The observatory’s detectors are like eyes, and set on top of them are color filters, which are like color-tinted glasses. While a standard color filter blocks all wavelengths but one, like yellow- or rose-tinted glasses, the SPHEREx filters are more like rainbow-tinted glasses: The wavelengths they block change gradually from the top of the filter to the bottom.

“I’m rendered speechless,” said Jim Fanson, SPHEREx project manager at JPL. “There was an incredible human effort to make this possible, and our engineering team did an amazing job getting us to this point.”

More About SPHEREx

The SPHEREx mission is managed by JPL for the agency’s Astrophysics Division within the Science Mission Directorate at NASA Headquarters. BAE Systems (formerly Ball Aerospace) built the telescope and the spacecraft bus. The science analysis of the SPHEREx data will be conducted by a team of scientists located at 10 institutions in the U.S., two in South Korea, and one in Taiwan. Caltech managed and integrated the instrument. Data will be processed and archived at IPAC at Caltech. The mission’s principal investigator is based at Caltech with a joint JPL appointment. The SPHEREx dataset will be publicly available at the NASA-IPAC Infrared Science Archive. Caltech manages JPL for NASA.

For more about SPHEREx, visit:

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

News Media Contact

Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov

2025-045

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Anthony Greicius

Studying Ice for the Future of Flight

Studying Ice for the Future of Flight

A man looks at white ice built up on a section of scale-model transonic truss-braced wing. The model wing stands vertically in NASA Glenn’s Icing Research Tunnel.
NASA/Jordan Cochran

Thomas Ozoroski, a researcher at NASA’s Glenn Research Center in Cleveland, takes icing accretion measurements in October 2024 as part of transonic truss-braced wing concept research.

In the future, aircraft with long, thin wings supported by aerodynamic braces could help airlines save on fuel costs – but those same wings could be susceptible to ice buildup. In the historic Icing Research Tunnel at NASA Glenn, scientists and engineers are testing a concept for a transonic truss-braced wing. Their goal: to collect important data to inform the design of these potential efficient aircraft of the future.

NASA Glenn can simulate icing conditions in its Icing Research Tunnel to identify potential challenges for new aircraft designs. These tests provide valuable information about how ice builds up on wings and can help identify the most critical icing conditions for safety.

Read more about icing testing at NASA Glenn.

Image credit: NASA/Jordan Cochran

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Monika Luabeya