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New Perspective of Home
Seen during Artemis II’s lunar flyby on April 6, 2026, the Moon and Earth align in the same frame, each partially illuminated by the Sun. The Moon’s surface appears in sharp detail in the foreground, while Earth sits much farther away, smaller and softly lit in the background. A faint reflection in the spacecraft window is also visible, subtly overlaying the scene. Though their phases differ, both are shaped by the same sunlight, revealing the geometry of the Sun–Earth–Moon system from deep space.
NASA astronauts Reid Wiseman, Christina Koch, and Victor Glover, and CSA (Canadian Space Agency) astronaut Jeremy Hansen are set to return to Earth, splashing down in the Pacific Ocean around 8:07 p.m. EDT. Watch their return with NASA.
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Indoor Testing Facilities available at the NASA Unmanned Autonomy Research Complex (NUARC)
A large WindShaper fan array is available for dynamic low-speed and hovering flight research. The WindShaper is ideal for generating arbitrary wind gradients and wind gusts via a simple Python API. A companion WindProbe is also available for quick surveys of flows. The WindProbe utilizes the lab’s OptiTrack motion capture system to extract the position and orientation of the 5-hole cone probe located on the probe tip.
- Large dynamic fan array: 9’x7’, 1134 fans arranged as 567 ‘wind pixels’
- Wind speeds: 0 to 16 m/s (0 to 36 mph/31 kts)
- Acceleration: 4 m/s2, Deceleration: 2.5 m/s2
- Each fan is programmable via Python scripting
- Replicates steady winds, gusts, and wind gradients
I Am Artemis: Dan Florez
Listen to this audio excerpt from Dan Florez, test director for NASA’s Exploration Ground Systems Program:
0:00 / 0:00
Your browser does not support the audio element.At 1:47 a.m. EST November 16, 2022, as the Artemis I engines ignited, NASA astronaut Reid Wiseman and Dan Florez, NASA test director for the agency’s Exploration Ground Systems, watched from Kennedy’s Launch Control Center roof as the midnight sky turned bright as daylight, the crackle and roar of launch vibrating through them. Little did they know, one of them soon would be the Artemis II commander, and the other would be an important figure in bringing the mission home safely.
Florez is one of the NASA test directors for the Exploration Ground Systems Program. The test directors are a group of 20 engineers at the agency’s Kennedy Space Center in Florida who plan and execute integrated testing for Artemis missions. Their work includes developing timelines and procedures for launch countdown, propellant loading, emergency egress, pad and launch abort scenarios, recovery operations, and more. They help lead the ground systems team in all areas of testing.
Members of the Artemis launch team participate in an Artemis II launch countdown simulation inside Firing Room 1 in the Launch Control Center at NASA’s Kennedy Space Center in Florida on Thursday, May 8, 2025. NASA/Frank MichauxAt the time of Artemis I launch, Florez and his fellow test directors had already developed the launch countdown timelines for Artemis II.
“We were really focused on loading that spacecraft with cryogenic propellants and successfully launching it. With Artemis II, we’re going to have to do all that again, but in the middle of that, we’re going to have to embed the crew timeline to get the crew safely inside the spacecraft, get all the systems checked out, and launch them into space,” Florez said. “And we have to do the same thing on the tail end through recovery. So, there’s a lot of complexities when you have the human element thrown into the operation.”
Since Artemis I, Florez has focused his work even more heavily on the human element, taking on rescue and recovery operations.
A wave breaks inside the well deck of USS Somerset as teams work to recover the Crew Module Test Article (CMTA), a full scale replica of the Orion spacecraft, as they practice Artemis recovery operations during Underway Recovery Test-12 off the coast of California, Thursday, March 27, 2025. NASA/Joel Kowsky“We have to have a plan to go get to the crew if we have an abort, if we land anywhere in the world within 24 hours,” said Florez. “My role right now is to do a lot of that coordination to make sure we have all the assets and all the resources in place to get to the crew.”
When the Artemis II crew returns to Earth aboard the Orion spacecraft, Florez will be there, prepared and ready with NASA’s Landing and Recovery Team and the U.S. military.
