Vision, Immune System Studies and Hardware Inspections Keep Crew Busy

Vision, Immune System Studies and Hardware Inspections Keep Crew Busy

(From left) Expedition 73 Flight Engineers Anne McClain and Nichole Ayers, both NASA astronauts, take a break and pose for a portrait aboard the International Space Station Destiny laboratory module.
(From left) Expedition 73 Flight Engineers Anne McClain and Nichole Ayers, both NASA astronauts, take a break and pose for a portrait aboard the International Space Station’s Destiny laboratory module.
NASA

Life science was back on the schedule for Wednesday as the Expedition 73 crew studied how living in space affects eye structure and cellular immunity. The International Space Station residents also maintained the upkeep of exercise gear, life support components, and orbital plumbing hardware.

The ongoing space biology investigations aboard the orbital lab constantly informs doctors how astronauts adapt to months of living and working in weightlessness. Scientists extrapolate the continuous research data and are using the insights to protect future crews on longer spaceflight missions to the Moon, Mars, and beyond.

Doctors are exploring potential space-caused changes to crew eye structure and function since vision is critical whether piloting a spacecraft, conducting advanced space science, or performing other mission critical tasks. NASA Flight Engineers Jonny Kim and Nichole Ayers kicked off their shift with a test measuring the electrical responses of the retina to light stimuli. Kim attached electrodes to his forehead and around his eyes and Ayers operated the specialized, data-collecting hardware to understand how the eye adjusts to long-term weightlessness. The study is just one part of the CIPHER suite of 14 human research investigations to learn how to keep crews healthy in space.

Kim later collected and stowed his urine samples in a science freezer for later analysis then swapped a pair of research incubators in the Columbus laboratory module. Ayers moved on to the Tranquility module and replaced orbital plumbing gear that removes inorganic impurities from the station’s water.

Station Commander Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) continued studying how the stress of spaceflight affects cellular immunity helping doctors defend crews against infections. Onishi started his day his processing his blood samples that were incubating for 24 hours inside the Kubik research incubator. Next, he stowed the samples in a science freezer to later analyze the blood cells for signs of space-caused cellular stress or tissue damage. Onishi finally inspected and cleaned an experimental carbon dioxide removal device that also recovers water for oxygen generation.

NASA Flight Engineer Anne McClain spent her day inside Tranquility servicing and inspecting the COLBERT treadmill. The regularly scheduled maintenance activities take place every six months as McClain greased axles, cleaned components, and measured the acoustic volume of the workout device while operating with a crew member. McClain wrapped up her shift in the Quest airlock preparing spacesuit hardware for stowage.

Earth observations were back on the schedule as Roscosmos Flight Engineer Alexey Zubritskiy pointed a camera out a station window and photographed islands in the Pacific Ocean and other landmarks across the Pacific coasts of Asia and North America. Veteran cosmonaut Sergey Ryzhikov deactivated imaging hardware that observes Earth’s nighttime atmosphere in ultraviolet wavelengths. Flight Engineer Kirill Peskov wrapped up several days of training, checkouts, and inspections on the European robotic arm (ERA) attached to the Nauka science module. The ERA can be used to maneuver spacewalkers, payloads, and external hardware on the orbital outpost’s Roscosmos segment.

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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Mark A. Garcia

Cosmic Dawn Screening

Cosmic Dawn Screening

Join NASA for a free screening of Cosmic Dawn, the incredible true story of the James Webb Space Telescope–humanity’s mission to unveil the early universe, against all odds.

Cosmic Dawn is the incredible true story of the James Webb Space Telescope – humanity’s largest and most powerful space telescope – on a mission to unveil the early universe, against all odds.

The 90-minute documentary brings viewers on an unprecedented journey through Webb’s delicate assembly, rigorous testing, and triumphant launch, showcasing the sheer complexity and breathtaking risks involved in creating a telescope capable of peering billions of years into the past. Follow the telescope from an idea developed at NASA’s Goddard Space Flight Center all the way to the launchpad in French Guiana, with never-before-seen footage captured by the Webb film crew offering intimate access to the challenges and triumphs along the way.

Wednesday, June 11th  2025 | 7:00 PM EDT, doors open at 6:00 PM EDT

The Greenbelt Theater | 129 Centerway, Greenbelt, MD 20770

Space is limited, so please RSVP HERE by June 9th to reserve your free tickets.

We look forward to sharing how NASA achieves the remarkable. 

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Lauren Choice Parker

Eccentric ‘Star’ Defies Easy Explanation, NASA’s Chandra Finds

Eccentric ‘Star’ Defies Easy Explanation, NASA’s Chandra Finds

Scientists have discovered a star behaving like no other seen before, giving new clues about the origin of a class of mysterious objects. This object, known as ASKAP J1832, shows regular changes in both radio wave and X-ray intensity every 44 minutes, the first time such variations have been seen for a class of objects discovered only three years ago. X-rays from Chandra are shown along with infrared data from the Spitzer Space Telescope, and radio from LOFAR. An inset shows a more detailed view of the immediate area around this unusual object in X-ray and radio light.
X-ray: NASA/CXC/ICRAR, Curtin Univ./Z. Wang et al.; Infrared: NASA/JPL/CalTech/IPAC; Radio: SARAO/MeerKAT; Image processing: NASA/CXC/SAO/N. Wolk

Scientists have discovered a star behaving like no other seen before, giving fresh clues about the origin of a new class of mysterious objects.

