Friday, February 20, 2026

Sierra Space Dream Chaser Completes Tow Testing | NASA's Kennedy Space Center

Sierra Space Dream Chaser Completes Tow Testing | NASA's Kennedy Space Center

During tow testing at KSC and Space Florida’s Launch and Landing Facility, a Freightliner Cascadia truck towed Dream Chaser at high speeds to simulate critical dynamics and validate autonomous navigational parameters.

Dream Chaser also successfully demonstrated the ability to receive telemetry and distribute commands between the spacecraft and Mission Control in Louisville, Colorado over NASA’s Tracking and Data Relay Satellite System network.  

The testing campaign concluded with a post landing recovery rehearsal.

Learn more: https://www.sierraspace.com/press-releases/sierra-spaces-dream-chaser-spaceplane-successfully-completes-critical-pre-flight-milestones/


Video Credit: Sierra Space
Duration: 4 minutes, 38 seconds
Release Date: Feb. 20, 2026


#NASA #Space #ISS #CommercialCargo #CRS #SierraSpace #DreamChaser #ReusableSpacecraft #DreamChaserSpacecraft #CargoSpacecraft #Tenacity #VulcanCentaurRocket #ULA #Spaceflight #Science #SpaceTechnology #Engineering #CommercialSpace #KSC #NASAKennedy #MerrittIsland #Florida #UnitedStates #STEM #Education #HD #Video

A Tour of Nearby Spiral Galaxy NGC 5134 in Virgo | Webb Telescope

A Tour of Nearby Spiral Galaxy NGC 5134 in Virgo | Webb Telescope

Two powerful instruments of the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope joined forces to create this scenic galaxy view. This spiral galaxy is named NGC 5134, and it is located 65 million light-years away in the constellation Virgo.

Though 65 million light-years may seem like a huge distance—the light that Webb collected to create this image has been journeying to us from NGC 5134 since soon after Tyrannosaurus rex went extinct—NGC 5134 is fairly close by as far as galaxies go. Due to the galaxy’s relative proximity, Webb can spot incredible details in its tightly wound spiral arms.

Webb’s Mid-InfraRed Instrument (MIRI) collects the mid-infrared light emitted by the warm dust that speckles NGC 5134’s interstellar clouds, tracing clumps and strands of dusty gas. Part of the dust is composed of complex organic molecules called polycyclic aromatic hydrocarbons, featuring interconnected rings of carbon atoms and provide a way for astronomers to study the chemistry happening in interstellar clouds. Webb’s Near-InfraRed Camera (NIRCam) records shorter-wavelength near-infrared light, mostly from the stars and star clusters that dot the galaxy’s spiral arms.

Together, the MIRI and NIRCam data paint a portrait of a galaxy in constant ebb and flow. The gas clouds that billow along NGC 5134’s spiral arms are the sites of star formation, and each star that forms chips away at the galaxy’s supply of star-forming gas. When stars die, they recycle part of that gas back into the galaxy. Massive stars more than about eight times the mass of the Sun do so spectacularly, in cataclysmic supernova explosions that spread stellar material across hundreds of light-years.

Stars like the Sun give back a portion of their material as well, though more gently; these stars will balloon into bubbling red giants before shrugging off their atmospheres and sending them into space. Whether expelled by explosive supernovae or gentle red giants, this gas can then be incorporated into new stars.


Credits: ESA/Webb, NASA & CSA, A. Leroy
Directed by: Bethany Downer and Nico Bartmann
Editing: Nico Bartmann
Written by: Bethany Downer
Footage and photos: ESA/Webb, NASA & CSA, A. Leroy, N. Bartmann (ESA/Webb)
Duration: 1 minute
Release Date: Feb. 20, 2026

#NASA #Astronomy #Space #Science #Galaxy #NGC5134 #VirgoConstellation #Cosmos #Universe #JWST #NIRCam #MIRI #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

Close-up: Nearby Spiral Galaxy NGC 5134 in Virgo | Webb Telescope

Close-up: Nearby Spiral Galaxy NGC 5134 in Virgo | Webb Telescope

Two powerful instruments of the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope joined forces to create this scenic galaxy view. This spiral galaxy is named NGC 5134, and it is located 65 million light-years away in the constellation Virgo.

