NASA Invites Media to View Heliophysics, NOAA Space Weather Missions

NASA Invites Media to View Heliophysics, NOAA Space Weather Missions

Technicians at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida conduct illumination testing on Friday, July 18, 2025, by flashing a bright light that simulates the Sun into the two-panel solar array that will help power the agency’s IMAP (Interstellar Mapping and Acceleration Probe) observatory on its upcoming journey to a destination about one million miles away from Earth Lagrange Point 1.
Technicians at the Astrotech Space Operations Facility near NASA’s Kennedy Space Center in Florida conduct illumination testing on Friday, July 18, 2025, by flashing a bright light that simulates the Sun into the two-panel solar array that will help power the agency’s IMAP (Interstellar Mapping and Acceleration Probe) observatory on its upcoming journey to a destination about one million miles away from Earth Lagrange Point 1.
Credit: NASA/Kim Shiflett

NASA invites media to view the agency’s IMAP (Interstellar Mapping and Acceleration Probe) spacecraft and two other missions — the Carruthers Geocorona Observatory and the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Follow On–Lagrange 1 (SWFO-L1) observatory, which will launch along with IMAP as rideshares.

Media will have the opportunity to photograph the three spacecraft and speak with subject matter experts representing all three missions. The event will take place on Thursday, Aug. 28, at the Astrotech Space Operations payload processing facility in Titusville, Florida. Confirmed media will receive additional details after registering.

To participate in the event, media must RSVP by 11:59 p.m. on Tuesday, Aug. 19, by submitting their request online at: https://media.ksc.nasa.gov.

The IMAP mission will study the heliosphere, a vast magnetic bubble created by the Sun that protects our solar system from radiation incoming from interstellar space. Carruthers will use its ultraviolet cameras to monitor how material from the Sun impacts the outermost part of Earth’s atmosphere. The SWFO-L1 mission will observe solar eruptions, and monitor incoming space weather 24/7, providing early warnings and validating forecasts that protect vital communication and navigation infrastructure, economic interests, and national security, both on Earth and in space.

NASA is targeting no earlier than September for the launch of these three missions on a SpaceX Falcon 9 rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.

NASA’s media accreditation policy is available online. For questions about accreditation, please email: ksc-media-accreditat@mail.nasa.gov.

Facility Access
Due to spacecraft cleanliness requirements, this invitation is open to a limited number of media with no more than two individuals per media organization. This event is open to U.S. citizens who possess a valid government-issued photo identification and proof of U.S. citizenship, such as a passport or birth certificate.

Media attending this event must comply with cleanroom guidelines. This includes wearing specific cleanroom garments; avoiding cologne, cosmetics, and high-heeled shoes; cleaning camera equipment under the supervision or assistance of contamination control specialists; and placing all electronics in airplane mode in the designated areas near the spacecraft. NASA will provide detailed guidance to approved media.

Observatories Information
The three observatories are preparing to launch to Lagrange point 1, which lies about a million miles from Earth toward the Sun. There, they will orbit this gravitational balance point, holding a steady position between Earth and the Sun. NASA’s IMAP will use its 10 instruments to map the heliosphere’s edge and reveal how the Sun accelerates charged particles, filling in essential puzzle pieces to understand the space weather environment across the solar system. The mission’s varied instruments also will provide near real-time space weather data to scientists on Earth.

The Carruthers observatory will image the glow of ultraviolet light emitted by the uppermost parts of Earth’s atmosphere — called the geocorona — to help researchers understand how our planet’s atmosphere is shaped by conditions in space. NOAA’s SWFO-L1 will use its suite of instruments to sample the solar wind and interplanetary magnetic field, while its onboard coronagraph will detect coronal mass ejections and other solar events. Together, these real-time observations of space weather enable precautionary actions to protect satellites, power grids, aviation, and communication and navigation technology.

