NASA Progresses Toward Crewed Moon Mission with Spacecraft, Rocket Milestones

NASA Progresses Toward Crewed Moon Mission with Spacecraft, Rocket Milestones

Technicians move the Orion spacecraft for NASA’s Artemis II test flight out of the Neil A. Armstrong Operations and Checkout Building to the Multi-Payload Processing Facility at Kennedy Space Center in Florida on Saturday, May 3, 2025.
NASA/Kim Shiflett

Engineers, technicians, mission planners, and the four astronauts set to fly around the Moon next year on Artemis II, NASA’s first crewed Artemis mission, are rapidly progressing toward launch.

At the agency’s Kennedy Space Center in Florida, teams are working around the clock to move into integration and final testing of all SLS (Space Launch System) and Orion spacecraft elements. Recently they completed two key milestones – connecting the SLS upper stage with the rest of the assembled rocket and moving Orion from its assembly facility to be fueled for flight.

“We’re extremely focused on preparing for Artemis II, and the mission is nearly here,” said Lakiesha Hawkins, assistant deputy associate administrator for NASA’s Moon to Mars Program, who also will chair the mission management team during Artemis II. “This crewed test flight, which will send four humans around the Moon, will inform our future missions to the Moon and Mars.”

Teams with NASA’s Exploration Ground Systems Program begin integrating the interim cryogenic propulsion stage to the SLS (Space Launch System) launch vehicle stage adapter on Wednesday, April 30, 2025, inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida.
NASA/Isaac Watson

On May 1, technicians successfully attached the interim cryogenic propulsion stage to the SLS rocket elements already poised atop mobile launcher 1, including its twin solid rocket boosters and core stage, inside the spaceport’s Vehicle Assembly Building (VAB). This portion of the rocket produces 24,750 pounds of thrust for Orion after the rest of the rocket has completed its job. Teams soon will move into a series of integrated tests to ensure all the rocket’s elements are communicating with each other and the Launch Control Center as expected. The tests include verifying interfaces and ensuring SLS systems work properly with the ground systems.

Meanwhile, on May 3, Orion left its metaphorical nest, the Neil Armstrong Operations & Checkout Facility at Kennedy, where it was assembled and underwent initial testing. There the crew module was outfitted with thousands of parts including critical life support systems for flight and integrated with the service module and crew module adapter. Its next stop on the road to the launch pad is the Multi-Payload Processing Facility, where it will be carefully fueled with propellants, high pressure gases, coolant, and other fluids the spacecraft and its crew need to maneuver in space and carry out the mission.

After fueling is complete, the four astronauts flying on the mission around the Moon and back over the course of approximately 10 days, will board the spacecraft in their Orion Crew Survival System spacesuits to test all the equipment interfaces they will need to operate during the mission. This will mark the first time NASA’s Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, will board their actual spacecraft while wearing their spacesuits. After the crewed testing is complete, technicians will move Orion to Kennedy’s Launch Abort System Facility, where the critical escape system will be added. From there, Orion will move to the VAB to be integrated with the fully assembled rocket.

NASA also announced its second agreement with an international space agency to fly a CubeSat on the mission. The collaborations provide opportunities for other countries to work alongside NASA to integrate and fly technology and experiments as part of the agency’s Artemis campaign.

While engineers at Kennedy integrate and test hardware with their eyes on final preparations for the mission, teams responsible for launching and flying the mission have been busy preparing for a variety of scenarios they could face.

The launch team at Kennedy has completed more than 30 simulations across cryogenic propellant loading and terminal countdown scenarios. The crew has been taking part in simulations for mission scenarios, including with teams in mission control. In April, the crew and the flight control team at NASA’s Johnson Space Center in Houston simulated liftoff through a planned manual piloting test together for the first time. The crew also recently conducted long-duration fit checks for their spacesuits and seats, practicing several operations while under various suit pressures.

NASA astronaut Christina Koch participates in a fit check April 18, 2025, in the spacesuit she will wear during Artemis II.
NASA/Josh Valcarcel

Teams are heading into a busy summer of mission preparations. While hardware checkouts and integration continue, in coming months the crew, flight controllers, and launch controllers will begin practicing their roles in the mission together as part of integrated simulations. In May, the crew will begin participating pre-launch operations and training for emergency scenarios during launch operations at Kennedy and observe a simulation by the launch control team of the terminal countdown portion of launch. In June, recovery teams will rehearse procedures they would use in the case of a pad or ascent abort off the coast of Florida, with launch and flight control teams supporting. The mission management team, responsible for reviewing mission status and risk assessments for issues that arise and making decisions about them, also will begin practicing their roles in simulations. Later this summer, the Orion stage adapter will arrive at the VAB from NASA’s Marshall Spaceflight Center in Huntsville, Alabama, and stacked on top of the rocket.

