Help Map the Moon’s Molten Flows!

Help Map the Moon’s Molten Flows!

1 min read

Help Map the Moon’s Molten Flows!

moon surface
Cooled, lava-like flows of impact melt that streamed out of Little Lowell Crater. As a volunteer for the Lunar Melt Citizen Science Project, you’ll help identify and measure rocks and craters in images like this one.
Credit: NASA/GSFC/Arizona State University

When asteroids hit the Moon, the impacts carve out craters and with enough energy and pressure, melt parts of the rocky surface. Often, the white hot, gooey melt (it’s like lava, except that it doesn’t erupt from underground) sloshes around the new crater and surrounding regions. The molten rock cools and hardens into vast rock features called impact melt flow deposits. These flow deposits are sculpture-like abstract art with beautiful lines and textures.

Now, scientists at the Lunar Melt citizen science project are asking for your help mapping these flows. You’ll be marking rocks, measuring the lengths of boulders, and outlining craters and melt deposits in images from NASA’s Lunar Reconnaissance Orbiter spacecraft.

Your contributions will help reveal how impact melt has changed the Moon’s surface, especially around Little Lowell Crater and Tycho Crater, and help scientists use impact melt flows to learn about the moon’s interior.

Help planetary scientists map the geology of lava-like flows on the Moon! Sign up at mappers.psi.edu, and tell your friends!

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Sep 24, 2025

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Airplane Aerobatics

Airplane Aerobatics

A man in a dark blue jumpsuit faces away from the camera, watching a plane in the light blue sky. He shades his eyes with his right hand.
NASA/Bill Ingalls

NASA astronaut Nick Hague watches as Robert Schmidle Pitts Aerobatics perform, Friday, Sept. 12, 2025, at Joint Base Andrews in Prince George’s County, Maryland. Hague spent 171 days aboard the International Space Station as part of Expedition 72.

While aboard the orbital laboratory, Hague and fellow NASA astronauts Suni Williams and Butch Wilmore completed more than 900 hours of research between more than 150 unique scientific experiments and technology demonstrations. Some of the research conducted included growing microalgae that could convert carbon dioxide into oxygen for the crew to breathe and testing an exercise device to keep crews healthy on long-duration missions.

Image credit: NASA/Bill Ingalls

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Monika Luabeya

La NASA y la NOAA lanzan tres naves espaciales para cartografiar la influencia del Sol en el espacio

La NASA y la NOAA lanzan tres naves espaciales para cartografiar la influencia del Sol en el espacio

A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On-Lagrange 1 (SWFO-L1) missions launches from the agency’s Kennedy Space Center in Florida, Wednesday, Sept. 24, 2025.
Un cohete Falcon 9 de SpaceX que transporta las misiones Sonda de Cartografía y Aceleración Interestelar (IMAP, por su acrónimo en inglés) y el Observatorio Carruthers de la Geocorona, ambos de la NASA, y la nave espacial de Seguimiento de la Meteorología Espacial en el Punto de Lagrange 1 (SWFO-L1, por sus siglas en inglés) de la NOAA, despega desde el Centro Espacial Kennedy de la NASA en Florida el miércoles 24 de septiembre de 2025.
Crédito: NASA

Read this press release in English here.

La NASA y la Administración Nacional Oceánica y Atmosférica (NOAA, por sus siglas en inglés) lanzaron el miércoles tres nuevas misiones para investigar la influencia del Sol en todo el sistema solar.

A las 7:30 a. m. EDT, un cohete Falcon 9 de SpaceX despegó del Complejo de Lanzamiento 39A del Centro Espacial Kennedy de la NASA en Florida, llevando a bordo las misiones Sonda de Cartografía y Aceleración Interestelar (IMAP, por su acrónimo en inglés) y el Observatorio Carruthers de la Geocorona, ambos de la NASA, y la nave espacial de Seguimiento de la Meteorología Espacial en el Punto de Lagrange 1 (SWFO-L1, por sus siglas en inglés) de la NOAA.

“Este exitoso lanzamiento mejora la preparación de nuestro país ante las condiciones meteorológicas espaciales para proteger mejor nuestros satélites, misiones interplanetarias y astronautas que viajan al espacio de los peligros de la meteorología espacial en todo el sistema solar”, afirmó el administrador interino de la NASA, Sean Duffy. “Esta información será fundamental a medida que nos preparamos para futuras misiones a la Luna y Marte con la intención de mantener a Estados Unidos a la vanguardia en el espacio”.

