NASA Marks Milestone in Preparation for Artemis IV Testing

NASA Marks Milestone in Preparation for Artemis IV Testing

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

New cooling systems are tested at the Thad Cochran Test Stand
NASA Stennis teams complete a water system activation milestone on Jan. 30 at the Thad Cochran Test Stand (B-2). The milestone tested new cooling systems added to the stand for the future Green Run test series of NASA’s exploration upper stage that is expected to fly on the Artemis IV mission.
NASA/Danny Nowlin

Water flowing out. Data flowing in.

A water system activation at the Thad Cochran Test Stand (B-2) on Jan. 30 at NASA’s Stennis Space Center near Bay St. Louis, Mississippi, helped capture critical data to support testing a new SLS (Space Launch System) stage expected to fly on the Artemis IV mission.

The activation milestone tested new cooling systems that were added for the future Green Run test series of NASA’s exploration upper stage (EUS). The more powerful upper stage is a four-engine liquid hydrogen/liquid oxygen in-space stage for the evolved Block 1B version of SLS.

For Green Run, teams at NASA Stennis will activate and test all systems to ensure the stage is ready to fly. It will culminate with a hot fire of the stage’s four RL10 engines, just as during an actual mission.

As part of the test stand modification, crews have added water-cooled diffusers to act as a heat shield to manage the super-hot exhaust from all four RL10 engines; water-cooled fairings to direct engine exhaust to align with the diffuser walls; and a purge ring that supplies cooling water and gaseous nitrogen to protect a flexible seal that allows the engines to move, or gimbal, during testing.

These three systems all were integrated by the NASA Stennis team with the existing flame deflector and acoustic suppression equipment used during previous core stage testing for NASA’s SLS rocket ahead of the successful Artemis I launch.

NASA/Stennis

The exercise also pushed the high pressure industrial water system to maximum capacity. While a typical RS-25 engine test at NASA Stennis runs a subset of the 10 diesel pumps and one electric pump, testing the exploration upper stage will require all eleven pumps running simultaneously.

The 14-million gallons of water used during the exercise on Jan. 30 was recycled throughout the test complex. A 66-million-gallon reservoir feeds water to the test stand through an underground 96-inch diameter pipe, with water distributed to various cooling components. The water ultimately flows into the flame deflector, then through a concrete flume to the stand’s catch pond. When the catch pond fills up, the excess water drains back to the canal through a drainage ditch, ready to be recycled for future use.

“We will use the data gathered to set the final timing of when valves are cycled, determine our redline pressures, and select the operating pressure,” said Nick Nugent, NASA Stennis project engineer. “This exercise also put the water system under a full load prior to the final stress test. It is always good to give the system a good shake down run prior.”

Water vapor escapes the Thad Cochran Test Stand as the new cooling systems are tested
NASA Stennis teams complete a water system activation milestone on Jan. 30 at the Thad Cochran Test Stand (B-2). The milestone tested new cooling systems added to the stand for the future Green Run test series of NASA’s exploration upper stage that is expected to fly on the Artemis IV mission.
NASA/Danny Nowlin

The exploration upper stage is being built by Boeing at NASA’s Michoud Assembly Facility in New Orleans. The four RL10 engines for the upper stage are manufactured by L3Harris Technologies. Before it all arrives at NASA Stennis, crews will perform a final 24-hour check, or stress test, across all test complex facilities to demonstrate readiness for the test series.

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LaToya Dean

Summer Heat Hits Southeastern Australia

Summer Heat Hits Southeastern Australia

A map of Australia depicts near-surface air temperatures, where most of the country is warm, shown as orange to red. Extreme heat is concentrated over the southeast, and a small cooler blue area appears in Western Australia.
January 29, 2026

While a part of the United States braved extreme winter cold, January 2026 brought sweltering summer conditions to many parts of Australia.

Australia’s area-averaged mean temperature was 1.90 degrees Celsius (3.42 degrees Fahrenheit) above the 1961–1990 average, making it the fourth-warmest January since the start of observations in 1910, according to the Bureau of Meteorology (BoM). Contributing to this was a late-month heatwave in the country’s southeast that was especially intense between January 26 and January 30. During that period, numerous weather stations in South Australia, New South Wales, and Victoria recorded record-high daily temperatures.