Though 65 million light-years may seem like a huge distance—the light that Webb collected to create this image has been journeying to us from NGC 5134 since soon after Tyrannosaurus rex went extinct—NGC 5134 is fairly close by as far as galaxies go. Due to the galaxy’s relative proximity, Webb can spot incredible details in its tightly wound spiral arms.

Webb’s Mid-InfraRed Instrument (MIRI) collects the mid-infrared light emitted by the warm dust that speckles NGC 5134’s interstellar clouds, tracing clumps and strands of dusty gas. Part of the dust is composed of complex organic molecules called polycyclic aromatic hydrocarbons, featuring interconnected rings of carbon atoms and provide a way for astronomers to study the chemistry happening in interstellar clouds. Webb’s Near-InfraRed Camera (NIRCam) records shorter-wavelength near-infrared light, mostly from the stars and star clusters that dot the galaxy’s spiral arms.

Together, the MIRI and NIRCam data paint a portrait of a galaxy in constant ebb and flow. The gas clouds that billow along NGC 5134’s spiral arms are the sites of star formation, and each star that forms chips away at the galaxy’s supply of star-forming gas. When stars die, they recycle part of that gas back into the galaxy. Massive stars more than about eight times the mass of the Sun do so spectacularly, in cataclysmic supernova explosions that spread stellar material across hundreds of light-years.

Stars like the Sun give back a portion of their material as well, though more gently; these stars will balloon into bubbling red giants before shrugging off their atmospheres and sending them into space. Whether expelled by explosive supernovae or gentle red giants, this gas can then be incorporated into new stars.

This give and take between gas and stars is the focus of the observing program (#3707). It aims to study 55 galaxies in the nearby Universe that are actively forming new stars and have been studied across a broad range of wavelengths. The new Webb data contribute a rich understanding of individual star clusters and star-forming clouds and have already been used to study the life cycle of tiny dust grains, the shape and properties of star-forming clouds, the links between interstellar gas and dust, and how newly formed stars reshape their surrounding environment.

Image Description: A spiral galaxy, seen tilted diagonally. It has a blue-white, glowing spot at its core. Its oval-shaped disc glows faintly blue throughout with light from its many stars. The disc is filled with waves and strands of bright red dust that swirl around the core. At places there are holes torn in the dust, while elsewhere it forms dense clumps that glow orange. Several tiny, distant galaxies appear across the background.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Duration: 30 seconds
Release Date: Feb. 20, 2026

#NASA #Astronomy #Space #Science #Galaxy #NGC5134 #VirgoConstellation #Cosmos #Universe #JWST #NIRCam #MIRI #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education #HD #Video

The Stellar Lifecycle in Nearby Spiral Galaxy NGC 5134 | Webb Telescope

The Stellar Lifecycle in Nearby Spiral Galaxy NGC 5134 | Webb Telescope

Two powerful instruments of the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope joined forces to create this scenic galaxy view. This spiral galaxy is named NGC 5134, and it is located 65 million light-years away in the constellation Virgo.

Though 65 million light-years may seem like a huge distance—the light that Webb collected to create this image has been journeying to us from NGC 5134 since soon after Tyrannosaurus rex went extinct—NGC 5134 is fairly close by as far as galaxies go. Due to the galaxy’s relative proximity, Webb can spot incredible details in its tightly wound spiral arms.

Webb’s Mid-InfraRed Instrument (MIRI) collects the mid-infrared light emitted by the warm dust that speckles NGC 5134’s interstellar clouds, tracing clumps and strands of dusty gas. Part of the dust is composed of complex organic molecules called polycyclic aromatic hydrocarbons, featuring interconnected rings of carbon atoms and provide a way for astronomers to study the chemistry happening in interstellar clouds. Webb’s Near-InfraRed Camera (NIRCam) records shorter-wavelength near-infrared light, mostly from the stars and star clusters that dot the galaxy’s spiral arms.

Together, the MIRI and NIRCam data paint a portrait of a galaxy in constant ebb and flow. The gas clouds that billow along NGC 5134’s spiral arms are the sites of star formation, and each star that forms chips away at the galaxy’s supply of star-forming gas. When stars die, they recycle some of that gas back into the galaxy. Massive stars more than about eight times the mass of the Sun do so spectacularly, in cataclysmic supernova explosions that spread stellar material across hundreds of light-years.