We have a great partnership with the military. We have the Human Spaceflight Support Office within the Air Force that support us directly for not just for recovery operations, but also for any of the rescue operations.Dan Florez
NASA Test Director, Exploration Ground Systems Program
Recovery operations are routinely verified and validated in what is called an underway recovery test. NASA and Navy teams board a U.S. Navy ship and travel off the coast of San Diego to test retrieving the capsule and getting the crew safely on the ship. In late February 2024, the Artemis II crew joined the recovery team’s eleventh iteration of testing called, URT-11.
“It was really great to have that perspective of having astronauts in the loop during our test operations,” said Florez. “Everywhere along the way, we got feedback from them.”
Artemis II launched at 6:35 p.m. EDT April 1, from Launch Complex 39B, sending NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, on their approximately 10-day mission around the Moon.
Florez and his colleagues are prepared and ready to apply everything they tested to recover the crew.
Watching them launch is going to be great. I'm going to be happier when they land.Dan Florez
NASA Test Director, Exploration Ground Systems Program
About the AuthorAdeline Morgan RoeschStrategic Communications Specialist Share Details Last Updated Apr 10, 2026 Related Terms Explore More 1 min read Watching the Artemis II Mission Unfold at JPL’s Space Flight Operations FacilityDescription Staff at NASA’s Jet Propulsion Laboratory in Southern California watch the agency’s Artemis II…
Article 4 days ago 2 min read The Deep Space Network Acquires Artemis II SignalDescription A graphical representation of the Deep Space Network’s radio frequency antennas indicate signal acquisition…
Article 4 days ago 2 min read The Deep Space Network Acquires Artemis II SignalDescription The acquisition of the radio frequency signal from the Artemis II crewed mission to…
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Indoor Testing Facilities available at the NASA Unmanned Autonomy Research Complex (NUARC)
A large WindShaper fan array is available for dynamic low-speed and hovering flight research. The WindShaper is ideal for generating arbitrary wind gradients and wind gusts via a simple Python API. A companion WindProbe is also available for quick surveys of flows. The WindProbe utilizes the lab’s OptiTrack motion capture system to extract the position and orientation of the 5-hole cone probe located on the probe tip.
Windshaper fan array for dynamic low-speed and hovering flight research at NASA Ames Research Center.NASA/John Melton•Large dynamic fan array: 9’x7’, 1134 fans arranged as 567 ‘wind pixels’
•Wind speeds: 0 to 16 m/s (0 to 36 mph/31 kts)
•Acceleration: 4 m/s2, Deceleration: 2.5 m/s2
•Each fan is programmable via Python scripting
•Replicates steady winds, gusts, and wind gradients
WindProbe for handheld mobile wind data collection. WindShaperStarstruck
The Artemis II crew captured this photo of our galaxy, the Milky Way, on April 7, 2026. The Milky Way’s elegant spiral structure is dominated by just two arms wrapping off the ends of a central bar of stars. Spanning more than 100,000 light-years, Earth is located along one of the galaxy’s spiral arms, about halfway from the center.
See more photos from the mission.
Image credit: NASA
Watching the Artemis II Mission Unfold at JPL’s Space Flight Operations Facility
NASA/JPL-Caltech Photojournal Navigation Downloads Watching the Artemis II Mission Unfold at JPL’s Space Flight Operations Facility
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Staff at NASA’s Jet Propulsion Laboratory in Southern California watch the agency’s Artemis II mission unfold soon after launch on April 1, 2026, at the Space Flight Operations Facility, which operates the Deep Space Network (DSN).
The DSN comprises of three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex has several radio frequency antennas that communicate with dozens of spacecraft exploring the solar system in addition to the crewed Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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The Deep Space Network Acquires Artemis II Signal
NASA/JPL-Caltech Photojournal Navigation Downloads The Deep Space Network Acquires Artemis II Signal
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A graphical representation of the Deep Space Network’s radio frequency antennas indicate signal acquisition from NASA’s Artemis II mission to the Moon on April 1, 2026, inside the Space Flight Operations Facility at NASA’s Jet Propulsion Laboratory in Southern California. Two antennas at the Madrid Deep Space Communications Complex, Deep Space Station 54 and 56, can be seen communicating with Artemis II (the signals are labelled “EM2”, short for “Exploration Mission 2”; elsewhere they are labelled “ART2” for “Artemis II”).