The heatwave’s intensity and extent are evident in this map, which shows air temperatures at 03:00 Universal Time (2 p.m. local time in Victoria) on January 29, modeled at 2 meters (6.5 feet) above the ground. It was produced with a version of the GEOS (Goddard Earth Observing System) model, which integrates meteorological observations with mathematical equations that represent physical processes in the atmosphere. The darkest reds are where the model indicates temperatures reaching or exceeding 45°C (113°F).                                                                                                                                                                

According to BoM, the hottest temperatures of January 2026 were measured in two places in South Australia: in the town of Andamooka on the 29th and at the Port Augusta airport on the 30th, where temperatures reached 50.0°C (122.0°F). In both New South Wales and Victoria, the month’s hottest day was on the 27th, when temperatures reached 49.7°C (121.5°F) at a station in Pooncarie and 48.9°C (120.0°F) at stations in Walpeup and Hopetoun.

The heatwave brought significant human and public-health effects, including the increased risk of heat-related illness. Organizers of the Australian Open tennis tournament in Melbourne, Victoria, suspended play on some courts and closed roofs to provide shade as part of an “extreme heat policy” to protect players and spectators, according to news reports.

The recent warmth followed another bout of heat earlier in the month that, combined with strong winds and dry conditions, created dangerous fire conditions. Numerous bushfires were burning across Victoria on January 9 as officials urged people to evacuate. By mid-month, news reports indicated that the fires had destroyed hundreds of structures and killed tens of thousands of livestock.

NASA Earth Observatory image by Lauren Dauphin, using GEOS data from the Global Modeling and Assimilation Office at NASA GSFC. Story by Kathryn Hansen.

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Extreme January Cold

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Cardiac and Psychology Research on Station as Crew-12 Adjusts Launch Date

Cardiac and Psychology Research on Station as Crew-12 Adjusts Launch Date

Image of the International Space Station orbiting the Earth.
This mosaic taken on Dec. 8, 2021, depicts the International Space Station pictured from the SpaceX Dragon during a fly around of the orbiting lab that took place following its undocking from the Harmony module on Nov. 8, 2021.
NASA

NASA and SpaceX have completed a weather review and have waived off Crew-12’s Thursday, Feb. 12, launch opportunity to the International Space Station due to unfavorable forecasted weather conditions. Meanwhile, the Expedition 74 crew focused on astronaut health research, cargo operations, and lab maintenance.

Mission teams are targeting the launch of NASA’s SpaceX Crew-12 mission for no earlier than 5:15 a.m. EST on Friday, Feb. 13, from Cape Canaveral Space Force Station in Florida. NASA astronauts Jessica Meir and Jack Hathaway along with ESA (European Space Agency) astronaut Sophie Adenot and Roscosmos cosmonaut Andrey Fedyaev would then dock to the space station’s Harmony module at 3:15 p.m. on Saturday, Feb. 14. The commercial crew quartet will stay in space for a nine-month microgravity research mission.

Back on the orbital outpost, NASA Flight Engineer Chris Williams began his shift with a fitness test measuring his cardiovascular health. Williams attached sensors to his chest and strapped on a heart rate monitor then pedaled for an hour on an exercise bike in the Destiny laboratory module. Doctors on the ground monitored his workout session in real time to detect potential signs of space-caused distress and ensure his long-term well-being off the Earth.

Williams ended his day continuing to pack completed science experiments, their associated samples, and station hardware inside a SpaceX Dragon spacecraft for return to Earth on an upcoming date. Dragon arrived at the orbital outpost on Aug. 25, 2025, delivering over 5,000 pounds of scientific investigations, station hardware, and crew supplies.

Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev took turns measuring their heart activity using electrodes and collecting their blood pressure measurements wearing cuffs on their arm, wrist, and thumb. Their biomedical data was recorded to a computer and will be shared with doctors on Earth to assess microgravity’s effect on blood flow regulation and inflammation responses.

Kud-Sverchkov then studied how living in space affects memory and immunity. He first collected his saliva and hair samples for analysis. Next, he took a test measuring his sleep quality, daily moods, and the stress levels he experiences. Finally, he collected his heart and oxygen data and saved the data to a computer. Doctors will use the data to investigate how living in space long term impacts a crew member’s psychological state.

