NASA’s SpaceX 32nd Resupply Mission Launches New Research to Station

NASA’s SpaceX 32nd Resupply Mission Launches New Research to Station

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA and SpaceX are launching the company’s 32nd commercial resupply services mission to the International Space Station later this month, bringing a host of new research to the orbiting laboratory. Aboard the SpaceX Dragon spacecraft are experiments focused on vision-based navigation, spacecraft air quality, materials for drug and product manufacturing, and advancing plant growth with less reliance on photosynthesis.

This and other research conducted aboard the space station advances future space exploration, including missions to the Moon and Mars, and provides many benefits to humanity.

Investigations traveling to the space station include:

Robotic spacecraft guidance

Smartphone Video Guidance Sensor-2 (SVGS-2) uses the space station’s Astrobee robots to demonstrate using a vision-based sensor developed by NASA to control a formation flight of small satellites. Based on a previous in-space demonstration of the technology, this investigation is designed to refine the maneuvers of multiple robots and integrate the information with spacecraft systems.

Potential benefits of this technology include improved accuracy and reliability of systems for guidance, navigation, and control that could be applied to docking crewed spacecraft in orbit and remotely operating multiple robots on the lunar or Martian surface.

Two cube-shaped robots each about the size of a small suitcase, one green and one blue, float in the middle of a module on the space station. Below them are white storage bags and behind them a wall covered with equipment, laptops, cords, and wires. A black device mounted on the wall at the left of the image has four bright blue lights.
Two of the space station’s Astrobee robots are used to test a vision-based guidance system for Smartphone Video Guidance Sensor (SVGS)
NASA

Protection from particles

During spaceflight, especially long-duration missions, concentrations of airborne particles must be kept within ranges safe for crew health and hardware performance. The Aerosol Monitors investigation tests three different air quality monitors in space to determine which is best suited to protect crew health and ensure mission success. The investigation also tests a device for distinguishing between smoke and dust. Aboard the space station, the presence of dust can cause false smoke alarms that require crew member response. Reducing false alarms could save valuable crew time while continuing to protect astronaut safety.

Better materials, better drugs

The DNA Nano Therapeutics-Mission 2 produces a special type of molecule formed by DNA-inspired, customizable building blocks known as Janus base nanomaterials. It also evaluates how well the materials reduce joint inflammation and whether they can help regenerate cartilage lost due to arthritis. These materials are less toxic, more stable, and more compatible with living tissues than current drug delivery technologies.

Environmental influences such as gravity can affect the quality of these materials and delivery systems. In microgravity, they are larger and have greater uniformity and structural integrity. This investigation could help identify the best formulations and methods for cost-effective in-space production. These nanomaterials also could be used to create novel systems targeting therapy delivery that improves patient outcomes with fewer side effects.

The image shows stem cells embedded within a network of scaffolding material. The scaffold is densely populated with cells adhered throughout. 
Stem cells grown along the Janus base nanomaterials (JBNs) made aboard the International Space Station.
University of Connecticut

Next-generation pharmaceutical nanostructures

The newest Industrial Crystallization Cassette (ADSEP-ICC) investigation adds capabilities to an existing protein crystallization facility. The cassette can process more sample types, including tiny gold particles used in devices that detect cancer and other diseases or in targeted drug delivery systems. Microgravity makes it possible to produce larger and more uniform gold particles, which improves their use in research and real-life applications of technologies related to human health.

Helping plants grow

Rhodium USAFA NIGHT examines how tomato plants respond to microgravity and whether a carbon dioxide replacement can reduce how much space-grown plants depend on photosynthesis. Because photosynthesis needs light, which requires spacecraft power to generate, alternatives would reduce energy use. The investigation also examines whether using supplements increases plant growth on the space station, which has been observed in preflight testing on Earth. In future plant production facilities aboard spacecraft or on celestial bodies, supplements could come from available organic materials such as waste.