As described in our press release, a team of astronomers combined data from NASA’s Chandra X-ray Observatory and the SKA [Square Kilometer Array] Pathfinder (ASKAP) radio telescope on Wajarri Country in Australia to study the antics of the discovered object, known as ASKAP J1832−0911 (ASKAP J1832 for short).

ASKAP J1832 belongs to a class of objects called “long period radio transients” discovered in 2022 that vary in radio wave intensity in a regular way over tens of minutes. This is thousands of times longer than the length of the repeated variations seen in pulsars, which are rapidly spinning neutron stars that have repeated variations multiple times a second. ASKAP J1832 cycles in radio wave intensity every 44 minutes, placing it into this category of long period radio transients.

Using Chandra, the team discovered that ASKAP J1832 is also regularly varying in X-rays every 44 minutes. This is the first time that such an X-ray signal has been found in a long period radio transient.

In this composite image, X-rays from Chandra (blue) have been combined with infrared data from NASA’s Spitzer Space Telescope (cyan, light blue, teal and orange), and radio from LOFAR (red). An inset shows a more detailed view of the immediate area around this unusual object in X-ray and radio light.

Scientists have discovered a star behaving like no other seen before, giving new clues about the origin of a class of mysterious objects. This object, known as ASKAP J1832, shows regular changes in both radio wave and X-ray intensity every 44 minutes, the first time such variations have been seen for a class of objects discovered only three years ago. X-rays from Chandra are shown along with infrared data from the Spitzer Space Telescope, and radio from LOFAR. An inset shows a more detailed view of the immediate area around this unusual object in X-ray and radio light.
A wide field image of ASKAP J1832 in X-ray, radio, and infrared light.
X-ray: NASA/CXC/ICRAR, Curtin Univ./Z. Wang et al.; Infrared: NASA/JPL/CalTech/IPAC; Radio: SARAO/MeerKAT; Image processing: NASA/CXC/SAO/N. Wolk

Using Chandra and the SKA Pathfinder, a team of astronomers found that ASKAP J1832 also dropped off in X-rays and radio waves dramatically over the course of six months. This combination of the 44-minute cycle in X-rays and radio waves in addition to the months-long changes is unlike anything astronomers have seen in the Milky Way galaxy.

A close-up image of ASKAP J1832 in X-ray and radio light.
A close-up image of ASKAP J1832 in X-ray and radio light.
X-ray: NASA/CXC/ICRAR, Curtin Univ./Z. Wang et al.; Radio: SARAO/MeerKAT; Image processing: NASA/CXC/SAO/N. Wolk

The research team argues that ASKAP J1832 is unlikely to be a pulsar or a neutron star pulling material from a companion star because its properties do not match the typical intensities of radio and X-ray signals of those objects. Some of ASKAP J1832’s properties could be explained by a neutron star with an extremely strong magnetic field, called a magnetar, with an age of more than half a million years. However, other features of ASKAP J1832 — such as its bright and variable radio emission — are difficult to explain for such a relatively old magnetar.

On the sky, ASKAP J1832 appears to lie within a supernova remnant, the remains of an exploded star, which often contain a neutron star formed by the supernova. However, the research team determined that the proximity is probably a coincidence and two are not associated with each other, encouraging them to consider the possibility that ASKAP J1832 does not contain a neutron star. They concluded that an isolated white dwarf does not explain the data but that a white dwarf star with a companion star might. However, it would require the strongest magnetic field ever known for a white dwarf in our galaxy.

A paper by Ziteng Wang (Curtin University in Australia) and collaborators describing these results appears in the journal Nature. Another team led by Di Li from Tsinghua University in China independently discovered this source using the DAocheng Radio Telescope and submitted their paper to the arXiv on the same day as the team led by Dr Wang. They did not report the X-ray behavior described here.

NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

Learn more about the Chandra X-ray Observatory and its mission here:

https://www.nasa.gov/chandra

https://chandra.si.edu

Visual Description:

This release features two composite images of a mysterious object, possibly an unusual neutron star or white dwarf, residing near the edge of a supernova remnant. The object, known as ASKAP J1832, has been intriguing astronomers from the Chandra X-ray Observatory and Square Kilometre Array Pathfinder radio telescope with its antics and bizarre behavior.

Astronomers have discovered that ASKAP J1832 cycles in radio wave intensity every 44 minutes. This is thousands of times longer than pulsars, which are rapidly spinning neutron stars that have repeated variations multiple times a second. Using Chandra, the team discovered that the object is also regularly varying in X-rays every 44 minutes. This is the first time such an X-ray signal has been found in a long period radio transient like ASKAP J1832.