NASA astronauts Reid Wiseman (foreground) and Victor Glover participate in a simulation of their Artemis II entry profile on March 13, 2025.
NASA/Bill Stafford

Through Artemis, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and build the foundation for the first crewed missions to Mars.

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Rachel H. Kraft

SPHEREx Starts Scanning Entire Sky

SPHEREx Starts Scanning Entire Sky

Infrared image showing a field of copper stars with a distinct smoke-like cloud at the center.
NASA/JPL-Caltech

A soot-like cloud is revealed in a section of the sky in this May 1, 2025, image from NASA’S SPHEREx space observatory. On May 1, SPHEREx began regular science operations, which consist of taking about 3,600 images per day for the next two years to provide new insights about the origins of the universe, galaxies, and the ingredients for life in the Milky Way. The observatory won’t be the first to map the entire sky, but it will be the first to do so in so many colors. It observes 102 wavelengths, or colors, of infrared light, which are undetectable to the human eye.

When SPHEREx takes a picture of the sky, the light is sent to six detectors that each produces a unique image capturing different wavelengths of light. These groups of six images are called an exposure, and SPHEREx takes about 600 exposures per day. When it’s done with one exposure, the whole observatory shifts position — the mirrors and detectors don’t move as they do on some other telescopes.

Read more about SPHEREx and the images it will capture.

Image credit: NASA/JPL-Caltech

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Monika Luabeya

NASA’s NICER Maps Debris From Recurring Cosmic Crashes

NASA’s NICER Maps Debris From Recurring Cosmic Crashes

5 min read

NASA’s NICER Maps Debris From Recurring Cosmic Crashes

Lee esta nota de prensa en español aquí.

For the first time, astronomers have probed the physical environment of repeating X-ray outbursts near monster black holes thanks to data from NASA’s NICER (Neutron star Interior Composition Explorer) and other missions.

Scientists have only recently encountered this class of X-ray flares, called QPEs, or quasi-periodic eruptions. A system astronomers have nicknamed Ansky is the eighth QPE source discovered, and it produces the most energetic outbursts seen to date. Ansky also sets records in terms of timing and duration, with eruptions every 4.5 days or so that last approximately 1.5 days.

“These QPEs are mysterious and intensely interesting phenomena,” said Joheen Chakraborty, a graduate student at the Massachusetts Institute of Technology in Cambridge. “One of the most intriguing aspects is their quasi-periodic nature. We’re still developing the methodologies and frameworks we need to understand what causes QPEs, and Ansky’s unusual properties are helping us improve those tools.”

Watch how astronomers used data from NASA’s NICER (Neutron star Interior Composition Explorer) to study a mysterious cosmic phenomenon called a quasi-periodic eruption, or QPE.
NASA’s Goddard Space Flight Center

Ansky’s name comes from ZTF19acnskyy, the moniker of a visible-light outburst seen in 2019. It was located in a galaxy about 300 million light-years away in the constellation Virgo. This event was the first indication that something unusual might be happening.

A paper about Ansky, led by Chakraborty, was published Tuesday in The Astrophysical Journal.

A leading theory suggests that QPEs occur in systems where a relatively low-mass object passes through the disk of gas surrounding a supermassive black hole that holds hundreds of thousands to billions of times the Sun’s mass.

When the lower-mass object punches through the disk, its passage drives out expanding clouds of hot gas that we observe as QPEs in X-rays.

Scientists think the eruptions’ quasi-periodicity occurs because the smaller object’s orbit is not perfectly circular and spirals toward the black hole over time. Also, the extreme gravity close to the black hole warps the fabric of space-time, altering the object’s orbits so they don’t close on themselves with each cycle. Scientists’ current understanding suggests the eruptions repeat until the disk disappears or the orbiting object disintegrates, which may take up to a few years.

A snapshot of an all-sky survey.
A system astronomers call Ansky, in the galaxy at the center of this image, is home to a recently discovered series of quasi-periodic eruptions.
Sloan Digital Sky Survey

“Ansky’s extreme properties may be due to the nature of the disk around its supermassive black hole,” said Lorena Hernández-García, an astrophysicist at the Millennium Nucleus on Transversal Research and Technology to Explore Supermassive Black Holes, the Millennium Institute of Astrophysics, and University of Valparaíso in Chile. “In most QPE systems the supermassive black hole likely shreds a passing star, creating a small disk very close to itself. In Ansky’s case, we think the disk is much larger and can involve objects farther away, creating the longer timescales we observe.”

Hernández-García, in addition to being a co-author on Chakraborty’s paper, led the study that discovered Ansky’s QPEs, which was published in April in Nature Astronomy and used data from NICER, NASA’s Neil Gehrels Swift Observatory and Chandra X-ray Observatory, as well as ESA’s (European Space Agency’s) XMM-Newton space telescope.

