Friday is Full of Advancing Dragon Cargo Stowage, Advanced Research, and Maintenance of Orbital Systems

Friday is Full of Advancing Dragon Cargo Stowage, Advanced Research, and Maintenance of Orbital Systems

A small part of Earth from space is shown in dark green, and the edge of the curvature is illuminated with light that diffuses into space in shades of violet and then dark blue. In the background, a portion of the Milky Way runs perpendicular to the Earth’s curvature. Many other stars dot the area surrounding the Milky Way.
A small part of Earth from space is shown in dark green, and the edge of the curvature is illuminated with light that diffuses into space in shades of violet and then dark blue. In the background, a portion of the Milky Way runs perpendicular to the Earth’s curvature. Many other stars dot the area surrounding the Milky Way.
NASA

The Expedition 73 crew aboard the International Space Station continued work with Dragon cargo, advanced space experiments, and maintenance of orbital systems.

NASA astronauts Anne McClain and Nichole Ayers with the help of JAXA (Japan Aerospace Exploration Agency) astronaut and station commander Takuya Onishi work continued building toward the undocking of the SpaceX Dragon spacecraft by stowing and transferring cargo inside the spacecraft.

Ongoing work with the Advanced Space Experiment Processor (ADSEP-4) was carried out by NASA astronaut Jonny Kim as he worked through various steps removing quadcassettes from the ADSEP-4 then replaced and retrieved the crystallizer inside of the ADSEP ICC cassette and installed the newly configured quadcassette. For historical documentation Onishi photographed Kim’s work with the ADSEP-4. Results from this new technology with the Advanced Space Experiment Processor (ADSEP-4) could demonstrate that pharmaceutical production in space can be scaled up, supporting the fabrication of materials in space for commercial applications.

Both Onishi, McClain, and Ayers worked on the Environmental Health System’s (EHS) Exploration Potable Water Dispenser. Onishi collected station water samples for in-flight and post-flight analysis. He performed a water sample analysis with focus on detecting various microbes to determine the water quality onboard the station. Meanwhile McClain and Ayers removed and replaced the Exploration Potable Water Dispenser’s controller cards and performed a checks to verify functionality.

McClain later worked to deploy the Life Sciences Glovebox (LSG) work volume and set up the Extant Life Volumetric Imaging System (ELVIS) hardware in the glovebox where she later retrieved and inserted samples from the laboratory freezer. ELVIS is a microscope for 3D imaging of objects as small as bacteria, with the goal of making the technology available to anyone studying microscopic motion in space. The technology demonstration tests the microscope by studying active behavior and genetic changes in microalgae and marine bacteria strains. The imaging technology could be used to monitor water quality, detect potentially infectious organisms, and study liquid mixtures and microorganisms in space and on Earth.

Ayers removed the sophonster container, sensor container, and the microSd card and packed it for stowage. She also inserted a sample into a box module within Minus Eighty-Degree Laboratory Freezer for ISS (MELFI) to refrigerate it. The freezer is a cold storage unit that maintains experiment samples at ultra-cold temperatures throughout a mission.

The station’s three cosmonauts Sergey Ryzhikov, Alexey Zubritskiy, and Kirill Peskov continued with more Russian segment maintenance. Ryzhikov conducted additional Russian segment inspection activities. Together Ryzhikov and Zubritskiy removed protective screens from the BTN-NEUTRON-2 which is a nuclear physics experiment located in the Russian segment that measures the neutron component of the radiation background in the near-Earth space, spatial and temporal distribution of neutron fluxes and spectra, during solar flares. Peskov continued with his work to reconfiguring and restoring the ventilation system that connects the Russian and U.S. segments.

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. Get the latest from NASA delivered every week. Subscribe here: https://www.nasa.gov/subscribe.

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Kelcie Nicole Howren

NASA’s LRO Views Japan’s RESILENCE Lunar Lander Landing Area

NASA’s LRO Views Japan’s RESILENCE Lunar Lander Landing Area

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A black and white image of the surface of the Moon taken from NASA's Lunar Reconnaissance Orbiter showing the Mare Frigoris landing site on the surface of the Moon.

NASA’s Lunar Reconnaissance Orbiter Camera (LROC) imaged the landing area of the ispace SMBC x HAKUTO-R Venture Moon Mission 2 RESILIENCE lunar lander which is slated to land on the surface of the Moon no earlier than June 5, 2025 (UTC). This view of the primary landing area is 3.13 miles (5,040 meters) wide and north is up. The site is in Mare Frigoris, a volcanic region interspersed with large-scale faults known as wrinkle ridges. Mare Frigoris formed over 3.5 billion years ago as massive basalt eruptions flooded low-lying terrain.

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May 16, 2025

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Jamie Adkins

Nancy Grace Roman’s 100th Birthday

Nancy Grace Roman’s 100th Birthday

Two people - astronaut Buzz Aldrin and Dr. Nancy Grace Roman - look at a map of celestial objects hanging on a wall in front of them. The photos is taken from the side, so their profiles are visible. Aldrin wears a dark suit and tie, while Roman wears a gray short sleeved jacket. She is pointing at a constellation on the blue and white map.
NASA

Dr. Nancy Grace Roman, NASA’s first Chief of Astronomy and namesake of the Nancy Grace Roman Telescope, briefs astronaut Edwin “Buzz” Aldrin on celestial objects in 1965 in Washington, D.C. Nancy Grace Roman passed away on December 25, 2018, in Germantown, Maryland at the age of 93. May 16, 2025, would have been her 100th birthday.