A similar visualization can be found at DSN Now, which details all the missions that the network is communicating with 24 hours a day, seven days a week.
The Space Flight Operations Facility operates the DSN, which comprises of three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex consists of several radio frequency antennas that communicate with dozens of spacecraft exploring the solar system in addition to the Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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The Deep Space Network Acquires Artemis II Signal
NASA/JPL-Caltech Photojournal Navigation Downloads The Deep Space Network Acquires Artemis II Signal
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The acquisition of the radio frequency signal from the Artemis II crewed mission to the Moon by NASA’s Deep Space Network (DSN) is indicated by the peak in the data signal shown on the top computer screen.
Soon after the mission’s launch on April 1, 2026, at 6:35 p.m. EDT, NASA’s Near Space Network led communications with the Orion capsule. Then, communications were handed off to the DSN, marking the first time in over 50 years that the network would be communicating with a crewed spacecraft traveling through deep space.
The Space Flight Operations Facility at NASA’s Jet Propulsion Laboratory in Southern California (where this photo was taken) operates the DSN, which comprises three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex consists of several radio frequency antennas that communicate with dozens of robotic spacecraft exploring the solar system in addition to the Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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Watching Over the Deep Space Network Before Artemis II Signal Acquisition
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Blanca Renteria, Artemis Deep Space Network (DSN) operations chief, monitors data at the Space Flight Operations Facility at NASA’s Jet Propulsion Laboratory in Southern California shortly after Artemis II launched from the agency’s Kennedy Space Flight Center in Florida on April 1, 2026, at 6:35 p.m. EDT.
The Space Flight Operations Facility operates the DSN, which comprises three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex consists of several radio frequency antennas that communicate with dozens of robotic spacecraft exploring the solar system in addition to the crewed Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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Watching the Artemis II Launch From JPL’s Space Flight Operations Facility
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Staff at NASA’s Jet Propulsion Laboratory in Southern California watch the launch of the agency’s Artemis II mission to the Moon on April 1, 2026, at the Space Flight Operations Facility, which operates the Deep Space Network (DSN). Soon after launch, the Artemis II crew communicated with the Near Space Network while they were close to Earth. Later, communications were handed off to the DSN as the Orion capsule continued its journey into deep space.
The DSN comprises three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex has several radio frequency antennas that communicate with dozens of spacecraft exploring the solar system in addition to the Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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JPL’s ‘Lucky Peanuts’ Before Artemis II Launch
NASA/JPL-Caltech Photojournal Navigation Downloads JPL’s ‘Lucky Peanuts’ Before Artemis II Launch
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A container of “lucky peanuts” sits above workstations within the Space Flight Operations Facility at NASA’s Jet Propulsion Laboratory shortly before the launch of the Artemis II mission to the Moon on April 1, 2026. Eating peanuts before launches and other major mission events is a longstanding tradition at JPL.
The Space Flight Operations Facility operates the DSN, which comprises three complexes in Goldstone, California; Madrid, Spain; and Canberra, Australia. Each complex consists of several radio frequency antennas that communicate with dozens of spacecraft exploring the solar system in addition to the crewed Artemis II mission.
The DSN is managed by JPL for the agency’s Space Communications and Navigation program, which is located at NASA Headquarters within the Space Operations Mission Directorate. The DSN allows missions to track, send commands to, and receive scientific data from faraway spacecraft. JPL is managed by Caltech in Pasadena, California, for NASA.
For more information about Artemis II, visit: https://www.nasa.gov/mission/artemis-ii/
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Snow in the Shadow of the Andes
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Twin NASA Control Rooms Support Artemis Safety, Success
Twin control rooms at NASA’s Marshall Space Flight Center in Huntsville, Alabama, are actively supporting real-time mission operations in lunar orbit as part of the agency’s Artemis II mission, helping ensure astronaut safety and mission success as the crew prepares to return to Earth Friday, April 10.