Understanding how plants adapt to microgravity could help grow food during long-duration space missions or harsh environments on Earth.

A tan box about the size of a small microwave sits on top of a silver metal tray. The box has stickers on the top that say, “DoD Space Test Program,” “United States Air Force Academy,” and “United States Space Force.” On its front are six numbered chambers holding vials filled with a clear liquid, and more labels below them, including one that says, “Rhodium Plant Life” and a barcode.
Hardware for the Rhodium Plant LIFE, which was the first in a series used to study how space affects plant growth.
NASA

Atomic clocks in space

An ESA (European Space Agency) investigation, Atomic Clock Ensemble in Space (ACES), examines fundamental physics concepts such as Einstein’s theory of relativity using two next-generation atomic clocks operated in microgravity. Results have applications to scientific measurement studies, the search for dark matter, and fundamental physics research that relies on highly accurate atomic clocks in space. The experiment also tests a technology for synchronizing clocks worldwide using global navigation satellite networks.

An illustration of the space station fills the top two-thirds of this image, with a silver, cylindrical module in the middle. A large silver box is attached to the bottom of it. A blue, cloud-dappled Earth fills the right lower corner, with the blackness of space in the background.
An artist’s concept shows the Atomic Clock Ensemble in Space hardware mounted on the Earth-facing side of the space station’s exterior.
ESA

Download high-resolution photos and videos of the research mentioned in this article.

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Andrea Lloyd

NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise

NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise

6 Min Read

NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise

An illustration of a host star, which looks like an orange globe with flares coming out on various sides with a very transparent cloud of blue dust spread out from the star. A dark orange horizontal ring of material circles the host star.
NASA’s James Webb Space Telescope’s observations of what is thought to be the first-ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly depreciated over time, as seen in this artist’s concept. Full illustration below.
Credits:
NASA, ESA, CSA, R. Crawford (STScI)

Observations from NASA’s James Webb Space Telescope have provided a surprising twist in the narrative surrounding what is believed to be the first star observed in the act of swallowing a planet. The new findings suggest that the star actually did not swell to envelop a planet as previously hypothesized. Instead, Webb’s observations show the planet’s orbit shrank over time, slowly bringing the planet closer to its demise until it was engulfed in full.

“Because this is such a novel event, we didn’t quite know what to expect when we decided to point this telescope in its direction,” said Ryan Lau, lead author of the new paper and astronomer at NSF NOIRLab (National Science Foundation National Optical-Infrared Astronomy Research Laboratory) in Tuscon, Arizona. “With its high-resolution look in the infrared, we are learning valuable insights about the final fates of planetary systems, possibly including our own.”

Two instruments aboard Webb conducted the post-mortem of the scene – Webb’s MIRI (Mid-Infrared Instrument) and NIRSpec (Near-Infrared Spectrograph). The researchers were able to come to their conclusion using a two-pronged investigative approach.

Image A: Planetary Engulfment Illustration

A four panel illustration, with two boxes on the top row and two boxes on the bottom row. They are labeled: 1, 2, 3, 4. Panel 1 shows a host star, which looks like an orange globe with flares coming out on various sides. There is a blue line with arrows forming a spiral around the star. At 2 o’clock in the outer spiral, furthest away from the star, there is a blue planet. Panel 2 shows the same star and lines, but the planet is now at 7 o’clock and closer to the star. It is a little stretched out toward the star, appearing like an American football or rugby ball instead of a sphere. Panel 3 shows the same star and lines, but the planet is fully engulfed by the star, with big flares coming out where the planet and star collided. Panel 4 shows the aftermath, with a very transparent cloud of blue dust spread out from the star. A dark orange horizontal ring of material circles the host star.
NASA’s James Webb Space Telescope’s observations of what is thought to be the first-ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly depreciated over time, as seen in this artist’s concept.
NASA, ESA, CSA, R. Crawford (STScI)

Constraining the How

The star at the center of this scene is located in the Milky Way galaxy about 12,000 light-years away from Earth.

