Artemis II Orion Spacecraft Stacked

Artemis II Orion Spacecraft Stacked

The orange core stage of the Artemis II rocket with white boosters on each side fully stacked inside the Vehicle Assembly Building at NASA's Kennedy Space Center in Florida on Saturday, Oct. 18, 2025.
NASA/Kim Shiflett

In this Oct. 20, 2025, photo, NASA’s Artemis II Orion spacecraft with its launch abort system is stacked atop the agency’s SLS (Space Launch System) rocket in the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida.

Orion will carry NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen on a 10-day mission around the Moon and back in early 2026.

Follow along with the mission on the NASA Artemis blog.

Image credit: NASA/Kim Shiflett

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Monika Luabeya

Crew Works Wide Variety of Research and Awaits New Arrivals

Crew Works Wide Variety of Research and Awaits New Arrivals

A yellow-green airglow blankets Earth’s horizon beneath a star-filled sky in this long-exposure photograph taken from the International Space Station as it orbited 265 miles above the cloudy Pacific Ocean off the coast of Chile. In the right foreground, the Soyuz MS-27 crew spacecraft is docked to the Prichal module, which is itself attached to the Nauka science module.
A yellow-green airglow blankets Earth’s horizon beneath a star-filled sky in this long-exposure photograph taken from the International Space Station as it orbited 265 miles above the cloudy Pacific Ocean off the coast of Chile.
NASA

High intensity exercising and droplets teeming with particles were the main research topics aboard the International Space Station on Tuesday. The Expedition 73 crew is also preparing to welcome three new crewmates this week while another trio gets ready to return to Earth next month.

Crew health monitoring and fitness evaluations are a crucial part of an astronaut’s stay aboard the orbital outpost. The long-duration missions in microgravity affect the crew member’s body in numerous ways and daily exercise helps keep crews fit and healthy while living in weightlessness. Doctors constantly monitor the crew with a variety of checkups, sensors, questionnaires, and more to ensure mission success off the Earth.

NASA Flight Engineers Jonny Kim and Zena Cardman took part in one portion of the CIPHER human research study looking at how the cardiovascular system adapts to space. Cardman scanned Kim’s chest with the Ultrasound 2 device while electrodes recorded his cardiac activity. Doctors on the ground monitored in real-time to understand how his heart is adapting to living in space.

Next, Kim pedaled on the Destiny laboratory module’s exercise cycle while attached to sensors and breathing gear that monitored his heart and lung activity. Doctors will use the data collected from the hardware to evaluate aerobic capacity, or the bodies’ ability to deliver and use oxygen during strenuous physical activity in space. Afterward, he rejoined Cardman and reviewed procedures, tools, and communications necessary for a medical emergency aboard the space station.

NASA Flight Engineer Mike Fincke set up a fluorescence microscope inside Destiny and installed sample hardware so scientists on the ground could view how particles behave inside fluids. The fluid physics study may inform commercial in-space manufacturing techniques and improve optical materials and pollution removal operations.

Flight Engineer Kimiya Yui from JAXA (Japan Aerospace Exploration Agency) spent the first half of his shift reorganizing cargo inside the Kibo laboratory module to make space for upcoming activities. Later, Yui measured the airflow inside of his crew quarters located inside the Harmony module. The measurements help protect health and promote comfort for the crew.

Station Commander Sergey Ryzhikov from Roscosmos worked inside the Soyuz MS-27 crew spacecraft that he, Kim, and Roscosmos Flight Engineer Alexey Zubritsky will return to Earth in next month. Ryzhikov first checked the Soyuz’ electronics and communications systems then continued loading cargo inside the spacecraft for the ride back to Earth.

Zubritsky began his shift collecting his blood, saliva, and hair samples for analysis to understand how the brain and immune system adapt to weightlessness. He then spent the rest of his day checking the Roscosmos segment’s ventilation system and collecting station water samples for analysis to protect crew health.

Roscosmos Flight Engineer Oleg Platonov photographed and treated microbe samples collected on the station. Researchers will use the observations to learn how microbes survive in space and prevent contamination on spacecraft.

Back on Earth, three new crew members are counting down to their launch aboard the Soyuz MS-28 crew spacecraft from the Baikonur Cosmodrome in Kazakhstan to the International Space Station. NASA astronaut Chris Williams and Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev are scheduled to lift off inside the Soyuz at 4:27 a.m. EDT (2:27 p.m. Baikonur time) on Thursday, Nov. 27. They will orbit Earth twice before docking to the Rassvet module at 7:38 a.m. the same day to begin an eight-month space research mission. Live launch coverage begins 3:30 a.m. on NASA+, Amazon Prime, and YouTube.

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

LSAH Newsletter

LSAH Newsletter

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Reid Wiseman in the station’s Destiny lab.
Reid Wiseman finds a little peace and quiet in the station’s Destiny lab.
NASA

The Lifetime Surveillance of Astronaut Health (LSAH) program collects, analyzes, and interprets medical, physiological, hazard exposure, and environmental data for the purpose of maintaining astronaut health and safety as well as preventing occupationally induced injuries or disease related to space flight or space flight training. It allows NASA to effectively understand and mitigate the long-term health risks of human spaceflight, as well as support the physical and mental well-being of astronauts during future exploration missions.

The LSAH Newsletter serves to inform and update former astronauts on how their medical data is being utilized by the LSAH team. It is published and distributed bi-annually.