Estas misiones ayudarán a proteger de las duras condiciones de la meteorología espacial tanto a nuestra tecnología basada en tierra como a nuestros exploradores espaciales humanos y robóticos.

“Mientras Estados Unidos se prepara para enviar a seres humanos de vuelta a la Luna y más adelante a Marte, la NASA y la NOAA están proporcionando la guía definitiva de supervivencia interplanetaria para dar apoyo a este épico viaje de la humanidad”, afirmó Nicola Fox, administradora asociada de la Dirección de Misiones Científicas de la sede central de la NASA en Washington. “Nuestros descubrimientos científicos e innovaciones técnicas se incorporan directamente a nuestro plan de acción know-before-you-go (infórmate antes de ir) para garantizar una presencia humana bien preparada, segura y continua en otros mundos”.

Nueva ciencia para proteger a la sociedad

Cada misión investigará los diferentes efectos de la meteorología espacial y el viento solar, el cual es un flujo continuo de partículas emitidas por el Sol, desde su origen en nuestra estrella hasta el espacio interestelar.

“Estas tres misiones únicas nos ayudarán a conocer nuestro Sol y sus efectos sobre la Tierra mejor que nunca”, afirmó Joe Westlake, director de la División de Heliofísica en la sede central de la NASA. “Este conocimiento es fundamental, ya que la actividad solar afecta directamente a nuestra vida cotidiana, desde las redes eléctricas hasta el GPS. Estas misiones nos ayudarán a garantizar la seguridad y la resiliencia de nuestro mundo interconectado”.

La misión IMAP trazará los límites de la heliosfera, una burbuja inflada por el viento solar que protege nuestro sistema solar de los rayos cósmicos galácticos. Esta es una protección clave que contribuye a que nuestro planeta sea habitable. Además, la nave espacial tomará muestras y medirá las partículas del viento solar que fluyen hacia el exterior desde el Sol, así como las partículas energéticas que fluyen hacia el interior desde los límites de nuestro sistema solar y más allá.

“IMAP nos ayudará a comprender mejor cómo el entorno espacial puede perjudicarnos a nosotros y a nuestras tecnologías, y a descubrir la ciencia de nuestro vecindario solar”, afirmó David McComas, investigador principal de la misión IMAP en la Universidad de Princeton, en Nueva Jersey.

El Observatorio Carruthers de la Geocorona es la primera misión dedicada a medir los cambios en la capa más externa de nuestra atmósfera, la exosfera, la cual juega un papel importante en cómo la Tierra responde a la meteorología espacial. Al estudiar la geocorona —el brillo ultravioleta que emite la exosfera cuando la luz del sol la ilumina— la misión Carruthers revelará cómo la exosfera responde a las tormentas solares y cómo cambia con las estaciones. La misión se basa en el legado del primer instrumento que capturó imágenes de la geocorona, el cual viajó a la Luna a bordo de Apolo 16 y fue construido y diseñado por el científico, inventor, ingeniero y educador Dr. George Carruthers.

“La misión Carruthers nos mostrará cómo funciona la exosfera y nos ayudará a mejorar nuestra capacidad para predecir los efectos de la actividad solar aquí en la Tierra”, dijo Lara Waldrop, investigadora principal de la misión en la Universidad de Illinois en Urbana-Champaign.

La nave SWFO-L1 de la NOAA, la primera de su tipo, está diseñada para ser un observatorio de meteorología espacial operativo a tiempo completo. Al vigilar la actividad solar y las condiciones espaciales cerca de la Tierra las 24 horas del día, los 7 días de la semana, sin interrupciones ni obstrucciones, SWFO-L1 proporcionará pronósticos de meteorología espacial más rápidos y precisos que nunca.

“Se trata del primero de una nueva generación de observatorios de meteorología espacial de la NOAA dedicados a operaciones ininterrumpidas, que trabajarán para evitar lagunas en la continuidad. Las observaciones en tiempo real de SWFO-L1 proporcionarán a los operadores los datos fiables necesarios para emitir alertas tempranas, de modo que los responsables de la toma de decisiones puedan actuar con antelación para proteger las infraestructuras vitales, los intereses económicos y la seguridad nacional en la Tierra y en el espacio. Se trata de proteger a la sociedad contra los peligros de la meteorología espacial”, dijo Richard Ullman, subdirector de la Oficina de Observaciones de la Meteorología Espacial de la NOAA

Siguientes pasos

En las horas posteriores al lanzamiento, las tres naves espaciales se desplegaron desde el cohete con éxito y enviaron señales a la Tierra para confirmar que están activas y funcionando correctamente.