Mikaev focused on maintenance during the first part of his shift on Tuesday starting in the Nauka science module and servicing its ventilation system then inspecting and photographing cargo panels in the Zarya module. Next, he participated in a psychological test to determine how living in space affects his personality characteristics and his team behavior. Researchers will use the insights to help prevent stress-related health issues, maintain cognitive performance, and maintain team harmony during a spaceflight.

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

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Mark A. Garcia

Curiosity Blog, Sols 4798-4803: Back for More Science

Curiosity Blog, Sols 4798-4803: Back for More Science

2 min read

Curiosity Blog, Sols 4798-4803: Back for More Science

An overhead color photo of the Martian surface shows pale orange-tan, flat, rocky terrain, with the surface a mixture of jagged-edged slabs with fine soil leveling the gaps between them, and small rocks of various sizes scattered around the surface. Near the image center and at lower-right are two drill holes in the rock, each with mounded soil around the opening that had been extracted from the holes during drilling.
NASA’s Mars rover Curiosity acquired this image showing the side-by-side drill holes “Nevado Sajama” (right) and “Nevado Sajama2” (left). Curiosity used its Mast Camera (Mastcam) to capture the image on Jan. 31, 2026 — Sol 4795, or Martian day 4,795 of the Mars Science Laboratory mission — at 22:55:27 UTC.
NASA/JPL-Caltech/MSSS

Written by Michelle Minitti, MAHLI Deputy Principal Investigator

Earth planning date: Friday, Feb. 6, 2026

The results from our first visit to the “Nevado Sajama” drill location were intriguing enough to motivate our return to do a deeper dive into the minerals and compounds locked in this rock with SAM (the Sample Analysis at Mars instrument suite). As explained in the last blog, that deeper dive involves using the second of two vials of a chemical reagent, tetramethylammonium hydroxide (TMAH), that helps makes molecules detectable to SAM that would otherwise be undetectable. This week was focused on completing the many carefully-coordinated steps to apply the TMAH reagent to the rock powder from a drill hole and then analyze the treated sample. As you can see in the image above, we know the drilling necessary to collect the sample was successful, as was delivery of the sample to SAM. We are awaiting word about the first part of the SAM analysis, and are running the second part in the weekend plan. 

As you can imagine, running a mass spectrometer and chemistry experiment remotely on another planet takes a lot of energy, but throughout the week, the team took advantage of whatever spare power there was to include additional science observations. ChemCam planned two attempts at targeting the Nevado Sajama2 drill-hole interior, analyzed “Tiquipaya,” one of the family of rocks broken by the rover wheels that expose bright white material, and measured the chemistry of the atmosphere with a passive sky observation. They also planned an RMI mosaic of layers near the base of the “Mishe Mokwa” butte to our east. MAHLI and APXS paired up to image and analyze the ground-up tailings around the drill hole for the most direct measure of chemistry of what SAM analyzes. As Mastcam acquired a full 360-degree mosaic the first time we were at Nevado Sajama, they did not have many rock observations to plan. Instead, they turned their eyes toward the sky to measure the amount of dust in the atmosphere. Navcam made complementary measurements of atmospheric dust and planned movies and imaging surveys of clouds and dust devils. Ever watchful, RAD and REMS made their regular measurements of the Martian environment while DAN regularly monitored the Martian subsurface. 

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Feb 10, 2026

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CubeSats’ Missions Begin

CubeSats’ Missions Begin

Two CubeSats, one silver and one with a red face, are ejected from the International Space Station (bottom left) into the blackness of space.
NASA/Chris Williams

NASA astronaut Chris Williams pointed a camera out a window on the cupola as a set of CubeSats were deployed outside the Kibo laboratory module by a small satellite orbital deployer into Earth orbit. Students from Mexico, Italy, ThailandMalaysia, and Japan designed the shoe-boxed satellites for a series of Earth observations and technology demonstrations.

CubeSats are a class of nanosatellites – small spacecraft weighing 1-10 kilograms – that use a standard size and form factor. The development of CubeSats has advanced into its own industry with government, industry and academia collaborating for ever increasing capabilities.  CubeSats now provide a cost-effective platform for science investigations, new technology demonstrations and advanced mission concepts.

Image credit: NASA/Chris Williams

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Monika Luabeya