Week Wraps on Station With Cardiac Research, Stem Cells, and Eye Checks

Week Wraps on Station With Cardiac Research, Stem Cells, and Eye Checks

A bright yellow-green airglow blankets Earth's horizon, dotted with the city lights of northern India, beneath a star-filled sky. This long-exposure photograph was taken from the International Space Station as it orbited 260 miles above the Himalayas at approximately 1:11 a.m. local time.
A bright yellow-green airglow blankets Earth’s horizon, dotted with the city lights of northern India, beneath a star-filled sky. This long-exposure photograph was taken from the International Space Station as it orbited 260 miles above the Himalayas at approximately 1:11 a.m. local time.
NASA

Cardiac research, stem cell observations, and eye checks to ensure astronaut health wrapped up the week for the Expedition 73 crew aboard the International Space Station. The orbital residents also continued working on spacesuits and unpacked a pair of resupply ships rounding out their work week.

Doctors continuously study how living in weightlessness affects a crew member’s circulatory system from the heart to the tiniest vessels and blood cells. The station crew is constantly monitored through a variety of devices including electrodes, ultrasounds, and blood pressure cuffs providing insights potentially informing advanced ways to protect astronaut health on future missions to the Moon, Mars, and beyond.

Station Commander Sergey Ryzhikov and Flight Engineer Alexey Zubritsky, both Roscosmos cosmonauts, continued exploring how blood circulates to and from the smallest vessels in a crew member’s body. The duo once again wore sensors on their forehead, fingers, and toes that monitored blood flowing to their microcirculatory and tissue systems. The medical data may help researchers develop techniques that protect future space crews on long-duration missions and prepare them for the return to Earth’s gravity.

NASA Flight Engineer Jonny Kim assisted veteran Flight Engineer Mike Fincke from NASA as he treated stem cells inside the Kibo laboratory module’s Life Science Glovebox. Fincke placed the stem cell samples inside the KERMIT fluorescence microscope so scientists could observe how the programmed cells grow and change into heart and brain cells in microgravity. Results may lead to personalized health treatments in space and advanced treatments for heart conditions and degenerative neurological disorders on Earth.

Kim then joined NASA Flight Engineer Zena Cardman as she scanned his eyes in the Columbus laboratory module using standard medical imaging gear found in a doctor’s office on Earth. Cardman first attached electrodes to Kim’s forehead and to the sides of his eyes that sent flashes of light to measure the electrical response of Kim’s retinas. Next, she operated optical gear inside the Harmony module that sent lightwaves into his eyes so doctors on the ground could observes the retina, cornea, and optic nerve in real time. Doctors will use the data to look for and learn how to prevent space-caused vascular structure and functional changes to a crew member’s eyes.

Cardman, Kim and Fincke also took turns servicing spacesuits inside the Quest airlock. The trio removed and installed batteries on the suits and swapped a life support device inside the suit that provides ventilation and cooling during a spacewalk.

Earlier in their shift, Kim and Fincke spent some time unpacking science, supplies, and hardware recently delivered aboard a pair cargo ships. Kim offloaded some of the new life support gear and science experiments packed inside JAXA’s (Japan Aerospace Exploration Agency) HTV-X1 resupply ship that arrived on Oct. 29.  Fincke continued transferring some of the 11,000 pounds of research and supplies packed inside Northrop Grumman’s Cygnus XL cargo spacecraft.

JAXA Flight Engineer Kimiya Yui spent his day primarily on maintenance first inspecting filters inside the Columbus lab’s BioLab research incubator then cleaning the Tranquility module’s ventilation system. Roscosmos Flight Engineer Oleg Platonov also worked throughout the day on maintenance in the station’s Roscosmos segment checking smoke detection equipment and photographing module windows for inspection.

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.

Get the latest from NASA delivered every week. Subscribe here.

