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By Space Force
Natalia Serna, daughter of Space Launch Delta 30’s senior enlisted leader Chief Master Sgt. Jay Harris and Maria Tapia, wins U.S. Space Force's Military Child of the Year.
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By NASA
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
Acting 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, Leidos
Best Photography & Design
NASA’s 2024 Total Solar Eclipse Campaign
NASA
Events and Live streams
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, Leidos
Events and Live
NASA Streams Historic Cat Video From Deep Space
NASA’s Jet Propulsion Laboratory
Events and Live streams
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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By NASA
Norman Rockwell In his painting called Grissom and Young, American painter and illustrator Norman Rockwell captures technicians helping NASA astronauts John Young and Gus Grissom suit up for the first flight of the Gemini program in March 1965. NASA loaned Norman Rockwell a Gemini spacesuit to make this painting as accurate as possible.
Since its beginning, NASA has used the power of art to communicate the extraordinary aspects of its missions in a way that connects uniquely with humanity. NASA’s original art program, started in 1962 under the direction of Administrator James Webb, included a diverse collection of works from artists such as Rockwell, Andy Warhol, and Annie Leibovitz.
See more art inspired by NASA.
Image credit: Norman Rockwell
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By NASA
Explore This Section Earth Home Earth Observer Home Editor’s Corner Feature Articles Meeting Summaries News Science in the News Calendars In Memoriam More Archives 3 min read
Kaye Honored with Pecora Award
Expanded coverage of topics from “The Editor’s Corner” in The Earth Observer
Image. Recipient of the Pecora Individual Award: Jack A. Kaye, PhD. Image credit: Sources/Usage: Public Domain. View Media Details Jack Kaye, Associate Director for research with the Earth Science Division within NASA’s Science Mission Directorate, has received the Pecora award for his vision and creative leadership in multidisciplinary Earth science research, as well as spurring advancements in the investigator community, supporting development of sensors, and shaping NASA satellite and aircraft missions and research programs at the highest levels.
The William T. Pecora Award, presented annually by the U.S. Geological Survey (USGS) and NASA, honors individuals and groups who have made outstanding contributions to the field of remote sensing – advancing Earth observation and benefiting society.
As Associate Director for research since 1999, Kaye is responsible for the research and data analysis programs for Earth System Science. He has contributed to national and international groups for decades, by serving as the NASA principal on the Subcommittee on Global Change Research in the U.S. Global Change Research Program and chairing the World Meteorological Organization Expert Team on Satellite Systems. Kaye has also served as a member of the Steering Committee for the Global Climate Observing System and on the National Research Council’s Roundtable on Science and Technology for Sustainability and the Chemical Sciences Roundtable. He also serves as NASA’s representative to the Subcommittee on Ocean Science and Technology. Kaye has devoted considerable energy toward developing early career researchers, stimulating the inclusion of a more diverse student population in science, technology, engineering, and mathematics.
Kaye has received numerous NASA awards, including the Distinguished Service Medal in 2022 and the Meritorious Executive in the Senior Executive Service in 2004, 2010, and 2021. He was named a Fellow by the American Meteorological Society (AMS) in 2010 and by the American Association for the Advancement of Science (AAAS) in 2014. Kaye was also elected to serve as an office of the Atmospheric and Hydrospheric Science section of the AAAS (2015–2018).
Kaye received a Bachelor of Science degree from Adelphi University in 1976 and a Ph.D. from the California Institute of Technology in 1982. He held a post-doctoral research associateship at the U.S. Naval Research Laboratory. Kaye has published more than 50 refereed papers and contributed to numerous reports, books, and encyclopedias.
Kaye is joined in this honor by Chuanmin Hu, Professor of optical oceanography at the University of South Florida where he leads the Optical Oceanography Lab. Hu received the Pecora Group award for his lab’s groundbreaking advancements in remote sensing and real-world applications, including the Sargassum Watch System. The William T. Pecora Award honors the memory of William T. Pecora, former Director of USGS and Under Secretary of the Interior. His early vision and support helped establish what we know today as the Landsat satellite program.
Steve Platnick
EOS Senior Project Scientist
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Last Updated Mar 20, 2025 Related Terms
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By NASA
Explore This Section Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read NASA’s Webb Images Young, Giant Exoplanets, Detects Carbon Dioxide
NASA’s James Webb Space Telescope has provided the clearest look in the infrared yet at the iconic multi-planet system HR 8799. Full image below. Credits:
NASA, ESA, CSA, STScI, W. Balmer (JHU), L. Pueyo (STScI), M. Perrin (STScI) NASA’s James Webb Space Telescope has captured direct images of multiple gas giant planets within an iconic planetary system. HR 8799, a young system 130 light-years away, has long been a key target for planet formation studies.
The observations indicate that the well-studied planets of HR 8799 are rich in carbon dioxide gas. This provides strong evidence that the system’s four giant planets formed much like Jupiter and Saturn, by slowly building solid cores that attract gas from within a protoplanetary disk, a process known as core accretion.