The LUCA (Lunar Utilization Control Area) and LESA (Lander Engineering Support Area) rooms are part of the Huntsville Operations Support Center at NASA Marshall. While the spaces look nearly identical, the two are more like fraternal twins in their focus areas: LUCA primarily supports Artemis science operations, while LESA will provide engineering support for landing astronauts on the Moon.
LUCA (Lunar Utilization Control Area) at NASA Marshall is specially designed to support a wide variety of science operations on and around the Moon – and beyond. Engineers in the LUCA monitored operations for the Lunar Node-1 experiment, an autonomous navigation payload that was part of the first NASA Commercial Lunar Payload Services (CLPS) launch on Intuitive Machines’ Nova-C lunar lander in 2024. NASA Marshall flight controllers will use the LUCA again for Artemis II to monitor science operations.NASA/Charles Beason“The Huntsville Operations Support Center at NASA Marshall can be adapted to the needs of the agency’s missions, and LUCA and LESA are some of our newest configurable control rooms for the Artemis campaign,” said Harish Chandranath, Payload and Mission Operations Division Human Landing Systems project lead at Marshall. “In addition to supporting Artemis, our Huntsville Operations Support Center teams also support the Commercial Crew Program, the SLS (Space Launch System) rocket, and International Space Station science operations.”
Support center services include work to manage spacecraft command and telemetry, local and remote voice services for international connections, live and recorded video services, and a telescience resource kit – special software that makes sure two computers far apart can communicate without missing any information and without human help. All Huntsville Operations Support Center services can be tied into both the LUCA and LESA rooms, giving operators the capability to use data and communicate with scientists and experts around the world.
Support engineers will use the LESA (Lander Engineering Support Area) at NASA Marshall to monitor human landing system (HLS) for the first crewed Artemis missions.NASA/Charles BeasonDuring Artemis II, teams in LUCA are supporting first-of-their-kind science operations designed to better understand the effects of deep space – such as microgravity and radiation – on crew physiology, immune response, and performance. The data gathered during the mission will inform future crewed flights to the Moon.
Meanwhile, teams in LESA are observing Artemis II mission operations in real time, which is a critical opportunity to refine processes and prepare for future crewed landings on the Moon’s surface. For Artemis missions, members of NASA’s Human Landing System Mission Insight Support Team – including engineers, safety leads, flight operations experts, and technical authorities – will operate from LESA to monitor lander systems and support key decision-making.
Through the Artemis program, NASA is returning humans to the Moon for scientific discovery, economic opportunity, and to build the foundation for the first crewed missions to Mars – for the benefit of all.
To learn more about the Artemis program, visit:
Share Details Last Updated Apr 08, 2026 EditorLee MohonContactCorinne M. Beckingercorinne.m.beckinger@nasa.gov Related Terms Keep Exploring Discover More Topics From NASAArtemis II
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Solar Eclipse of the Heart
The Moon, seen here backlit by the Sun during a solar eclipse on April 6, 2026, is photographed by one of the cameras on the Orion spacecraft’s solar array wings. During lunar flyby, the Artemis II astronauts observed a solar eclipse that only they could see due to their unique position.
See more photos from the Artemis II mission.
Image credit: NASA
A Volcanic Medley Near Mammoth Lakes
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Celestial Wonders in Leo
NASA, ESA and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration; Acknowledgment: Davide De Martin and Robert Gendler
Leo is a prominent sight for stargazers in April. Its famous sickle, punctuated by the bright star Regulus, draws many a beginning stargazer’s eyes, inviting deeper looks into some of Leo’s celestial delights, including a great double star and a famous galactic trio.