Powered by WPeMatico

Get The Details…

Mark A. Garcia

NASA Sets Launch Coverage for International Ocean Tracking Mission

NASA Sets Launch Coverage for International Ocean Tracking Mission

In this artist’s concept, the ocean-observing satellite Sentinel-6B orbits Earth with its deployable solar panels extended.
In this artist’s concept, the ocean-observing satellite Sentinel-6B orbits Earth with its deployable solar panels extended.
Credit: NASA/JPL-Caltech

NASA will provide live coverage of prelaunch and launch activities for Sentinel-6B, an international mission delivering critical sea level and ocean data to protect coastal infrastructure, improve weather forecasting, and support commercial activities at sea.

Launch is targeted at 12:21 a.m. EST, Monday, Nov. 17 (9:21 p.m. PST, Sunday, Nov. 16) aboard a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California.

Watch coverage beginning at 11:30 p.m. EST (8:30 p.m. PST) on NASA+, Amazon Prime, and more. Learn how to watch NASA content through a variety of platforms, including social media.

The Sentinel-6B mission continues a decades-long effort to monitor global sea level and ocean conditions using precise radar measurements from space. Since the early 1990s, satellites launched by NASA and domestic and international partners have collected precise sea level data. The launch of Sentinel-6B will extend this dataset out to nearly four decades.

NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):

Saturday, Nov. 15

4 p.m. – NASA Prelaunch Teleconference on International Ocean Tracking Mission

  • Karen St. Germain, director, Earth Science Division, NASA Headquarters in Washington
  • Pierrik Veuilleumier, Sentinel-6B project manager, ESA (European Space Agency)
  • Parag Vaze, Sentinel-6B project manager, NASA’s Jet Propulsion Laboratory in Pasadena, California
  • Tim Dunn, senior launch director, Launch Services Program, NASA’s Kennedy Space Center in Florida
  • Julianna Scheiman, director, NASA Science Missions, SpaceX
  • 1st Lt. William Harbin, launch weather officer, U.S. Air Force

Audio of the teleconference will stream on the NASA Video YouTube channel.  

Media interested in participating by phone must RSVP no later than two hours prior to the start of the call at: ksc-newsroom@mail.nasa.gov. A copy of NASA’s media accreditation policy is online.

Sunday Nov. 16

11:30 p.m. – Launch coverage begins on NASA+, Amazon Prime, and more.

Audio-only coverage

Audio-only of the launch coverage will be carried on the NASA “V” circuits, which may be accessed by dialing 321-867-1220 or -1240. On launch day, “mission audio” countdown activities without NASA+ launch commentary will be carried at 321-867-7135.

NASA website launch coverage

Launch day coverage of the mission will be available on the agency’s website. Coverage will include links to live streaming and blog updates beginning no earlier than 11 p.m. EST, Nov. 16, as the countdown milestones occur. Streaming video and photos of the launch will be accessible on demand shortly after liftoff. Follow countdown coverage on NASA’s Sentinel-6/Jason-CS blog.

For questions about countdown coverage, contact the NASA Kennedy newsroom at: 321-867-2468.

Attend launch virtually

Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch.

Watch, engage on social media

Let people know you’re watching the mission on X, Facebook, and Instagram by following and tagging these accounts:

X: @NASA, @NASAKennedy, @NASAJPL, @NASAEarth

Facebook: NASA, NASA Kennedy, NASA JPL, NASA Earth

Instagram: @NASA, @NASAKennedy, @NASAJPL, @NASAEarth

Sentinel-6B is the second of twin satellites in the Copernicus Sentinel-6/Jason-CS (Continuity of Service) mission, a collaboration among NASA, ESA, EUMETSAT (European Organisation for the Exploitation of Meteorological Satellites), and the National Oceanic and Atmospheric Administration (NOAA). The first satellite in the mission, Sentinel-6 Michael Freilich, launched in November 2020. The European Commission contributed funding support, while France’s space agency CNES (Centre National d’Études Spatiales) provided technical expertise. The mission also marks the first international involvement in Copernicus, the European Union’s Earth Observation Programme.