Durante los próximos meses, los satélites se dirigirán a su destino, un lugar situado entre la Tierra y el Sol, a unos 1,6 millones de kilómetros de la Tierra, denominado punto de Lagrange 1 (L1). Se espera que lleguen en enero y, una vez completadas las comprobaciones y calibraciones de sus instrumentos, comiencen sus misiones para comprender mejor la meteorología espacial y proteger a la humanidad.

David McComas, de la Universidad de Princeton, dirige la misión IMAP con un equipo internacional formado por 27 instituciones asociadas. El Laboratorio de Física Aplicada de la Universidad Johns Hopkins, ubicado en Laurel, Maryland, construyó la nave espacial y operará la misión.

La misión del Observatorio Carruthers de la Geocorona está dirigida por Lara Waldrop, de la Universidad de Illinois Urbana-Champaign. La ejecución de la misión está a cargo del Laboratorio de Ciencias Espaciales de la Universidad de California, Berkeley, que también diseñó y construyó los dos generadores de imágenes ultravioletas. BAE Systems diseñó y construyó la nave espacial Carruthers.

La División de Proyectos de Exploradores y Heliofísica de la NASA en el Centro de Vuelo Espacial Goddard de la NASA en Greenbelt, Maryland, gestiona las misiones IMAP y Observatorio Carruthers de la Geocorona para la Dirección de Misiones Científicas de la NASA.

La misión SWFO-L1 está gestionada por la NOAA y desarrollada en colaboración con el centro Goddard de la NASA y socios comerciales. El Programa de Servicios de Lanzamiento de la NASA, con sede en el centro Kennedy de la NASA, gestiona el servicio de lanzamiento de las misiones.

Para obtener más información sobre estas misiones, visite:

https://ciencia.nasa.gov/sol

-fin-

Abbey Interrante / María José Viñas
Sede central, Washington
301-201-0124
abbey.a.interrante@nasa.gov / maria-jose.vinasgarcia@nasa.gov

Sarah Frazier
Centro de Vuelo Espacial Goddard, Greenbelt, Maryland
202-853-7191
sarah.frazier@nasa.gov

Leejay Lockhart
Centro Espacial Kennedy, Florida
321-747-8310
leejay.lockhart@nasa.gov

John Jones-Bateman
Servicio de Satélites e Información de la NOAA, Silver Spring, Maryland
202-242-0929
john.jones-bateman@noaa.gov

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Tiernan P. Doyle

NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way

NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way

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NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way

A wide view of a region of space filled with stars and clumps of orange clouds.
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. Full image and caption below.
Credits:
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

NASA’s James Webb Space Telescope has revealed a colorful array of massive stars and glowing cosmic dust in the Sagittarius B2 molecular cloud, the most massive and active star-forming region in our Milky Way galaxy. 

“Webb’s powerful infrared instruments provide detail we’ve never been able to see before, which will help us to understand some of the still-elusive mysteries of massive star formation and why Sagittarius B2 is so much more active than the rest of the galactic center,” said astronomer Adam Ginsburg of the University of Florida, principal investigator of the program.

Image A: Sagittarius B2 (NIRCam Image)

A wide view of a region of space filled with stars and clumps of orange clouds.
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through some of the area’s thick clouds to reveal young stars and the warm dust surrounding them. 

However, one of the most notable aspects of Webb’s images of Sagittarius B2 are the portions that remain dark. These ironically empty-looking areas of space are actually so dense with gas and dust that even Webb cannot see through them. These thick clouds are the raw material of future stars and a cocoon for those still too young to shine.

The high resolution and mid-infrared sensitivity of Webb’s MIRI (Mid-Infrared Instrument) revealed this region in unprecedented detail, including glowing cosmic dust heated by very young massive stars. The reddest area on the right half of MIRI’s image, known as Sagittarius B2 North, is one of the most molecularly rich regions known, but astronomers have never seen it with such clarity. (Note: North is to the right in these Webb images.)

Image B: Sagittarius B2 (MIRI Image)

Cosmic clouds of pink and purple, some with bright centers, are surrounded by dark areas that appear like black space dotted with bright blue stars. A group of small clouds to the right is more red than any other area of the image.
Webb’s MIRI instrument shows the Sagittarius B2 region in mid-infrared light, with warm dust glowing brightly. Only the brightest stars emit strongly enough to appear through the dense clouds as blue pinpoints.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

The difference longer wavelengths of light make, even within the infrared spectrum, are stark when comparing the images from Webb’s MIRI and NIRCam (Near-Infrared Camera) instruments. Glowing gas and dust appear dramatically in mid-infrared light, while all but the brightest stars disappear from view.