Prior to joining NASA in 1959, Dr. Roman was a well-respected and influential astronomer, publishing some of the most cited papers in the mid-20th century, one included in a list of 100 most influential papers in 100 years. At the agency, Roman worked to gain science support for space-based observatories. She established NASA’s scientific ballooning and airborne science, oversaw the start of the Great Observatory program with the first decade of Hubble Space Telescope development, and invested early in charge-coupled devices technology development used on Hubble – and now in digital cameras everywhere.  

She was also key to the decision to link the development of the Large Space Telescope (that became Hubble) and the Space Transportation System – more commonly known as the Space Shuttle. Finally, after retiring from NASA, Dr. Roman often worked with young students in underserved communities, hoping her story and mentoring could inspire them to join humanity’s quest for knowledge in a STEM field.

Learn more about Dr. Roman.

Text credit: NASA/Jackie Townsend

Image credit: NASA

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Monika Luabeya

NASA, International Astronauts Address Students from New York, Ohio

NASA, International Astronauts Address Students from New York, Ohio

Astronaut Anne McClain is pictured on May 1, 2025, near one of the International Space Station's main solar arrays.
Astronaut Anne McClain is pictured on May 1, 2025, near one of the International Space Station’s main solar arrays.
Credit: NASA

NASA astronaut Nichole Ayers and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi will answer prerecorded questions submitted by middle and high school students from New York and Ohio. Both groups will hear from the astronauts aboard the International Space Station in two separate events.

The first event at 10:20 a.m. EDT on Tuesday, May 20, includes students from Long Beach Middle School in Lido Beach, New York. Media interested in covering the event at Long Beach Middle School must RSVP no later than 5 p.m. Monday, May 19, to Christi Tursi at: ctursi@lbeach.org or 516-771-3960.

The second event at 11 a.m. EDT on Friday, May 23, is with students from Vermilion High School in Vermilion, Ohio. Media interested in covering the event at Vermilion High School must RSVP no later than 5 p.m. Thursday, May 22, to Jennifer Bengele at: jbengele@vermilionschools.org or 440-479-7783.

Watch both 20-minute Earth-to-space calls live on NASA STEM YouTube Channel.

Long Beach Middle School will host the event for students in grades 6 through 8. The school aims to provide both the students and community with an experience that bridge gaps in space sciences with teaching and learning in classrooms.

Vermilion High School will host the event for students in grades 9 through 12, to help increase student interest in science, technology, engineering, and mathematics career pathways.

For more than 24 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing skills needed to explore farther from Earth. Astronauts aboard the orbiting laboratory communicate with NASA’s Mission Control Center in Houston 24 hours a day through SCaN’s (Space Communications and Navigation) Near Space Network.

Research and technology investigations taking place aboard the space station benefit people on Earth and lay the groundwork for other agency missions. As part of NASA’s Artemis campaign, the agency will send astronauts to the Moon to prepare for future human exploration of Mars, inspiring Artemis Generation explorers and ensuring the United States continues to lead in space exploration and discovery.

See videos of astronauts aboard the space station at:

https://www.nasa.gov/stemonstation

-end-

Gerelle Dodson
Headquarters, Washington
202-358-1600
gerelle.q.dodson@nasa.gov

Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov

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Gerelle Q. Dodson

Hubble Captures Cotton Candy Clouds

Hubble Captures Cotton Candy Clouds

2 min read

Hubble Captures Cotton Candy Clouds

Part of a nebula in space. Layers of gas and dust clouds in different colors, from blue and green shades to pink, red, and black, each indicating light emitted by different molecules, comprise the nebula. The background cloud layers are thicker and puffier, though still translucent, and the upper layers are thin and bright at the edges. Behind the clouds are many small, mostly orange and some blue, stars.
This NASA/ESA Hubble Space Telescope image features a cloudscape in the Large Magellanic Cloud., a dwarf satellite galaxy of the Milky Way.
ESA/Hubble & NASA, C. Murray

This NASA/ESA Hubble Space Telescope image features a sparkling cloudscape from one of the Milky Way’s galactic neighbors, a dwarf galaxy called the Large Magellanic Cloud. Located 160,000 light-years away in the constellations Dorado and Mensa, the Large Magellanic Cloud is the largest of the Milky Way’s many small satellite galaxies.

This view of dusty gas clouds in the Large Magellanic Cloud is possible thanks to Hubble’s cameras, such as the Wide Field Camera 3 (WFC3) that collected the observations for this image. WFC3 holds a variety of filters, and each lets through specific wavelengths, or colors, of light. This image combines observations made with five different filters, including some that capture ultraviolet and infrared light that the human eye cannot see.

The wispy gas clouds in this image resemble brightly colored cotton candy. When viewing such a vividly colored cosmic scene, it is natural to wonder whether the colors are ‘real’. After all, Hubble, with its 7.8-foot-wide (2.4 m) mirror and advanced scientific instruments, doesn’t bear resemblance to a typical camera! When image-processing specialists combine raw filtered data into a multi-colored image like this one, they assign a color to each filter. Visible-light observations typically correspond to the color that the filter allows through. Shorter wavelengths of light such as ultraviolet are usually assigned blue or purple, while longer wavelengths like infrared are typically red.

This color scheme closely represents reality while adding new information from the portions of the electromagnetic spectrum that humans cannot see. However, there are endless possible color combinations that can be employed to achieve an especially aesthetically pleasing or scientifically insightful image.

Media Contact:

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

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