NICER’s position on the International Space Station allowed it to observe Ansky about 16 times every day from May to July 2024. The frequency of the observations was critical in detecting the X-ray fluctuations that revealed Ansky produces QPEs.

Chakraborty’s team used data from NICER and XMM-Newton to map the rapid evolution of the ejected material driving the observed QPEs in unprecedented detail by studying variations in X-ray intensity during the rise and fall of each eruption.

The researchers found that each impact resulted in about a Jupiter’s worth of mass reaching expansion velocities around 15% of the speed of light.

An astronaut takes a selfie with a telescope
The NICER (Neutron star Interior Composition Explorer) X-ray telescope is reflected on NASA astronaut and Expedition 72 flight engineer Nick Hague’s spacesuit helmet visor in this high-flying “space-selfie” taken during a spacewalk on Jan. 16, 2025.
NASA/Nick Hague

The NICER telescope’s ability to frequently observe Ansky from the space station and its unique measurement capabilities also made it possible for the team to measure the size and temperature of the roughly spherical bubble of debris as it expanded.

“All NICER’s Ansky observations used in these papers were collected after the instrument experienced a ‘light leak’ in May 2023,” said Zaven Arzoumanian, the mission’s science lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Even though the leak – which was patched in January – affected the telescope’s observing strategy, NICER was still able to make vital contributions to time domain astronomy, or the study of changes in the cosmos on timescales we can see.”

After the repair, NICER continued observing Ansky to explore how the outbursts have evolved over time. A paper about these results, led by Hernández-García and co-authored by Chakraborty, is under review.

Observational studies of QPEs like Chakraborty’s will also play a key role in preparing the science community for a new era of multimessenger astronomy, which combines measurements using light, elementary particles, and space-time ripples called gravitational waves to better understand objects and events in the universe.

One goal of ESA’s future LISA (Laser Interferometer Space Antenna) mission, in which NASA is a partner, is to study extreme mass-ratio inspirals — or systems where a low-mass object orbits a much more massive one, like Ansky. These systems should emit gravitational waves that are not observable with current facilities. Electromagnetic studies of QPEs will help improve models of those systems ahead of LISA’s anticipated launch in the mid-2030s.

“We’re going to keep observing Ansky for as long as we can,” Chakraborty said. “We’re still in the infancy of understanding QPEs. It’s such an exciting time because there’s so much to learn.”

By Jeanette Kazmierczak
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Media Contact:
Claire Andreoli
301-286-1940
claire.andreoli@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Sols 4529-4531: Honeycombs and Waffles… on Mars!

Sols 4529-4531: Honeycombs and Waffles… on Mars!

4 min read

Sols 4529-4531: Honeycombs and Waffles… on Mars!

An extreme wide-angle photo of the Martian surface in front of the Curiosity rover shows extremely rocky, rough terrain, with flat rocks in the foreground showing apparent honeycomb-shaped patterns on their exposed faces, and a larger rock at the center of the image, looking like an offset stack of waffles. Portions of the rover are visible in each corner of the frame, with two wheels visible, but shadowed, in the lower left and right corners.
NASA’s Mars rover Curiosity captured this image of its current workspace, containing well-preserved polygonal shaped fractures, with waffle or honeycomb patterns. The rover acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on May 1, 2025 — Sol 4527, or Martian day 4,527 of the Mars Science Laboratory mission — at 16:41:35 UTC.
NASA/JPL-Caltech

Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick

Earth planning date: Friday, May 2, 2025

From our Wednesday stopping spot, the drive direction ahead (looking along the path we would follow in the Wednesday drive) appeared to be full of rough, gnarly material, which can be tricky targets for contact science instruments like APXS. However, coming into planning this morning, we found a workspace with amazingly well preserved polygonal shaped fractures, with raised ridges (about 1 centimeter, or about 0.39 inches, high), looking like a patchwork of honeycombs, or maybe a patch of waffles. We have spotted these before but usually not as well preserved and extensive as this — we can see these stretching away into the distance for 20-30 meters (about 66-98 feet), almost to the edge of the “boxwork” fracture structures at “Ghost Mountain” butte in this Navcam image. We are all counting down the drives to get to the boxwork structures — this will be such an exciting campaign to be part of.

As APXS operations planner today, I was really interested to see if we could get APXS close to one of the raised ridges, to determine what they are made of. The Rover Planners were able to get a paired set of targets — “Orosco Ridge” along a ridge and “Box Canyon” in the adjacent, flat center of the polygon. The ChemCam team is also interested (in truth, everyone on the team is interested!!) in the composition of the ridges. So ChemCam will use LIBS to measure both bedrock and ridge fill at “Kitchen Creek” on the first sol of the plan and “Storm Canyon” on the second sol.  