In contrast to MIRI, colorful stars steal the show in Webb’s NIRCam image, punctuated occasionally by bright clouds of gas and dust. Further research into these stars will reveal details of their masses and ages, which will help astronomers better understand the process of star formation in this dense, active galactic center region. Has it been going on for millions of years? Or has some unknown process triggered it only recently?

Image C: Compare NIRCam and MIRI Images of Sagittarius B2




NIRCam
MIRI

A wide view of a region of space filled with stars and clumps of orange clouds.
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

Cosmic clouds of pink and purple, some with bright centers, are surrounded by dark areas that appear like black space dotted with bright blue stars. A group of small clouds to the right is more red than any other area of the image.

A wide view of a region of space filled with stars and clumps of orange clouds.
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
Cosmic clouds of pink and purple, some with bright centers, are surrounded by dark areas that appear like black space dotted with bright blue stars. A group of small clouds to the right is more red than any other area of the image.

NIRCam

MIRI

Compare NIRCam and MIRI Images of Sagittarius B2


Slide between these images from Webb to see what different wavelengths of infrared light reveal and conceal. Near-infrared light, which is nearest to visible red, comes from some gas and an abundance of colorful stars. The longer wavelengths of mid-infrared light are emitted by warm dust and only the brightest stars. Credits: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)

Astronomers hope Webb will shed light on why star formation in the galactic center is so disproportionately low. Though the region is stocked with plenty of gaseous raw material, on the whole it is not nearly as productive as Sagittarius B2. While Sagittarius B2 has only 10 percent of the galactic center’s gas, it produces 50 percent of its stars. 

“Humans have been studying the stars for thousands of years, and there is still a lot to understand,” said Nazar Budaiev, a graduate student at the University of Florida and the co-principal investigator of the study. “For everything new Webb is showing us, there are also new mysteries to explore, and it’s exciting to be a part of that ongoing discovery.”

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing 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 CSA (Canadian Space Agency).

To learn more about Webb, visit:

https://science.nasa.gov/webb

Related Information

Read more: NASA’s Webb Reveals New Features in Heart of Milky Way

Explore: ViewSpace interactive image tour of the center of the Milky Way

Explore: ViewSpace interactive views of the Eagle Nebula in different forms of light

Read more: Webb’s Star Formation Discoveries

Read more: Star formation in the Cat’s Paw Nebula

More Webb News

More Webb Images

Webb Science Themes

Webb Mission Page

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Last Updated
Sep 24, 2025
Editor
Marty McCoy
Contact
Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Leah Ramsay
Space Telescope Science Institute
Baltimore, Maryland

Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

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NASA, NOAA Launch Three Spacecraft to Map Sun’s Influence Across Space

NASA, NOAA Launch Three Spacecraft to Map Sun’s Influence Across Space

A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On-Lagrange 1 (SWFO-L1) missions launches from the agency’s Kennedy Space Center in Florida, Wednesday, Sept. 24, 2025.
A SpaceX Falcon 9 rocket carrying NASA’s IMAP (Interstellar Mapping and Acceleration Probe), Carruthers Geocorona Observatory, and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On-Lagrange 1 (SWFO-L1) missions launches from the agency’s Kennedy Space Center in Florida, Wednesday, Sept. 24, 2025.
Credit: NASA

Lee este comunicado de prensa en español aquí.

NASA and the National Oceanic and Atmospheric Administration (NOAA) launched three new missions Wednesday to investigate the Sun’s influence across the solar system.

At 7:30 a.m. EDT, a SpaceX Falcon 9 rocket lifted off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida carrying the agency’s IMAP (Interstellar Mapping and Acceleration Probe), Carruthers Geocorona Observatory, and NOAA’s SWFO-L1 (Space Weather Follow On-Lagrange 1) spacecraft.

“This successful launch advances the space weather readiness of our nation to better protect our satellites, interplanetary missions, and space-faring astronauts from the dangers of space weather throughout the solar system,” said acting NASA Administrator Sean Duffy, “This insight will be critical as we prepare for future missions to the Moon and Mars in our endeavor to keep America first in space.”

These missions will help safeguard both our ground-based technology, as well as our human and robotic space explorers from the harsh conditions known of space weather.