For more information about these missions, visit:

https://science.nasa.gov/mission/sentinel-6b/

-end-

Elizabeth Vlock
NASA Headquarters, Washington
202-358-1600
elizabeth.a.vlock@nasa.gov

Leejay Lockhart
Kennedy Space Center, Fla.
321-747-8310
leejay.lockhart@nasa.gov

Andrew Wang / Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-393-2433
andrew.wang@jpl.nasa.gov / andrew.c.good@jpl.nasa.gov

Powered by WPeMatico

Get The Details…
Tiernan P. Doyle

Mapping Dark Matter

Mapping Dark Matter

Webb near-infrared data combined with Chandra X-ray data of the Bullet Cluster show many overlapping objects, including foreground stars, galaxies in galaxy clusters, and distorted background galaxies behind the galaxy clusters. The objects are all at various distances set against the black background of space. Most galaxies appear as tiny fuzzy ovals in white, orange, or red. A slightly larger, very bright, light blue spiral galaxy is at center. To its immediate left and right are two large bright pink splotches representing X-rays. The right pink area has a rounded nose facing right, where it is darker pink, and fades to the left as a triangular shape. This is referred to as the Bullet. To the far left and far right, next to the pink regions, are two blue regions representing dark matter mass. The left blue region is a large, long oval at an angle. The blue region at right is a far smaller oval.
NASA, ESA, CSA, STScI, CXC

This image released on June 30, 2025, combines data from NASA’s James Webb Space Telescope and NASA’s Chandra X-ray Observatory to visualize dark matter. Researchers used Webb’s observations to carefully measure the mass of the galaxy clusters shown here as well as the collective light emitted by stars that are no longer bound to individual galaxies.

Learn more.

Image credit: NASA, ESA, CSA, STScI, CXC

Powered by WPeMatico

Get The Details…
Monika Luabeya

NASA Glenn Teams Win 2025 R&D 100 Awards 

NASA Glenn Teams Win 2025 R&D 100 Awards 

Graphic drawing showing the Earth and the Moon with satellites in space linked by lasers to circles showing planetary habitats, satellite dishes, and the space station.
Artistic rendering of the High-Rate Delay Tolerant Networking protocol being used on the Laser Communications Relay Demonstration to transfer radio and optical communications between Earth and space.
Credit: NASA 

NASA’s Glenn Research Center in Cleveland has earned 2025 R&D 100 Awards for developing a system that delivers high-speed internet for space and co-inventing technology for a new class of soft magnetic nanocrystalline materials designed to operate at extreme temperatures. This brings NASA Glenn’s total to 130 R&D 100 Awards. 

High-Rate Delay Tolerant Networking  

NASA Glenn’s Daniel Raible and Rachel Dudukovich led their team of engineers to create High-Rate Delay Tolerant Networking  (HDTN), a cutting-edge software solution designed to revolutionize data streaming and communication in space. HDTN enables reliable, high-speed transmission of data between space and Earth — even under the extreme conditions of space — minimizing loss and system delay. 

Eleven people stand next to one another inside an airplane hangar. Two small planes sit behind them. An American flag and a banner reading “Welcome! John H. Glenn Research Center at Lewis Field, Cleveland, Ohio” are visible behind the group.
High-Rate Delay Tolerant Networking team photo, left to right: Tad Kollar, Eric Brace, Brian Tomko, José Lombay-González, Nadia Kortas, Daniel Raible, John Nowakowski, Shaun McKeehan, Ethan Schweinsberg, Prash Choksi, and Rachel Dudukovich.
Credit: NASA/Jef Janis 

“The HDTN software protocol allows faster, automated, and seamless data transfer between spacecraft, even across communication systems operating on different link speeds,” Raible said. “It’s up to 10 times faster than current delay-tolerant networking (DTN).” 

This advanced technology has far-reaching implications beyond NASA. With its open-source code, HDTN paves the way for collaboration, innovation, and adoption across the rapidly expanding commercial space industry, offering near real-time communication capabilities. 

Looking ahead, HDTN could form the foundation of a solar system-wide internet, supporting data exchange between Earth, spacecraft, and even future missions involving human travel to the Moon and Mars. 