The constellation, Leo. You can find this constellation in the springtime skies. StellariumLeo’s distinctive forward sickle, or “reverse question mark,” is easy to spot as it climbs the skies in the southeast after sunset. If you are having a difficult time spotting the sickle, look for bright Sirius and Procyon in Canis Major and Canis Minor. Complete a triangle by drawing two lines to the east, joining at the bright star Regulus, the “period” in the reverse question mark. Trailing them is a trio of bright stars forming an isosceles triangle, the brightest star in that formation named Denebola. Connecting these two patterns together forms the constellation of Leo the Lion, with the forward-facing sickle being the lion’s head and mane, and the rear triangle its hindquarters. Can you see this mighty feline? It might help to imagine Leo proudly sitting up and staring straight ahead, like a celestial Sphinx. To help find these objects, you can use online tools like Stellarium Web.
If you peer deeper into Leo with a small telescope or binoculars, you’ll find a notable double star! Look in the sickle of Leo for its second-brightest star, Algieba, also called Gamma Leonis. This star splits into two bright yellow stars even with a small magnification. You can make this “split” with binoculars, but it’s more apparent with a telescope. Compare the color and intensity of these two stars: do you notice any differences? There are other multiple-star systems in Leo; spend a few minutes scanning with your instrument of choice, and see what you discover.
The Leo Triplet – three galaxies that appear to be close together under the star Chertan in the Leo constellation. StellariumOne of the most famous sights in Leo is the “Leo Triplet”: three galaxies that appear to be close together. They are indeed gravitationally bound to one another, around 30 million light-years away! You’ll need a telescope to spot them, and use an eyepiece with a wide field of view to see all three galaxies at once! Look below the star Chertan to find galaxies M65, M66, and NGC 3628 – The Hamburger Galaxy. Compare and contrast the appearance of each galaxy – while they are all spiral galaxies, each one is tilted at different angles to our point of view! Do they all look like spiral galaxies to you?
April is Citizen Science Month, and there are some fun Leo-related activities you can participate in! If you enjoy
comparing the Triplets, the Galaxy Zoo project could use your eyes to help classify different galaxies from sky survey data! Looking at Leo itself can even help measure light pollution: the Globe at Night project uses Leo as their target constellation for sky quality observations from the Northern Hemisphere. Find and participate in many more NASA community science programs at NASA Citizen Science. Happy observing!
Originally posted by Dave Prosper: April 2021
Last Updated by Kat Troche: April 2026
NASA’s Artemis II Crew Beams Official Moon Flyby Photos to Earth
Editor’s note: Some photo captions were updated on April 8, 2026, to reflect ongoing scientific observations and discussion about the images.
The first flyby images of the Moon captured by NASA’s Artemis II astronauts during their historic test flight reveal some regions no human has seen, including a rare in-space solar eclipse. Released Tuesday, astronauts captured the images April 6 during the mission’s seven-hour flyby of the lunar far side, showing humanity’s return to the Moon’s vicinity and opening a trove of scientific data.
NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, have used a fleet of cameras to take thousands of photos. The agency released several images, with more expected in the coming days as the crew members are more than halfway through their journey and now headed home toward Earth.
“Our four Artemis II astronauts — Reid, Victor, Christina, and Jeremy — took humanity on an incredible journey around the Moon and brought back images so exquisite and brimming with science, they will inspire generations to come,” said Dr. Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington.
During the lunar flyby, the crew documented impact craters, ancient lava flows, and surface fractures that will help scientists study the Moon’s geologic evolution. They monitored color, brightness, and texture differences across the terrain, observed an earthset and earthrise, and captured solar‑eclipse views of the Sun’s corona. The crew also reported six meteoroid impact flashes on the darkened lunar surface.