The brightening event, formally called ZTF SLRN-2020, was originally spotted as a flash of optical light using the Zwicky Transient Facility at the Palomar Observatory in San Diego, California. Data from NASA’s NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) showed the star actually brightened in the infrared a year before the optical light flash, hinting at the presence of dust. This initial 2023 investigation led researchers to believe that the star was more Sun-like, and had been in the process of aging into a red giant over hundreds of thousands of years, slowly expanding as it exhausted its hydrogen fuel.

However, Webb’s MIRI told a different story. With powerful sensitivity and spatial resolution, Webb was able to precisely measure the hidden emission from the star and its immediate surroundings, which lie in a very crowded region of space. The researchers found the star was not as bright as it should have been if it had evolved into a red giant, indicating there was no swelling to engulf the planet as once thought.

Reconstructing the Scene

Researchers suggest that, at one point, the planet was about Jupiter-sized, but orbited quite close to the star, even closer than Mercury’s orbit around our Sun. Over millions of years, the planet orbited closer and closer to the star, leading to the catastrophic consequence.

“The planet eventually started to graze the star’s atmosphere. Then it was a runaway process of falling in faster from that moment,” said team member Morgan MacLeod of the Harvard-Smithsonian Center for Astrophysics and the Massachusetts Institute of Technology in Cambridge, Massachusetts. “The planet, as it’s falling in, started to sort of smear around the star.”

In its final splashdown, the planet would have blasted gas away from the outer layers of the star. As it expanded and cooled off, the heavy elements in this gas condensed into cold dust over the next year.

Inspecting the Leftovers

While the researchers did expect an expanding cloud of cooler dust around the star, a look with the powerful NIRSpec revealed a hot circumstellar disk of molecular gas closer in. Furthermore, Webb’s high spectral resolution was able to detect certain molecules in this accretion disk, including carbon monoxide.

“With such a transformative telescope like Webb, it was hard for me to have any expectations of what we’d find in the immediate surroundings of the star,” said Colette Salyk of Vassar College in Poughkeepsie, New York, an exoplanet researcher and co-author on the new paper. “I will say, I could not have expected seeing what has the characteristics of a planet-forming region, even though planets are not forming here, in the aftermath of an engulfment.”

The ability to characterize this gas opens more questions for researchers about what actually happened once the planet was fully swallowed by the star.

“This is truly the precipice of studying these events. This is the only one we’ve observed in action, and this is the best detection of the aftermath after things have settled back down,” Lau said. “We hope this is just the start of our sample.”

These observations, taken under Guaranteed Time Observation program 1240, which was specifically designed to investigate a family of mysterious, sudden, infrared brightening events, were among the first Target of Opportunity programs performed by Webb. These types of study are reserved for events, like supernova explosions, that are expected to occur, but researchers don’t exactly know when or where. NASA’s space telescopes are part of a growing, international network that stands ready to witness these fleeting changes, to help us understand how the universe works.

Researchers expect to add to their sample and identify future events like this using the upcoming Vera C. Rubin Observatory and NASA’s Nancy Grace Roman Space Telescope, which will survey large areas of the sky repeatedly to look for changes over time.

The team’s findings appear today in The Astrophysical Journal.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

To learn more about Webb, visit: https://science.nasa.gov/webb

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View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.

View/Download the science paper from the The Astrophysical Journal.

Media Contacts

Laura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Hannah Braunhbraun@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Related Information

Read more about Webb’s impact on exoplanet research

Video: How to Study Exoplanets

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Webb Mission Page

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NASA Offers Free High School Engineering Program This Summer

NASA Offers Free High School Engineering Program This Summer

This summer, NASA’s Glenn Research Center in Cleveland is offering a free summer STEM program for high school students in their junior and senior years.
Credit: NASA

NASA’s Glenn Research Center in Cleveland is launching the NASA Glenn High School Engineering Institute this summer. The free, work-based learning experience is designed to help high school students prepare for a future in the aerospace workforce.