VulcanAlloy 

In a project led by the University of Pittsburgh, researchers at NASA Glenn, including Nick Bruno, Grant Feichter, Vladimir Keylin, Alex Leary, and Ron Noebe, partnered with CorePower Magnetics to develop VulcanAlloy — a breakthrough soft magnetic nanocrystalline material. 

Two packaged inductors with electrical windings sit on a large plate with wiring attached to the inductors and to the Glenn Extreme Environments Rig.
NASA’s Glenn Research Center in Cleveland tested high-temperature inductors using VulcanAlloy technology in the NASA Glenn Extreme Environments Rig, which simulates the conditions on Venus’ surface, on May 13, 2025.
Credit: NASA 

VulcanAlloy, developed under NASA’s High Operating Temperature Technology Program using processing capability established by the Advanced Air Transport Technology project, operates above 500°C, far beyond the limits of conventional soft magnetic materials. Its nano-engineered structure maintains efficiency at high temperatures and frequencies. 

With adjustable magnetic properties, it can replace multiple materials in components like inductors, transformers, motors, and sensors while reducing the need for bulky cooling systems — ideal for extreme environments. 

Raytheon has tested VulcanAlloy cores, highlighting their potential in electrified aircraft, defense, and aerospace systems. 

This innovation also promises major impact in electric vehicles, data centers, microgrids, and energy systems, where smaller, lighter, and more efficient components are key to advancing next-generation power electronics. 

The R&D 100 Awards, a worldwide science and innovation competition, received entries from organizations around the world. Now in its 63rd year, this year’s judging panel included industry professionals from across the globe who evaluated breakthrough innovations in technology and science. 

Powered by WPeMatico

Get The Details…
Kelly M. Matter

Hubble Studies Star Ages in Colorful Galaxy

Hubble Studies Star Ages in Colorful Galaxy

2 min read

Hubble Studies Star Ages in Colorful Galaxy

An oval-shaped spiral galaxy. Only the center and lower half of the galaxy is in frame. Its center is primarily golden in color with a white glowing core, while its thick spiral arms are mostly blue, particularly at the outskirts; these colors merge in between. Dark lanes of dust swirl through the center, blocking some of the galaxy’s light. Stars and distant galaxies are visible around the edges on a black background.
This NASA/ESA Hubble Space Telescope image features the spiral galaxy called NGC 6000.
ESA/Hubble & NASA, A. Filippenko; Acknowledgment: M. H. Özsaraç

Stars of all ages are on display in this NASA/ESA Hubble Space Telescope image of the sparkling spiral galaxy called NGC 6000, located 102 million light-years away in the constellation Scorpius.

NGC 6000 has a glowing yellow center and glittering blue outskirts. These colors reflect differences in the average ages, masses, and temperatures of the galaxy’s stars. At the heart of the galaxy, the stars tend to be older and smaller. Less massive stars are cooler than more massive stars, and somewhat counterintuitively, cooler stars are redder, while hotter stars are bluer. Farther out along NGC 6000’s spiral arms, brilliant star clusters host young, massive stars that appear distinctly blue.

Hubble collected the data for this image while surveying the sites of recent supernova explosions in nearby galaxies. NGC 6000 hosted two recent supernovae: SN 2007ch in 2007 and SN 2010as in 2010. Using Hubble’s sensitive detectors, researchers can discern the faint glow of supernovae years after the initial explosion. These observations help constrain the masses of supernovae progenitor stars and can indicate if they had any stellar companions.

By zooming in to the right side of the galaxy’s disk in this image, you can see a set of four thin yellow and blue lines. These lines are an asteroid in our solar system that was drifting across Hubble’s field of view as it gazed at NGC 6000. The four lines are due to four different exposures recorded one after another with slight pauses in between. Image processors combined these four exposures to create the final image. The lines appear dashed with alternating colors because each exposure used a filter to collect very specific wavelengths of light, in this case around red and blue. Having these separate exposures of particular wavelengths is important to study and compare stars by their colors — but it also makes asteroid interlopers very obvious!

Media Contact:

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

Powered by WPeMatico

Get The Details…