Peeking at EarthAs NASA’s Artemis II crew came close to passing behind the Moon and experiencing a planned loss of signal on Monday, April 6, 2026, they captured this image of a crescent Earth setting on the Moon’s limb. In this photo, the dark portion of Earth is experiencing nighttime, while Australia and Oceania are in the daylight. In the foreground, the Ohm crater is visible, with terraced edges and a flat floor interrupted by central peaks. Peaks such as these form in complex craters when the lunar surface is liquified on impact, and the liquefied surface splashes upward during the crater’s formation.Credit: NASA Setting EarthThe lunar surface fills the frame in sharp detail, as seen during NASA’s Artemis II lunar flyby, while a distant Earth sets in the background. This image was captured at 6:41 p.m. EDT, on April 6, 2026, just three minutes before the Orion spacecraft and its crew went behind the Moon and lost contact with Earth for 40 minutes before emerging on the other side. In this image, the dark portion of Earth is experiencing nighttime, while on its day side, swirling clouds are visible over the Australia and Oceania region. In the foreground, Ohm crater shows terraced edges and a relatively flat floor marked by central peaks — formed when the surface rebounded upward during the impact that created the crater.Credit: NASA Shadows Across Vavilov CraterA close-up view taken by the Artemis II crew of Vavilov Crater on the rim of the older and larger Hertzsprung basin on Monday, April 6, 2026. The right portion of the image shows the transition from smooth material within an inner ring of mountains to more rugged terrain around the rim. Vavilov and other craters and their ejecta are accentuated by long shadows at the terminator, the boundary between lunar day and night. The image was captured with a handheld camera at a focal length of 400 mm, as the crew flew around the far side of the Moon.Credit: NASA Artemis Era EarthriseEarthrise captured through the Orion spacecraft window at 7:22 p.m. EDT on Monday, April 6, 2026, during the Artemis II crew’s flyby of the Moon’s far side. Earth appears as a delicate crescent, with only its upper edge illuminated. The planet’s soft blue hue and scattered white cloud systems stand out against the blackness of space, while the lower portion fades into night. Taken with a 400 mm lens, the image, Earthrise, reveals a striking alignment of Earth and Moon, with the Moon in the top foreground and the Earth below. Along the lunar horizon, rugged terrain is silhouetted against the bright crescent Earth. Both bodies are oriented with their north poles to the left and south poles to the right, offering a unique perspective of our home planet from deep space. This photo was rotated 90 degrees clockwise for standard viewing orientation. Credit: NASA Artemis II in EclipseCaptured by the Artemis II crew during their lunar flyby on Monday, April 6, 2026, this image shows the Moon fully eclipsing the Sun. From the crew’s perspective, the Moon appears large enough to completely block the Sun, creating nearly 54 minutes of totality and extending the view far beyond what is possible from Earth. We see a glowing halo around the dark lunar disk. The science community is investigating whether this effect is due to the corona, zodiacal light, or a combination of the two. Also visible are stars, typically too faint to see when imaging the Moon, but with the Moon in darkness stars are readily imaged. This unique vantage point provides both a striking visual and a valuable opportunity for astronauts to document their observations during humanity’s return to deep space. The faint glow of the nearside of the Moon is visible in this image, having been illuminated by light reflected off the Earth.Credit: NASA Artemis II Total Solar Eclipse, Partial FrameA close-up view from the Orion spacecraft during the Artemis II crew’s lunar flyby on Monday, April 6, 2026, captures a total solar eclipse, with only part of the Moon visible in the frame as it fully obscures the Sun. We see a glowing halo around the dark lunar disk. The science community is investigating whether this effect is due to the corona, zodiacal light, or a combination of the two. From this deep-space vantage point, the Moon appeared large enough to sustain nearly 54 minutes of totality, far longer than total solar eclipses typically seen from Earth. The bright silver glint on the left edge of the image is the planet Venus. The round, dark gray feature visible along the Moon’s horizon between the 9 and 10 o’clock positions is Mare Crisium, a feature visible from Earth. We see faint lunar features because light reflected off of Earth provides a source of illumination.Credit: NASA EarthsetEarthset captured through the Orion spacecraft window at 6:41 p.m. EDT, April 6, 2026, during the Artemis II crew’s flyby of the Moon. A muted blue Earth with bright white clouds sets behind the cratered lunar surface. The dark portion of Earth is experiencing nighttime. On Earth’s day side, swirling clouds are visible over the Australia and Oceania region. In the foreground, Ohm crater has terraced edges and a flat floor interrupted by central peaks. Central peaks form in complex craters when the lunar surface, liquefied on impact, splashes upwards during the crater’s formation.Credit: NASA Final Flyby PreparationsNASA astronauts Victor Glover and Reid Wiseman, and CSA (Canadian Space Agency) astronaut Jeremy Hansen prepare for their journey around the far side of the Moon by configuring their camera equipment shortly before beginning the Artemis II lunar flyby observations.Credit: NASA Ready for Close UpCaptured by the Artemis II crew, the heavily cratered terrain of the eastern edge of the South Pole-Aitken basin is seen with the shadowed terminator – the boundary between lunar day and night – at the top of the image. The South Pole-Aitken basin is the largest and oldest basin on the Moon, providing a glimpse into an ancient geologic history built up over billions of years.Credit: NASAScientists already are analyzing the downlinked images, audio, and data to refine the timing and locations of these events and compare them with observations from amateur astronomers. The new imagery also will help NASA better understand the Moon’s geology and inform future exploration and science missions that will lay the foundation for an enduring presence on the Moon ahead of future astronaut missions to Mars.