In the primary composite image of this release, the curious object is shown in the context of the supernova remnant and nearby gas clouds. Radio data is red and and X-ray sources seen with Chandra are in dark blue. The supernova remnant is the large, wispy, red oval ring occupying the lower right of the image. The curious object sits inside this ring, to our right of center; a tiny purple speck in a sea of colorful specks. The gas cloud shows infrared data from NASA’s Spitzer Space Telescope and resembles a mottled green, teal blue, and golden orange cloud occupying our upper left half of the square image.

The second, close-up image shows a view of the immediate area around ASKAP J1832. In this composite image, infrared data from Spitzer has been removed, eliminating the mottled cloud and most of the colorful background specks. Here, near the inside edge of the hazy red ring, the curious object resembles a bright white dot with a hot pink outer edge, set against the blackness of space. Upon close inspection, the hot pink outer edge is revealed to have three faint spikes emanating from the surface.

The primary and close-up images are presented both unadorned, and with labels, including fine white circles identifying ASKAP J1832.

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu

Lane Figueroa
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
lane.e.figueroa@nasa.gov

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Lee Mohon

How Do We Do Research in Zero Gravity? We Asked a NASA Expert: Episode 62

How Do We Do Research in Zero Gravity? We Asked a NASA Expert: Episode 62

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

How do we do research in zero gravity?

Actually when astronauts do experiments on the International Space Station, for instance, to environment on organisms, that environment is actually technically called microgravity. That is, things feel weightless, but we’re still under the influence of Earth’s gravity.

Now, the very microgravity that we’re trying to study up there can make experiments actually really kind of difficult for a bunch of different reasons.

First of all, stuff floats. So losing things in the ISS is a very real possibility. For example,

there was a set of tomatoes that was harvested in 2022 put it in a bag and it floated away and we couldn’t find it for eight months.

So to prevent this kind of thing from happening, we use a lot of different methods, such as using enclosed experiment spaces like glove boxes and glove bags. We use a lot of Velcro to stick stuff to.

Another issue is bubbles in liquids. So, on Earth, bubbles float up, in space they don’t float up, they’ll interfere with optical measurements or stop up your microfluidics. So space experiment equipment often includes contraptions for stopping or blocking or trapping bubbles.

A third issue is convection. So on Earth, gravity drives a process of gas mixing called convection and that helps circulate air. But without that in microgravity we worry about some of our experimental organisms and whether they’re going to get the fresh air that they need. So we might do things like adding a fan to their habitat, or if we can’t, we’ll take their habitat and put it somewhere where there might already be a fan on the ISS or in a corridor where we think they are going to be a lot of astronauts moving around and circulating the air.

Yet another issue is the fact that a lot of the laboratory instruments we use on Earth are not designed for microgravity. So to ensure that gravity doesn’t play a factor in how they work, we might do experiments on the ground where we turn them on their side or upside down, or rotate them on a rotisserie to make sure that they keep working.

So, as you can tell, for every experiment that we do on the International Space Station, there’s a whole team of scientists on the ground that has spent years developing the experiment design. And so I guess the answer to how we do research in microgravity is with a lot of practice and preparation.

[END VIDEO TRANSCRIPT]

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Emily Furfaro

Summer Students Scan the Radio Skies with SunRISE

Summer Students Scan the Radio Skies with SunRISE

A woman presents a scientific poster titled “Solar Radio Burst Events Detected by the SunRISE Ground Radio Lab” to a man at a conference. The poster includes graphs, charts, and images related to solar radio bursts, with sections labeled
L. Y. Zhou, a senior at Skyline High School, Ann Arbor, MI, representing the SunRISE Ground Radio Lab (GRL) summer research project team at the Solar Heliospheric and INterplanetary Environment (SHINE) conference, held in Juneau, AK in August 2024. Other contributing high school students were S. Rajavelu-Mohan (Washtenaw Technical Middle College, Ann Arbor, MI), M. I. Costacamps-Rivera (Centro Residencial de Oportunidades Educativas de Mayagüez, Mayagüez, PR), E. Schneider (Marquette Senior High School, Marquette, MI), and L. Cui (Skyline High School, Ann Arbor, MI).

Solar radio bursts, intense blasts of radio emission associated with solar flares, can wreak havoc on global navigation systems. Now, as part of the Ground Radio Lab campaign led by the University of Michigan and NASA’s SunRISE (Sun Radio Interferometer Space Experiment) mission, which is managed by the agency’s Jet Propulsion Laboratory in Southern California, high school and college students across the nation are collecting, processing, and analyzing space weather data to help better understand these bursts. 

Participating students have presented their findings at local science fairs and national conferences, including the Solar Heliospheric and INterplanetary Environment (SHINE) conference held in Juneau, Alaska in August 2024. These students sifted through thousands of hours of observations to identify and categorize solar radio bursts.  

Your school can get involved too! 

Participating high schools receive free, self-paced online training modules sponsored by the SunRISE mission that cover a range of topics, including radio astronomy, space physics, and science data collection and analysis. Students and teachers participate in monthly webinars with space science and astronomy experts, build radio telescopes from kits, and then use these telescopes to observe low frequency emissions from the Sun and other objects like Jupiter and the Milky Way. 

Visit the Ground Radio Lab website to learn more about the new campaign and apply to participate.

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Last Updated
May 28, 2025

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