Stars like the Sun give back a portion of their material as well, though more gently; these stars will balloon into bubbling red giants before shrugging off their atmospheres and sending them into space. Whether expelled by explosive supernovae or gentle red giants, this gas can then be incorporated into new stars.

This give and take between gas and stars is the focus of the observing program (#3707). It aims to study 55 galaxies in the nearby Universe that are actively forming new stars and have been studied across a broad range of wavelengths. The new Webb data contribute a rich understanding of individual star clusters and star-forming clouds and have already been used to study the life cycle of tiny dust grains, the shape and properties of star-forming clouds, the links between interstellar gas and dust, and how newly formed stars reshape their surrounding environment.

Image Description: A spiral galaxy, seen tilted diagonally. It has a blue-white, glowing spot at its core. Its oval-shaped disc glows faintly blue throughout with light from its many stars. The disc is filled with waves and strands of bright red dust that swirl around the core. At places there are holes torn in the dust, while elsewhere it forms dense clumps that glow orange. Several tiny, distant galaxies appear across the background.


Credit: ESA/Webb, NASA & CSA, A. Leroy
Release Date: Feb. 20, 2026

#NASA #Astronomy #Space #Science #Galaxy #NGC5134 #VirgoConstellation #Cosmos #Universe #JWST #NIRCam #MIRI #InfraredAstronomy #SpaceTelescopes #GSFC #STScI #UnitedStates #ESA #Europe #CSA #Canada #STEM #Education

Thursday, February 19, 2026

Dwarf Galaxies NGC 147 & NGC 185 in Cassiopeia

Dwarf Galaxies NGC 147 & NGC 185 in Cassiopeia

Dwarf galaxies NGC 147 (left) and NGC 185 stand side by side in this deep telescopic portrait. The two are not-often-imaged satellite galaxies of M31, the great spiral Andromeda Galaxy, about 2.5 million light-years away. Their separation in the sky, less than one degree across a pretty field of view toward the constellation Cassiopeia, translates to only about 35 thousand light-years at Andromeda's distance, but Andromeda itself is found well outside this frame. Brighter and more famous satellite galaxies of Andromeda, M32 and M110, are seen much closer to the great spiral. NGC 147 and NGC 185 have been identified as binary galaxies, forming a gravitationally stable binary system. However, the recently discovered faint dwarf galaxy Cassiopeia II also seems to be part of their system, forming a gravitationally bound group within Andromeda's intriguing population of small satellite galaxies.


Image Credit & Copyright: Chuck Ayoub
Chuck's website:
https://www.youtube.com/chucksastrophotography
Release Date: February 13, 2026

#NASA #Astronomy #Space #Science #Galaxies #NGC147 #NGC185 #CassiopeiaConstellation #AndromedaGalaxy #Messier31 #M31 #Cosmos #Universe #Astrophotography #ChuckAyoub #Astrophotographers #STEM #Education #APoD

Globular Star Cluster NGC 1854 in The Large Magellanic Cloud | Hubble

Globular Star Cluster NGC 1854 in The Large Magellanic Cloud | Hubble


This NASA/European Space Agency Hubble Space Telescope image shows the globular cluster NGC 1854, a gathering of white and blue stars in the southern constellation of Dorado (The Dolphinfish). NGC 1854 is located about 135,000 light-years away, in the Large Magellanic Cloud (LMC), one of our closest cosmic neighbors and a satellite galaxy of the Milky Way.

The LMC is a hotbed of vigorous star formation. Rich in interstellar gas and dust, the galaxy is home to approximately 60 globular clusters and 700 open clusters. These clusters are frequently the subject of astronomical research, as the Large Magellanic Cloud and its little sister, the Small Magellanic Cloud, are the only systems known to contain clusters at all stages of evolution. Hubble is often used to study these clusters as its extremely high-resolution cameras can resolve individual stars, even at the clusters’ crowded cores, revealing their mass, size and degree of evolution.


Credit: ESA/Hubble & NASA
Release Date: June 20, 2016


#NASA #ESA #Astronomy #Space #Science #Stars #StarClusters #GlobularClusters #NGC1854 #DoradoConstellation #Galaxies #LMC #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

Sights to See on Orbital Maneuvers | International Space Station

Sights to See on Orbital Maneuvers | International Space Station

Former Expedition 74 flight engineer Zena Cardman and NASA astronaut: "The International Space Station rarely makes big changes to its orientation, but we were lucky to experience such maneuvers (flipping around to fly butt-first, then flipping back again) before and after each SpaceX CRS-33 reboost. This 60x speed timelapse was one of my favorites since it captures a little of everything—sunset, lightning storms, air glow, moon glint, stars, and sunrise—as we did one (actually very slow) orbital cartwheel from Atlantic to Pacific."