“It was remarkable listening to the crew describe the stunning views during the flyby,” said Jacob Bleacher, NASA’s chief exploration scientist at the agency’s headquarters. “At first, their descriptions didn’t quite match what we were seeing on our screens. Now that higher resolution images are coming down, we can finally experience the moments they were trying to share and truly appreciate the scientific return provided by these images and our other research on this mission.”
Official NASA imagery for viewing and download is available on the agency website and digital platforms, including:
Media should follow NASA’s media usage guidelines for all publication and distribution of these images.
NASA is targeting 8:07 p.m. EDT (5:07 p.m. PDT) Friday, April 10, for the return of Artemis II off the coast of San Diego. NASA+ live return coverage begins at 6:30 p.m. and will continue until NASA and Department of War personnel safely assist the crew out of Orion and transport them to the USS John P. Murtha.
Briefings, events, and 24/7 mission coverage are streaming on NASA’s YouTube channel and events will each have their own stream closer to their start time. Learn how to watch NASA content through a variety of online platforms, including social media.
As part of Golden Age of innovation and exploration, NASA will send Artemis astronauts on increasingly difficult missions to explore more of the Moon for scientific discovery, economic benefits, and to build on our foundation for the first crewed missions to Mars.
To learn more about the Artemis program, visit:
-end-
Cheryl Warner / Katherine Rohloff
Headquarters, Washington
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cheryl.m.warner@nasa.gov / katherine.a.rohloff@nasa.gov
Earthset
The Artemis II crew captured this view of Earth setting on April 6, 2026, as they flew around the Moon. As the astronauts flew over the Moon’s far side, the crew photographed and described terrain features including impact craters, ancient lava flows, and surface cracks and ridges formed as the Moon slowly evolved over time. They also noted differences in color, brightness and texture, which provide clues that help scientists understand the composition and history of the lunar surface.
The image is reminiscent of the iconic Earthrise image taken by astronaut Bill Anders 58 years earlier as the Apollo 8 crew flew around the Moon. The Apollo 8 mission was the first crewed spacecraft to circumnavigate the Moon.
For more imagery from the mission, visit our Artemis II Multimedia Page.
Image credit: NASA
Experience the Rollout of SLS Hardware for Artemis III
Digital creators and social media users are invited to register to attend the rollout of the third SLS (Space Launch System) core stage as it is prepped to head from NASA’s Michoud Assembly Facility to NASA’s Kennedy Space Center.
Are you passionate about social media and communications? Do you love to create content for an audience? Are you a fan of new, unique experiences? If you said yes, this NASA Social event is for you! This is your opportunity to be on the front lines as NASA continues to lay the groundwork for future deep space exploration.
The NASA Social event will be a one-day event as soon as mid to late April pending the launch of Artemis II. A maximum of 20 digital creators will be selected to attend this event and will be given access similar to news media.
NASA Social participants will have the opportunity to:
- Tour NASA’s Michoud Assembly Facility
- Learn directly from subject matter experts
- Meet fellow digital creators and social media users
- Spend time with members of NASA’s social media team
- View the rollout of the SLS core stage for Artemis III
NASA Social registration for the hardware rollout opens on this page on Tuesday, April 7, and the deadline to apply is noon EDT on Friday, April 10. All applications will be considered on a case-by-case basis.
