Dragon Counts Down to Launch to Resupply Space Station

Dragon Counts Down to Launch to Resupply Space Station

A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands in a vertical position at Launch Complex 39A at NASA’s Kennedy Space Center in Florida on Monday, April 21, in preparation for the 32nd commercial resupply services launch to the International Space Station.
A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands in a vertical position at Launch Complex 39A at NASA’s Kennedy Space Center in Florida on April 21, 2024.
SpaceX

Live launch coverage is underway on NASA+, Amazon Prime, and the agency’s YouTube channel for the launch of SpaceX’s 34th commercial resupply services mission to the International Space Station for the agency. Learn how to watch NASA content through a variety of online platforms, including social media.

The SpaceX Dragon spacecraft is scheduled to lift off at 6:05 p.m. EDT aboard a Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida.

Filled with nearly 6,500 pounds of food, supplies, and equipment, Dragon will arrive at the orbiting outpost at approximately 7 a.m. Sunday, May 17, and dock autonomously to the forward port of the orbiting laboratory’s Harmony module.

In addition to cargo for the crew aboard the space station, Dragon will deliver several new experiments, including a project to determine how well Earth-based simulators mimic microgravity conditions, a bone scaffold made from wood that could produce new treatments for fragile bone conditions like osteoporosis, and equipment to help researchers evaluate how red blood cells and the spleen change in space. The Dragon spacecraft also will carry a new instrument to study charged particles around Earth that can impact power grids and satellites, an investigation that could provide a fundamental understanding of how planets form, and an instrument designed to take highly accurate measurements of sunlight reflected by Earth and the Moon.

Watch NASA’s live rendezvous and docking coverage beginning at 5:30 a.m. on NASA+, Amazon Prime, and the agency’s YouTube channel.

Learn more about space station operations by follow @NASASpaceOps and @space_station on X, as well as the International Space Station’s Facebook and Instagram accounts.

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Mark A. Garcia

Dragon Nears Launch as Crew Works Biomedical Science and Spacewalk Preps

Dragon Nears Launch as Crew Works Biomedical Science and Spacewalk Preps

A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands in a vertical position at Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida on Wednesday, May 13, 2026, in preparation for the company’s 34th commercial resupply services launch to the International Space Station for NASA. Dragon will deliver about 6,500 pounds of science investigations, supplies, and equipment to the International Space Station. NASA and SpaceX are targeting liftoff at 6:50 p.m. EDT, Wednesday May 13.
A SpaceX Falcon 9 rocket, with the company’s Dragon spacecraft atop, stands at Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida on Wednesday, May 13, 2026, in preparation for launch to the International Space Station.
SpaceX

A SpaceX Falcon 9 rocket, with a cargo-packed Dragon spacecraft atop, stands ready to launch to the International Space Station at 6:05 p.m. EDT today, weather permitting, from Launch Complex 40 at Cape Canaveral Space Force Station in Florida. Watch NASA’s live launch coverage beginning at 5:45 p.m. on NASA+Amazon Prime, and the agency’s YouTube channel.

The uncrewed Dragon, packed with about 6,500 pounds of science experiments, crew supplies, and lab hardware for the Expedition 74 crew, will approach the orbital outpost for an automated docking to the Harmony module’s forward port at 7:05 a.m. on Sunday. Flight engineers Jack Hathaway of NASA and Sophie Adenot of ESA (European Space Agency) will be on duty Sunday morning monitoring Dragon during its approach and rendezvous with the space station.

Hathaway and Adenot joined NASA flight engineer Jessica Meir midday on Friday and had a brief science conference with researchers on the ground. The trio discussed the numerous experiments taking place aboard the orbiting lab and how the research benefits humans living on and off the Earth. At the beginning of his shift, Hathaway finalized the installation of new science module in the Cold Atom Lab quantum physics research facility. Adenot recorded a pair of video messages for ESA, her home space agency, targeting international scientists and French students.

NASA flight engineer Chris Williams spent his day on lab maintenance first inspecting and cleaning hatch seals. Williams wrapped up his shift checking out the operation of the Ultrasound 3 biomedical device and its components, including computer cables and probes.