Learn more about NASA’s IMAP at:

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

-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, Florida
321-747-8310
leejay.lockhart@nasa.gov

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Gerelle Q. Dodson

Rare Type of Black Hole Snacks on Star

Rare Type of Black Hole Snacks on Star

Two elliptical galaxies at upper right and lower left appear as fuzzy white ovals. At bottom center is a fuzzy purple blob. The main image also has two bright stars with prominent diffraction spikes. The background of space is black and is speckled with tiny white dots.⁣
Science: NASA, ESA, CXC, Yi-Chi Chang (National Tsing Hua University); Image Processing: Joseph DePasquale (STScI)

NASA’s Hubble Space Telescope and NASA’s Chandra X-ray Observatory teamed up to identify a new possible example of a rare class of black holes, identified by X-ray emission (in purple) in this image released on July 24, 2025. Called NGC 6099 HLX-1, this bright X-ray source seems to reside in a compact star cluster in a giant elliptical galaxy. These rare black holes are called intermediate-mass black holes (IMBHs) and weigh between a few hundred to a few 100,000 times the mass of our Sun.

Learn more about IMBHs and what studying them can tell us about the universe.

Image credit: Science: NASA, ESA, CXC, Yi-Chi Chang (National Tsing Hua University); Image Processing: Joseph DePasquale (STScI)

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Monika Luabeya

Hubble Captures a Tarantula

Hubble Captures a Tarantula

2 min read

Hubble Captures a Tarantula

A colorful nebula. The image’s top-left is filled with layers of fluffy pink and greenish clouds. Long strands of green clouds stretch out from here; a faint layer of translucent blue dust combines with them to create a three-dimensional scene. A sparse network of dark dust clouds in the foreground adds reddish-black patches atop the nebula. Blue-white and orange stars, from our galaxy and beyond, are spread throughout the clouds.
This NASA/ESA Hubble Space Telescope image shows a portion of the Tarantula Nebula.
ESA/Hubble & NASA, C. Murray

This NASA/ESA Hubble Space Telescope image captures incredible details in the dusty clouds of a star-forming factory called the Tarantula Nebula. Most of the nebulae Hubble images are in our galaxy, but this nebula is in the Large Magellanic Cloud, a dwarf galaxy located about 160,000 light-years away in the constellations Dorado and Mensa.

The Large Magellanic Cloud is the largest of the dozens of small satellite galaxies that orbit the Milky Way. The Tarantula Nebula is the largest and brightest star-forming region, not just in the Large Magellanic Cloud, but in the entire group of nearby galaxies to which the Milky Way belongs.

The Tarantula Nebula is home to the most massive stars known, some roughly 200 times as massive as our Sun. This image is very close to a rare type of star called a Wolf–Rayet star. Wolf–Rayet stars are massive stars that have lost their outer shell of hydrogen and are extremely hot and luminous, powering dense and furious stellar winds.

This nebula is a frequent target for Hubble, whose multiwavelength capabilities are critical for capturing sculptural details in the nebula’s dusty clouds. The data used to create this image come from an observing program called Scylla, named for a multi-headed sea monster from Greek mythology. The Scylla program was designed to complement another Hubble observing program called ULLYSES (Ultraviolet Legacy Library of Young Stars as Essential Standards). ULLYSES targets massive young stars in the Small and Large Magellanic Clouds, while Scylla investigates the structures of gas and dust that surround these stars.

Explore More:

Media Contact:

Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight CenterGreenbelt, MD

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NASA, SpaceX Stand Down on Crew-10 Undocking

NASA, SpaceX Stand Down on Crew-10 Undocking

From left, NASA's SpaceX Crew-10 members Kirill Peskov of Roscosmos, NASA astronauts Nichole Ayers and Anne McClain, and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi pose for a group portrait inside the International Space Station's Kibo laboratory module.
From left, NASA’s SpaceX Crew-10 members Kirill Peskov of Roscosmos, NASA astronauts Nichole Ayers and Anne McClain, and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi pose for a group portrait inside the International Space Station’s Kibo laboratory module.
NASA

NASA and SpaceX are standing down from the Thursday undocking opportunity of the Crew-10 mission from the International Space Station due to high winds forecasted for the splashdown locations off the coast of California. 