Do I need to have a social media account to register?
Yes. This event is designed for people who:
- Actively use multiple social networking platforms and tools to disseminate information to a unique audience.
- Regularly produce new content that features multimedia elements.
- Have the potential to reach a large number of people using digital platforms.
- Reach a unique audience, separate and distinctive from traditional news media and/or NASA audiences.
- Must have an established history of posting content on social media platforms.
- Have previous postings that are highly visible, respected, and widely recognized.
Users are encouraged to follow @NASAArtemis for Artemis updates on X, Facebook, and Instagram. Updates and information about the event will be shared on X via @NASA_Events.
How do I register?
Registration for this event opens April 7 and closes at noon EDT on April 10. Registration is for one person only (you) and is non-transferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis.
Can I register if I am not a U.S. citizen?
No, this event is open to only U.S citizens
When will I know if I am selected?
After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the first notifications on Monday, April 13.
What are NASA Social credentials?
All NASA social applications will be considered on a case-by-case basis. Those chosen must prove through the registration process they meet specific engagement criteria.
What are the registration requirements?
Registration indicates your intent to travel to NASA Michoud and attend the one-day event in person. You are responsible for your own expenses for travel, accommodation, food, and other amenities.
The schedule of events and special guest appearances are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is canceled with limited or no notice. Please plan accordingly.
Michoud is a government facility. Those who are selected may need to complete additional steps to receive clearance to enter the secure areas.
IMPORTANT: Those without proper identification cannot be admitted.
For United States Citizens:
You will be required to present a REAL ID compliant identification or valid U.S. passport PLUS one of the following:
Acceptable documents to accompany federal or state identification:
- U.S. Passport
- Unexpired Employment Authorization Card (Form I-688A)
- Unexpired Employment Authorization Document issued by DHS that contains a photograph (Form I-688B)
- Driver’s license or ID card issued by a state or outlying possession of the United States provided it contains a photograph or information such as name, date of birth, gender, height, eye color, and address
- ID card issued by federal, state or local government agencies or entities, provided it contains a photograph or information such as name, date of birth, gender, height, eye color and address
- School ID card with a photograph
- Voter’s Registration Card
- Military Dependent’s ID Card
- U.S. Military card or draft record
- U.S. Coast Guard Merchant Mariner Card
- Native American Tribal Document
- U.S. Social Security Card issued by the Social Security Administration (other than a card stating it is not valid for employment)
- Original or Certified copy of birth certificate issued by a state, county, municipal authority or outlying possessions of the United States bearing an official seal
- U.S. Citizen ID Card (Form I-197)
- ID Card for use of Resident Citizens of the United States (Form I-179)
- Unexpired employment authorization document issued by DHS (other than those listed previously)
For Legal Resident Aliens:
- Same items required of U. S. Citizens, and:
- Permanent Resident Card or Alien Registration Receipt Card with photograph (Form I-551)
- Unexpired Temporary Resident Card (Form I-688)
- Certification of Birth Abroad issued by the Department of State (Form FS-545 or Form DS-1350)
The REAL ID Act was passed by Congress in 2005 to establish minimum security standards for state-issued driver’s licenses and identification cards.
All registrants must be at least 18 years old.
What if the rollout date changes?
Many different factors can cause a scheduled date change. NASA may adjust the date of the NASA Social accordingly to coincide with a new target rollout date, and will notify registrants of any changes via email.
If the event is postponed, attendees will be invited to attend at a later date. If the rollout is postponed beyond 72 hours, the NASA Social event may be canceled.
NASA Social attendees are responsible for any additional costs they incur related to any launch delay. We strongly encourage participants to make travel arrangements that are refundable and/or flexible.
What if I cannot come to Michoud Assembly Facility?
If you cannot come to NASA Michoud and attend in person, you should not register for the NASA Social. Join the conversation by following @NASAArtemis on X, Facebook, and Instagram,
If you cannot make this NASA Social, don’t worry; NASA is planning many other NASA Social events in the near future at various locations! Check for updates on NASA Socials.