+ October 2025 | Vol 30 Issue 2 – LSAH Newsletter

+ Past LSAH Newsletters and Publications

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Nov 25, 2025

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Robert E. Lewis

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Ahmed El-Rasheedy

NASA’s Roman Observatory Passes Spate of Key Tests

NASA’s Roman Observatory Passes Spate of Key Tests

NASA’s nearly complete Nancy Grace Roman Space Telescope has made another set of critical strides toward launch. This fall, the outer portion passed two tests — a shake test and an intense sound blast — to ensure its successful launch. The inner portion of the observatory underwent a major 65-day thermal vacuum test, showing that it will function properly in space. As NASA’s next flagship space telescope, Roman will address essential questions in the areas of dark energy, planets outside our solar system, and astrophysics.

Core portion of Roman observatory exiting test chamber
The inner portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the telescope, instrument carrier, two instruments, and spacecraft) recently passed thermal vacuum testing. In this photo, the assembly is being lifted out of the Space Environment Simulator after completing 65 days of assessments.
Credit: NASA/Jolearra Tshiteya

“We want to make sure Roman will withstand our harshest environments,” said Rebecca Espina, a deputy test director at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “From a mechanical standpoint, our heaviest loads and stresses come from launch, so we use testing to mimic the launch environment.”

The vibration and acoustic testing were the final round of launch simulations for the outer portion of the Roman observatory, which consists of the outer barrel assembly, deployable aperture cover, and recently installed flight solar panels.

During acoustic testing, a large chamber with gigantic horns emulated the launch’s thunderous sounds, which cause high-frequency vibrations. Test operators outfitted the chamber and assembly with various sensors to monitor the hardware’s response to the sound, which gradually ramped up to a full minute at 138 decibels — louder than a jet plane’s takeoff at close range!

After moving to a massive shaker table, Roman’s outer assembly went through testing to replicate the rocket launch’s lower-frequency vibrations. Each individual test lasts only about a minute, sweeping from 5 to 50 hertz (the lowest note on a grand piano vibrates at 27.5 hertz), but NASA engineers tested three axes of movement over several weeks, breaking up the tests with on-the-spot data analysis.

Like in acoustic testing, the team installed sensors to capture the assembly’s response to the shaking. Structural analysts and test operators use this information not only to evaluate success but also to improve models and subsequent assessments.

“There’s a real sense of accomplishment when you get a piece of hardware this large through this test program,” said Shelly Conkey, lead structural analyst for this assembly at NASA Goddard. “I am proud of the work that our team of people has done.”

The outer portion of the Roman observatory stands in the acoustic testing chamber
The outer portion of NASA’s Nancy Grace Roman Space Telescope (which consists of the outer barrel assembly, deployable aperture cover, and solar panels) recently passed vibration and acoustic testing. The structure is shown here in the acoustic testing chamber at NASA’s Goddard Space Flight Center in Greenbelt, Md., where it was blasted with intense sound to simulate launch conditions.
Credit: NASA/Jolearra Tshiteya

The core portion of the observatory (the telescope, instrument carrier, two instruments, and spacecraft bus) moved into the Space Environment Simulator test chamber at NASA Goddard in August. There, it was subjected to extreme temperatures to mimic the chill of space and heat from the Sun. A team of more than 200 people ran simulations continuously for more than two months straight, assessing the telescope’s optics and the assembly’s overall mission readiness.

“The thermal vacuum test marked the first time the telescope and instruments were used together,” said Dominic Benford, Roman’s program scientist at NASA Headquarters in Washington. “The next time we turn everything on will be when the observatory is in space!”

Gif of the inner portion of the observatory exiting thermal vacuum testing
Following extensive assessments, the core portion of NASA’s Nancy Grace Roman Space Telescope was removed from the test chamber (as shown in this gif) and returned to the largest clean room at NASA’s Goddard Space Flight Center in Greenbelt, Md. Next, it will be prepped for final integration.
Credit: NASA/Sophia Roberts

The team expects to connect Roman’s two major parts in November, resulting in a complete observatory by the end of the year. Following final tests, Roman will move to the launch site at NASA’s Kennedy Space Center in Florida for launch preparations in summer 2026. Roman remains on schedule for launch by May 2027, with the team aiming for as early as fall 2026.

The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems Inc. in Boulder, Colorado; L3Harris Technologies in Rochester, New York; and Teledyne Scientific & Imaging in Thousand Oaks, California.

For more information about the Roman Space Telescope, visit:

https://www.nasa.gov/roman

By Laine Havens and Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Media contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940

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Last Updated

Nov 25, 2025

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Ashley Balzer
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Ashley Balzer
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Goddard Space Flight Center

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Ashley Balzer

Red Spider Nebula

Red Spider Nebula

A multicolored nebula stands out against the star-studded background of space. The nebula’s central star is hidden by a blotchy pinkish cloud of dust. A strong red light radiates from this area, lighting up the nearby dust. An elongated purple ‘S’ shape is centered on the heart of the nebula, while two blue lobes stretch diagonally outward to the edges of the image, making the entire structure look like a tilted hourglass.
ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)

Using its Near-InfraRed Camera (NIRCam), NASA’s James Webb Space Telescope captured never-before-seen details of the Red Spider Nebula, a planetary nebula, in this image released on Oct. 26, 2025. NIRCam is Webb’s primary near-infrared imager, providing high-resolution imaging and spectroscopy for a wide variety of investigations.

Webb’s new view of the Red Spider Nebula reveals for the first time the full extent of the nebula’s outstretched lobes, which form the ‘legs’ of the spider. These lobes, shown in blue, are traced by light emitted from H2 molecules, which contain two hydrogen atoms bonded together. Stretching over the entirety of NIRCam’s field of view, these lobes are shown to be closed, bubble-like structures that each extend about 3 light-years. Outflowing gas from the center of the nebula has inflated these massive bubbles over thousands of years.

Image credit: ESA/Webb, NASA & CSA, J. H. Kastner (Rochester Institute of Technology)

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Monika Luabeya