Mier followed up Williams’ inspection work by installing hatch seal covers to protect them from damage and stains. She also staged cargo that will be packed inside the Dragon after its arrival for return to Earth next month.

Station commander Sergey Kud-Sverchkov and flight engineer Sergey Mikaev, both from Roscosmos, took turns at the beginning of their shift wearing heart sensors and testing their arm strength for a standard fitness assessment. Next, the duo worked on a pair of Orlan spacesuits ensuring their components were properly installed, checking their functionality, and staging them inside the Poisk module’s airlock.

Roscosmos flight engineer Andrey Fedyaev spent his shift on a pair of human research studies exploring how microgravity affects a crew member’s blood flow and orientation. For his first experiment, Fedyaev wore arm, wrist, and finger cuffs that measured his blood pressure. The biomedical data helps doctors monitor how living in space affects blood flow, clot prevention, and inflammation responses. Next, he wore a virtual reality headset then responded to computerized stimuli as electrodes measured his brain activity and eye movement tracking his sense of direction, movement, and position in weightlessness.

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

Curiosity Shakes Loose a Pesky Rock

Curiosity Shakes Loose a Pesky Rock

A large, reddish-brown rock as seen by NASA's Curiosity Mars rover. The rock is broken into several pieces. A drill hole is visible in the top middle piece.
NASA/JPL-Caltech/MSSS

After NASA’s Curiosity Mars rover drilled a sample from this rock on April 25, 2026, it withdrew its robotic arm and pulled the entire rock off the surface with it. Engineers spent several days repositioning the arm and vibrating the drill to try and get the rock loose. When it finally detached on May 1, the rock broke into pieces.

This close-up image of the rock was produced by Curiosity’s Mast Camera, or Mastcam, on May 6. Nicknamed “Atacama,” the rock is estimated to be 1.5 feet in diameter at its base and 6 inches thick. It would weigh roughly 28.6 pounds on Earth (and about a third of that on Mars). The circular hole produced by Curiosity’s drill is visible in the rock.

See Atacama stuck on Curiosity’s drill.

Credit: NASA/JPL-Caltech/MSSS

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HQ Web Team

Hubble Sights Galaxy in Transition

Hubble Sights Galaxy in Transition

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Hubble Sights Galaxy in Transition

This Hubble image is of a bright lenticular galaxy (NGC 1266) seen nearly face on. Broad bright and dimmer areas of light hint at spiral structure, but there are no distinct spiral arms. Rusty-reddish-brown dust bisects the galaxy. More distant galaxies dot the black background, some even shining through the less dense regions of the bright foreground lenticular galaxy.
This NASA Hubble Space Telescope images reveals the lenticular galaxy, NGC 1266. This enigmatic post-starburst galaxy has a bright center and a face that hints at spiral structure, yet it holds no discernable spiral arms.
NASA, ESA, K. Alatalo (STScI); Image Processing: G. Kober (NASA/Catholic University of America)

This NASA Hubble Space Telescope image reveals an enigmatic galaxy with a bright center and a face that hints at spiral structure, yet it holds no obvious spiral arms. Reddish-brown clumps and filaments of dust partially obscure the galaxy’s full face, while red, blue, and orange light from distant galaxies shines through its diffuse outer regions and dots the inky-black background.

NGC 1266 is a lenticular galaxy located some 100 million light-years away in the constellation Eridanus (the Celestial River). Astronomers classify lenticulars as transitional galaxies that represent an evolutionary bridge between spirals and ellipticals. Lenticulars are “lens-shaped” and have a bright central bulge and flattened disk like spirals, but they have no spiral arms and little to no star formation like ellipticals.

As interesting as this galaxy’s structure and lenticular classification are, those traits aren’t its most intriguing features. NGC 1266 is a rare post-starburst galaxy that is in transition between a galaxy that experienced a major burst of star formation and a quieter elliptical galaxy. Post-starburst galaxies have a young population of stars but few star-forming regions. Roughly one percent of the local galaxy population is a post-starburst galaxy.

Astronomers think that NGC 1266 had a minor merger with another galaxy some 500 million years ago. The merger spurred the formation of new stars and increased the mass of the galaxy’s central bulge while funneling gas into its supermassive black hole. The additional matter made the black hole much more active, creating an active galactic nucleus or AGN. The black hole’s increased activity would have generated powerful winds and jets of gas along its axis of rotation. Over time, the burst of new stars and the black hole’s powerful jets would deplete the galaxy’s reservoir of star-forming gas, while the turbulence generated in these processes suppressed new stars from forming in the gas that remained.