Rising high school juniors and seniors in Northeast Ohio can submit applications for this new, in-person summer program from Friday, April 11, through Friday, May 9.

The NASA Glenn High School Engineering Institute will immerse students in NASA’s work while providing essential career readiness tools to help them in future science, technology, engineering, and mathematics-focused academic and professional pursuits.

Throughout the five-day institute, students will use authentic NASA mission content and work alongside Glenn’s technical experts to gain a deeper understanding of the engineering design process, develop practical engineering solutions to real-world challenges, and test prototypes to answer questions in key mission areas:

  • Acoustic dampening – How can we reduce noise pollution from jet engines?
  • Power management and distribution – How can we develop a smart power system for future space stations?
  • Simulated lunar operations – Can we invent tires that don’t use air?

Program Dates
Selected students will participate in one of the following week-long sessions.

  • Session 1: July 7 – 11, 2025
  • Session 2: July 14 – 18, 2025
  • Session 3: July 21 – 25, 2025

Eligibility and Application Requirements
To be eligible for this program, students must:

  • Be entering 11th or 12th grade for the 2025-2026 academic year
  • Have a minimum 3.2 GPA, verified by their school counselor
  • Submit a letter of recommendation from a teacher

Additional application requirements are outlined in the Supplemental Application.

How to Apply:
To be considered for this opportunity, complete and submit the NASA Gateway application and the Supplemental Application by Friday May 9.

Questions pertaining to the NASA Glenn High School Engineering Institute should be directed to Gerald Voltz at GRC-Ed-Opportunities@mail.nasa.gov.

For information about NASA Glenn, visit:

https://www.nasa.gov/glenn

-end-

Debbie Welch
Glenn Research Center, Cleveland
216-433-8655
debbie.welch@nasa.gov

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Kelly M. Matter

NASA’s Juno Back to Normal Operations After Entering Safe Mode

NASA’s Juno Back to Normal Operations After Entering Safe Mode

3 min read

NASA’s Juno Back to Normal Operations After Entering Safe Mode

This illustration depicts NASA's Juno spacecraft in orbit above Jupiter's Great Red Spot.
NASA’s Juno flies above Jupiter’s Great Red Spot in this artist’s concept.
NASA/JPL-Caltech

The spacecraft was making its 71st close approach to Jupiter when it unexpectedly entered into a precautionary status.

Data received from NASA’s Juno mission indicates the solar-powered spacecraft went into safe mode twice on April 4 while the spacecraft was flying by Jupiter. Safe mode is a precautionary status that a spacecraft enters when it detects an anomaly. Nonessential functions are suspended, and the spacecraft focuses on essential tasks like communication and power management. Upon entering safe mode, Juno’s science instruments were powered down, as designed, for the remainder of the flyby.

The mission operations team has reestablished high-rate data transmission with Juno, and the spacecraft is currently conducting flight software diagnostics.The team will work in the ensuing days to transmit the engineering and science data collected before and after the safe-mode events to Earth.

Juno first entered safe mode at 5:17 a.m. EDT, about an hour before its 71st close passage of Jupiter — called perijove. It went into safe mode again 45 minutes after perijove. During both safe-mode events, the spacecraft performed exactly as designed, rebooting its computer, turning off nonessential functions, and pointing its antenna toward Earth for communication.

Of all the planets in our solar system, Jupiter is home to the most hostile environment, with the radiation belts closest to the planet being the most intense. Early indications suggest the two Perijove 71 safe-mode events occurred as the spacecraft flew through these belts. To block high-energy particles from impacting sensitive electronics and mitigate the harmful effects of the radiation, Juno features a titanium radiation vault.