The results also confirm that Webb can infer the chemistry of exoplanet atmospheres through imaging. This technique complements Webb’s powerful spectroscopic instruments, which can resolve the atmospheric composition.
“By spotting these strong carbon dioxide features, we have shown there is a sizable fraction of heavier elements, like carbon, oxygen, and iron, in these planets’ atmospheres,” said William Balmer, of Johns Hopkins University in Baltimore. “Given what we know about the star they orbit, that likely indicates they formed via core accretion, which is an exciting conclusion for planets that we can directly see.”
Balmer is the lead author of the study announcing the results published today in The Astrophysical Journal. Balmer and their team’s analysis also includes Webb’s observation of a system 97 light-years away called 51 Eridani.
Image A: HR 8799 (NIRCam Image)
NASA’s James Webb Space Telescope has provided the clearest look in the infrared yet at the iconic multi-planet system HR 8799. The closest planet to the star, HR 8799 e, orbits 1.5 billion miles from its star, which in our solar system would be located between the orbit of Saturn and Neptune. The furthest, HR 8799 b, orbits around 6.3 billion miles from the star, more than twice Neptune’s orbital distance. Colors are applied to filters from Webb’s NIRCam (Near-Infrared Camera), revealing their intrinsic differences. A star symbol marks the location of the host star HR 8799, whose light has been blocked by the coronagraph. In this image, the color blue is assigned to 4.1 micron light, green to 4.3 micron light, and red to the 4.6 micron light. NASA, ESA, CSA, STScI, W. Balmer (JHU), L. Pueyo (STScI), M. Perrin (STScI) Image B: 51 Eridani (NIRCam Image)
Webb’s NIRCam (Near-Infrared Camera) captured this image of 51 Eridani b (also referred to as 51 Eri b), a cool, young exoplanet that orbits 890 million miles from its star, similar to Saturn’s orbit in our solar system. The 51 Eridani system is 97 light-years from Earth. This image includes filters representing 4.1-micron light as red. The background red in this image is not light from other planets, but a result of light subtraction during image processing. NASA, ESA, CSA, STScI, W. Balmer (JHU), L. Pueyo (STScI), M. Perrin (STScI) HR 8799 is a young system about 30 million years old, a fraction of our solar system’s 4.6 billion years. Still hot from their tumultuous formation, the planets within HR 8799 emit large amounts of infrared light that give scientists valuable data on how they formed.
Giant planets can take shape in two ways: by slowly building solid cores with heavier elements that attract gas, just like the giants in our solar system, or when particles of gas rapidly coalesce into massive objects from a young star’s cooling disk, which is made mostly of the same kind of material as the star. The first process is called core accretion, and the second is called disk instability. Knowing which formation model is more common can give scientists clues to distinguish between the types of planets they find in other systems.
“Our hope with this kind of research is to understand our own solar system, life, and ourselves in the comparison to other exoplanetary systems, so we can contextualize our existence,” Balmer said. “We want to take pictures of other solar systems and see how they’re similar or different when compared to ours. From there, we can try to get a sense of how weird our solar system really is—or how normal.”
Image C: Young Gas Giant HR 8799 e (NIRCam Spectrum)
This graph shows a spectrum of one of the planets in the HR 8799 system, HR 8799 e. Spectral fingerprints of carbon dioxide and carbon monoxide appear in data collected by Webb’s NIRCam (Near-Infrared Camera). NASA, ESA, CSA, STScI, J. Olmsted (STScI) Of the nearly 6,000 exoplanets discovered, few have been directly imaged, as even giant planets are many thousands of times fainter than their stars. The images of HR 8799 and 51 Eridani were made possible by Webb’s NIRCam (Near-Infrared Camera) coronagraph, which blocks light from bright stars to reveal otherwise hidden worlds.
This technology allowed the team to look for infrared light emitted by the planets in wavelengths that are absorbed by specific gases. The team found that the four HR 8799 planets contain more heavy elements than previously thought.
The team is paving the way for more detailed observations to determine whether objects they see orbiting other stars are truly giant planets or objects such as brown dwarfs, which form like stars but don’t accumulate enough mass to ignite nuclear fusion.
“We have other lines of evidence that hint at these four HR 8799 planets forming using this bottom-up approach” said Laurent Pueyo, an astronomer at the Space Telescope Science Institute in Baltimore, who co-led the work. “How common is this for planets we can directly image? We don’t know yet, but we’re proposing more Webb observations to answer that question.”
“We knew Webb could measure colors of the outer planets in directly imaged systems,” added Rémi Soummer, director of STScI’s Russell B. Makidon Optics Lab and former lead for Webb coronagraph operations. “We have been waiting for 10 years to confirm that our finely tuned operations of the telescope would also allow us to access the inner planets. Now the results are in and we can do interesting science with it.”
The NIRCam observations of HR 8799 and 51 Eridani were conducted as part of Guaranteed Time Observations programs 1194 and 1412 respectively.
The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.
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Media Contacts
Laura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Hannah Braun – hbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Roberto Molar Candanosa
Johns Hopkins University, Baltimore, Md.
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