Observations by Hubble and other observatories reveal a strong outflow of gas from the galaxy and that the space between its stars is shocked or highly disturbed. Researchers found that any remaining stellar nurseries are in the core of the galaxy, and that very little to no star formation happens beyond that core. These observations suggest the supermassive black hole in the galaxy’s heart may be suppressing star birth by stripping or ejecting star-forming gas from the galaxy. The shockwaves from this process would create turbulence that disturbs the gas and dust between stars enough to stop any remaining matter from gravitationally condensing into infant stars.

Post-starburst galaxies like NGC 1266 are ideal subjects for astronomers to study the complex physical processes that suppress star formation. They help us better understand the evolution of galaxies and how supermassive black holes interact with their hosts.

Media Contact:

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

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Picturing Earth in a New Light

Picturing Earth in a New Light

A global map shows changes in artificial light at night from 2014 to 2022, with increases shown in yellow and orange and decreases shown in purple.
Some parts of the planet are shown to brighten (gold) and some dim (purple) in an analysis of nearly a decade of nighttime lights data from NASA’s Black Marble product.
NASA Earth Observatory/Michala Garrison

Maps can show more than just where things are—they can also show how things change. New maps of artificial light reveal a planet that has been reshaping its nights through patterns of brightening and dimming.

The maps are based on a recent analysis of NASA’s Black Marble data, which found that instead of a gradual increase in artificial light at night over the course of nearly a decade, the patterns are much more nuanced. The analysis portrays a world flickering with industrial booms and busts, construction, and blackouts, as well as more gradual shifts, such as policy-driven retrofits.

NASA’s Black Marble product uses observations from the VIIRS (Visible Infrared Imaging Radiometer Suite) sensors on the Suomi-NPP, NOAA-20, and NOAA-21 satellites to produce records of nighttime lights at daily, monthly, and yearly time scales. The VIIRS day-night band detects nighttime light in a range of wavelengths from green to near-infrared and uses filtering techniques to observe signals such as city lights, reflected moonlight, and auroras.

The map above shows changes in brightness across most of the inhabited world (between 60 degrees south and 70 degrees north). Yellow and gold areas are where there has been more brightening during the study period, from 2014 to 2022, and purple areas are where there has been more dimming.  

The visualization below shows the same data for the Eastern Hemisphere. Note that this version includes some artistic touches, such as simulated sunlight and shadows, while the nighttime lights data overlaid on the globe remain grounded in the scientific analysis. The image was featured on the cover of Nature, where the study was published in April 2026.

A data visualization shows changes in artificial light at night across the Eastern Hemisphere from 2014 to 2022, with increases shown in yellow and orange and decreases shown in purple.
An analysis of nearly a decade of nighttime lights data (2014-2022) from NASA’s Black Marble product revealed areas of brightening (gold) and dimming (purple) shown here across the Eastern Hemisphere.
NASA Earth Observatory/Michala Garrison

Overall, the researchers found that global radiance increased by 34 percent during the study period, but that surge masks large areas of dimming. Such “bidirectional changes” often happen side by side. In the U.S., for example, West Coast cities grew brighter as their populations increased, while much of the East Coast showed dimming, which the team attributed to the increased use of energy-efficient LEDs and broader economic restructuring.

The authors concluded that internationally, nighttime light surged in China and northern India along with urban development, while LEDs and energy conservation measures coincided with reduced light pollution in Paris and throughout France (a 33 percent dimming), the UK (22 percent dimming), and the Netherlands (21 percent dimming). European nights dimmed sharply in 2022 during a regional energy crisis that followed the outbreak of the Russia-Ukraine conflict.

Large versions of the maps on this page can be downloaded below. Animations showing annual changes in nighttime lights throughout the study period are available from NASA’s Scientific Visualization Studio.

NASA Earth Observatory images by Michala Garrison, using data from Li, T., et al. (2026). Story by Sally Younger adapted for Earth Observatory by Kathryn Hansen.

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