Including the Perijove 71 events, Juno has unexpectedly entered spacecraft-induced safe mode four times since arriving at Jupiter in July 2016: first, in 2016 during its second orbit, then in 2022 during its 39th orbit. In all four cases, the spacecraft performed as expected and recovered full capability.

Juno’s next perijove will occur on May 7 and include a flyby of the Jovian moon Io at a distance of about 55,300 miles (89,000 kilometers).

More About Juno

NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. The Italian Space Agency (ASI) funded the Jovian InfraRed Auroral Mapper. Lockheed Martin Space in Denver built and operates the spacecraft. Various other institutions around the U.S. provided several of the other scientific instruments on Juno.

More information about Juno is available at:

https://www.nasa.gov/juno

News Media Contacts

DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov

Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov

Deb Schmid
Southwest Research Institute, San Antonio
210-522-2254
dschmid@swri.org

2025-049

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Apr 09, 2025

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Cardiovascular Research Underway as New Crew Gets Used to Station Life

Cardiovascular Research Underway as New Crew Gets Used to Station Life

NASA astronaut and Expedition 72 Flight Engineer Jonny Kim enters the International Space Station shortly after docking to the Prichal module aboard the Soyuz MS-27 spacecraft. Kim is greeted by station Commander Alexey Ovchinin of Roscosmos (at left) and flight engineer Don Pettit of NASA (at right).
NASA astronaut Jonny Kim enters the International Space Station shortly after docking to the Prichal module aboard the Soyuz MS-27 spacecraft. Kim is greeted by Expedition 72 crew members welcoming him aboard the orbital outpost.
NASA

Ten residents are living aboard the International Space Station today following the arrival of a NASA astronaut and two Roscosmos cosmonauts on Tuesday. The new Expedition 72 crewmates are beginning an eight-month research mission in low Earth orbit and getting used to life in microgravity.

New station flight engineers Jonny Kim of NASA and Sergey Ryzhikov and Alexey Zubritsky, both from Roscosmos, are in their second day aboard the orbital outpost. They arrived aboard the Soyuz MS-27 spacecraft docking to the Prichal module at 4:57 a.m. EDT on Tuesday after a three-hour, ten-minute trip that began with a lift off from Kazakhstan.

The new trio will spend the next several days getting up to speed with space station systems, orbital safety procedures, and living and working in weightlessness. On Wednesday, they joined the other seven orbiting crew members and reviewed roles and responsibilities in the unlikely event of an emergency such as a fire or pressure and chemical leaks. Kim, on his first spaceflight, also got to work checking life support gear and servicing spacesuit batteries. Ryzhikov, a veteran cosmonaut on his third station mission, and first-time space flyer Zubritsky partnered together wearing sensors measuring how blood flows from the head to the limbs and back. Scientists will use the data to understand how living long-term in microgravity affects the cardiovascular system and protect crews living in space.

The other space station residents kept up ongoing advanced space research and lab maintenance. Flight Engineers Don Pettit, Anne McClain, and Nichole Ayers, all three from NASA, and Takuya Onishi of JAXA (Japan Aerospace Exploration Agency) took turns on Wednesday for scanning each other’s neck, shoulder, and leg veins using the Ultrasound 2 device. McClain also trained to use virtual reality gear while Onishi tested the operations of a free-flying, spherical robot camera. Ayers wore electrodes for another experiment monitoring how blood flows from the brain to the heart. Pettit loaded items for stowage inside a decommissioned life support rack.

Station Commander Alexey Ovchinin and Flight Engineers Ivan Vagner and Kirill Peskov of Roscosmos trained to use the lower body negative pressure suit that may prevent space-caused head and pressure. The specialized suit may also help crews quickly readjust to Earth’s gravity after living in space for months or years at a time. Ovchinin also participated in the circulatory system study with Ryzhikov and Zubritsky. Vagner explored how spaceflight affects fungus cell cultures for a Roscosmos biotechnology experiment. Kirill focused on life support maintenance collecting drinking water samples for analysis.

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