The “problem” with a workspace like this is picking which images to take in our short time here, before we drive on the second sol. We could stay here for a week and still find things to look at in this workspace. After much discussion, it was decided that MAHLI should focus on a “dog’s eye” mosaic (“Valley of the Moon”) along the vertical face of the large block. We hope this will allow us to examine how the fractures interact with each other, and with the preexisting layering in the bedrock.  

Mastcam will then focus on the two main blocks in the workspace in an 8×4 (4 rows of 8 images) Kitchen Creek mosaic, which also encompasses the LIBS target of the same name, and a single image on the Storm Canyon LIBS target. Three smaller mosaics at “Green Valley Falls” (3×1), “Lost Palms Canyon” (7×2) and “San Andreas Fault” (1×2) will examine the relationships between the polygonal features and other fractures in the workspace, close to the rover. 

Further afield, ChemCam will turn the “LD RMI” (Long-Distance Remote Micro Imager) on “Texoli” butte (the large butte to the side of the rover, visible in this image from sol 4528). Both Mastcam and ChemCam will image the boxwork fracture system near Ghost Mountain — they are so close now, it’s just a few drives away! Any information we get now may be able to help us answer some of the questions we have on the origin and timing of the boxwork structures, especially when we can combine it with the in situ analysis we will be getting shortly! (Did I mention how excited we all are about this campaign?)With all the excitement today on the wild fracture structures, it could be easy to overlook Curiosity’s dataset of environmental and atmospheric data. For more than 12 years now, we have been collecting information on dust and argon levels in the atmosphere, water and chlorine levels in the subsurface, wind speeds, humidity, temperature, ultraviolet radiation, pressure, and capturing movies and images of dust devils. This weekend is no different, adding a full complement of activities from almost every team — Navcam, REMS, DAN, Mastcam, ChemCam, and APXS will all collect data for the environmental and atmospheric theme group (ENV) in this plan.

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May 06, 2025

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Crew Kicks off Week with Agriculture and Tech Work, Wraps Spacewalk Cleanup

Crew Kicks off Week with Agriculture and Tech Work, Wraps Spacewalk Cleanup

NASA astronaut and Expedition 72 Flight Engineer Anne McClain points a camera towards herself and takes a
NASA astronaut and Expedition 72 Flight Engineer Anne McClain points a camera towards herself and takes a “space-selfie” during a spacewalk to upgrade the orbital outpost’s power generation system and relocate a communications antenna. Reflected in her helmet’s visor is fellow spacewalker and NASA astronaut Nichole Ayers.
NASA

The Expedition 73 crew members are kicking off a busy week aboard the International Space Station. Technology development, space botany, and clean up following last Thursday’s spacewalk topped Monday’s schedule.

The morning started with NASA astronaut Nichole Ayers and current station commander Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) teaming up to check out the petri plates housing thale cress plant in the station’s Veggie facility. The duo harvested some of the plants as part of the APEX-12 experiment, which observes how space radiation affects plant genetics.

Following space botany work, Ayers moved onto troubleshooting communications and network hardware before completing her daily two hours of exercise on the station’s treadmill and Advanced Resistive Exercise Device.

To wrap up cleanup duties following Ayers’ and NASA Astronaut Anne McClain’s 5 hour and 44-minute spacewalk last Thursday, Onishi spent the afternoon on spacesuit work, performing a cooling loop scrub. He was later joined by NASA’s Jonny Kim as the first-time space resident removed batteries from the spacesuits and the propulsive jetpack system (SAFER).

Kim also spent part of his day connecting with students from Verona, Italy, where he answered questions about living and working aboard the orbiting laboratory during a Ham Radio call and later performed routine on-orbit plumbing.

McClain set her sights to monitoring an ongoing tech demonstration that looks at capabilities for producing pharmaceutical ingredients in space that could be used to synthesize medications during future deep-space missions. She removed samples in the ADSEP cassette carriers then installed new cassettes for future analysis. Midafternoon, she photographed tomato plants for a space agricultural study to help researchers better understand if crops can be cultivated in space without photosynthesis. She later collected water samples from the Water Processing Assembly for chemical analysis and reorganized cargo racks in SpaceX’s Dragon cargo spacecraft, which arrived to the microgravity lab April 22.

The station’s three cosmonauts had a busy day of cleaning, cargo operations, and experiment prep. Flight Engineers Sergey Ryzhikov and Alexey Zubritsky worked together auditing Roscosmos cargo that will be loaded in the Progress 90 spacecraft before its eventual departure from the station. The duo then installed photo and videography hardware for a future experiment that will examine the station’s aerodynamic force. Meanwhile, Flight Engineer Kirill Peskov conducted routine orbital cleaning in the Roscosmos segment and synced up the cameras the trio uses to photograph Earth and its landmarks.

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

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Abby Graf