Pending weather reviews, NASA and SpaceX now are targeting undocking no earlier than 6:05 p.m. EDT, Friday, Aug. 8. For this undocking opportunity, splashdown is targeted at approximately 11:33 a.m., Saturday, Aug. 9, off the coast of California. 

NASA astronauts Anne McClain and Nichole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov are completing a five-month science expedition aboard the orbiting laboratory and will return time-sensitive research to Earth. 

Follow @space_station and @NASAKennedy on X for updates.

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Elyna Niles-Carnes

Linking Local Lithologies to a Larger Landscape

Linking Local Lithologies to a Larger Landscape

2 min read

Linking Local Lithologies to a Larger Landscape

A color photo from the Martian surface shows a landscape of sandy, rocky terrain. What looks like a pair of light orange-brown sand dunes rise in the background. Four or five large, sharp-edged rocks are strewn among the sand on the left side of the image. But a clear vertical dividing line extends from the center of the image to the right side, where the sand is covered by similar rocks of all sizes. A pale yellow sky is visible above the scene.
This image from NASA’s Mars Perseverance rover, taken by the Mastcam-Z instrument’s right eye, shows a collection of ridge-forming boulders. The rover acquired this image looking south along the ridge while exploring the “Westport” region of the outer crater rim on July 18, 2025 — Sol 1568, or Martian day 1,568 of the Mars 2020 mission — at the local mean solar time of 11:53:04.
NASA/JPL-Caltech/ASU

Written by Margaret Deahn, Ph.D. Student at Purdue University

NASA’s Mars 2020 rover is continuing to explore a boundary visible from orbit dividing bright, fractured outcrop from darker, smoother regolith (also known as a contact). The team has called this region “Westport,” (a fitting title, as the rover is exploring the western-most rim of Jezero), which hosts a contact between the smoother, clay-bearing “Krokodillen” unit and an outcrop of olivine-bearing boulders that converge to form a ridge on the outer Jezero crater rim. To learn more about the nature of this contact, see this blog post by Dr. Melissa Rice. Piecing together geologic events like the formation of this olivine-bearing material on Jezero’s crater rim may allow us to better understand Mars’ most ancient history. 

The rover has encountered several olivine-bearing rocks while traversing the rim, but it is unclear if, and how these rocks are all connected. Jezero crater is in a region of Mars known as Northeast Syrtis, which hosts the largest contiguous exposure (more than 113,000 square kilometers, or more than 43,600 square miles) of olivine-rich material identified from orbit on Mars (about the same square mileage as the state of Ohio!). The olivine-rich materials are typically found draping over older rocks, often infilling depressions, which may provide clues to their origins. Possible origins for the olivine-rich materials in Northeast Syrtis may include (but are not limited to): (1) intrusive igneous rocks (rocks that cool from magma underground), (2) melt formed and deposited during an impact event, or (3) pyroclastic ash fall or flow from a volcanic eruption. 

The Perseverance rover’s investigation of the olivine-bearing materials on the rim of Jezero crater may allow us to better constrain the history of the broader volcanic units present in the Northeast Syrtis region. Olivine-rich material in Northeast Syrtis is consistently sandwiched between older, clay-rich rock and younger, more olivine-poor material (commonly referred to as the “mafic capping” unit), and may act as an important marker for recording early alteration by water, which could help us understand early habitable environments on Mars. We see potential evidence of all of these units on Jezero crater’s rim based on orbital mapping. If the olivine-bearing rocks the Perseverance rover is encountering on the rim are related to these materials, we may be able to better constrain the age of this widespread geologic unit on Mars. 

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Last Updated
Aug 07, 2025

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