“As the United States prepares to send humans back to the Moon and onward to Mars, NASA and NOAA are providing the ultimate interplanetary survival guide to support humanity’s epic journey along the way,” said Nicola Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “Our scientific discoveries and technical innovations directly feed into our know-before-you-go roadmap to ensure a prepared, safe, and sustained human presence on other worlds.”

New science to protect society

Each mission will investigate different effects of space weather and the solar wind, which is a continuous stream of particles emitted by the Sun, from their origins at the Sun all the way outward to interstellar space.

“These three unique missions will help us get to know our Sun and its effects on Earth better than ever before,” said Joe Westlake, Heliophysics Division director at NASA Headquarters. “This knowledge is critical because the Sun’s activity directly impacts our daily lives, from power grids to GPS. These missions will help us ensure the safety and resilience of our interconnected world.”

The IMAP mission will chart the boundary of the heliosphere, a bubble inflated by the solar wind that shields our solar system from galactic cosmic rays — a key protection that helps make our planet habitable. In addition, the spacecraft will sample and measure solar wind particles streaming outward from the Sun, as well as energetic particles streaming inward from the boundary of our solar system and beyond.

“IMAP will help us better understand how the space environment can harm us and our technologies, and discover the science of our solar neighborhood,” said David McComas, IMAP mission principal investigator at Princeton University in New Jersey.

The Carruthers Geocorona Observatory is the first mission dedicated to recording changes in the outermost layer of our atmosphere, the exosphere, which plays an important role in Earth’s response to space weather. By studying the geocorona — the ultraviolet glow given off by the exosphere when sunlight shines on it — the Carruthers mission will reveal how the exosphere responds to solar storms and how it changes with the seasons. The mission builds on the legacy of the first instrument to image the geocorona, which flew to the Moon aboard Apollo 16 and was built and designed by scientist, inventor, engineer, and educator Dr. George Carruthers.

“The Carruthers mission will show us how the exosphere works and will help improve our ability to predict the impacts of solar activity here on Earth,” said Lara Waldrop, the mission’s principal investigator at the University of Illinois at Urbana-Champaign.

The first of its kind, NOAA’s SWFO-L1 is designed to be a full-time operational space weather observatory. By keeping a watchful eye on the Sun’s activity and space conditions near Earth 24/7, and without interruption or obstruction, SWFO-L1 will provide quicker and more accurate space weather forecasts than ever before.

“This is the first of a new generation of NOAA space weather observatories dedicated to 24/7 operations, working to avoid gaps in continuity. Real-time observations from SWFO-L1 will give operators the trusted data necessary to issue advance warnings so that decision-makers can take early action to protect vital infrastructure, economic interests, and national security on Earth and in space. It’s about safeguarding society against space weather hazards,” said Richard Ullman, deputy director of the Office of Space Weather Observations at NOAA. 

Next steps

In the hours after launch, all three spacecraft successfully deployed from the rocket and sent signals to Earth to confirm they’re active and working well.

Over the next few months, the spacecraft will make their way to their destination — a location between Earth and the Sun, about a million miles from Earth, called Lagrange point 1 (L1). They should arrive by January and, once their instrument checkouts and calibrations are complete, begin their missions to better understand space weather and protect humanity.

David McComas of Princeton University leads the IMAP mission with an international team of 27 partner institutions. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, built the spacecraft and will operate the mission.

The Carruthers Geocorona Observatory mission is led by Lara Waldrop from the University of Illinois Urbana-Champaign. Mission implementation is led by the Space Sciences Laboratory at University of California, Berkeley, which also designed and built the two ultraviolet imagers. BAE Systems designed and built the Carruthers spacecraft.

The Explorers and Heliophysics Projects Division at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the IMAP and Carruthers Geocorona Observatory missions for NASA’s Science Mission Directorate.

The SWFO-L1 mission is managed by NOAA and developed with NASA Goddard, and commercial partners. NASA’s Launch Services Program, based at NASA Kennedy, manages the launch service for the missions.

To learn more about these missions, visit:

https://www.nasa.gov/sun

-end-

Abbey Interrante
Headquarters, Washington
301-201-0124
abbey.a.interrante@nasa.gov

Sarah Frazier
Goddard Space Flight Center, Greenbelt, Md.
202-853-7191
sarah.frazier@nasa.gov

Leejay Lockhart
Kennedy Space Center, Fla.
321-747-8310
leejay.lockhart@nasa.gov

John Jones-Bateman
NOAA’s Satellite and Information Service, Silver Spring, Md.
202-242-0929
john.jones-bateman@noaa.gov

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Tiernan P. Doyle