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Video Credit: NASA's Johnson Space Center, Z. Cardman
Duration: 51 seconds
Release Date: Feb. 19, 2026

#NASA #Space #ISS #SpaceX #CargoDragonSpacecraft #CRS33 #Astronauts #ZenaCardman #AstronautVideography #UnitedStates #Japan #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #STEM #Education #HD #Video

Orion's Cradle: Stellar Nurseries

Orion's Cradle: Stellar Nurseries

Cradled in red-glowing hydrogen gas, stars are being born in Orion. These stellar nurseries lie at the edge of the giant Orion molecular cloud complex, some 1,500 light-years away. This detailed view spans about 12 degrees across the center of the well-known constellation, with the Great Orion Nebula, the closest large star-forming region, visible toward the lower right. The deep mosaic also includes, near the top center, the Flame Nebula and the Horsehead Nebula. Image data acquired with a hydrogen-alpha filter adds other remarkable features to this wide-angle cosmic vista: pervasive tendrils of energized atomic hydrogen gas and portions of the surrounding Barnard's Loop.

While the Orion Nebula and many stars in Orion are easy to see with the unaided eye, emission from the extensive interstellar gas is faint and much harder to record, even in telescopic views of the nebula-rich complex.


Image Credit & Copyright: Piotr Czerski
Piotr's website: 

#NASA #Astronomy #Space #Science #Stars #Nebulae #StellarNurseries #FlameNebula #NGC2024 #HorseheadNebula #Barnard33 #GreatOrionNebula #BarnardsLoop #Messier78 #OrionConstellation #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #PiotrCzerski #Astrophotographer #CitizenScience #STEM #Education #APoD

Orbital Sunset through the 'Eye of a Dragon' | International Space Station

Orbital Sunset through the 'Eye of a Dragon' | International Space Station

NASA astronaut Don Pettit shared this photo. He returned to Earth on April 19, 2025, concluding a seven-month science mission aboard the International Space Station. Pettit spent 220 days in space, earning him a total of 590 days in space over the course of his four spaceflights. He orbited the Earth 3,520 times, traveling 93.3 million miles in low-Earth orbit.

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

Image Credit: NASA's Johnson Space Center
Release Date: Feb. 17, 2026

#NASA #Space #Astronomy #Science #ISS #Sun #Sunset #SpaceX #DragonSpacecraft #Planets #Earth #Astronauts #DonPettit #AstronautPhotography #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education

Planet Uranus: Auroral Activity | James Webb Space Telescope

Planet Uranus: Auroral Activity | James Webb Space Telescope

Uranus (January 2025)
Two bright auroral bands were detected near Uranus’s magnetic poles, together with reduced emission and ion density in part of the region between the two bands (a feature likely linked to transitions in magnetic field lines).
Uranus collage (January 2025, labeled version)

For the first time, an international team of astronomers have mapped the vertical structure of Uranus’s upper atmosphere, uncovering how temperature and charged particles vary with height across the planet. Using Webb’s NIRSpec instrument, the team detected the faint glow from molecules high above the clouds. These unique data provide the most detailed portrait yet of where the planet’s auroras form, how they are influenced by its unusually tilted magnetic field, and how Uranus’s atmosphere has continued to cool over the past three decades. The results offer a new window into how ice-giant planets distribute energy in their upper layers.

Two bright auroral bands were detected near Uranus’s magnetic poles, together with reduced emission and ion density in part of the region between the two bands (a feature likely linked to transitions in magnetic field lines).

L2 is one of the so-called Lagrangian points, discovered by mathematician Joseph Louis Lagrange. Lagrangian points are locations in space where gravitational forces and the orbital motion of a body balance each other. Therefore, they can be used by spacecraft to 'hover'. L2 is located 1.5 million kilometers directly 'behind' the Earth as viewed from the Sun. It is about four times further away from the Earth than the Moon ever gets and orbits the Sun at the same rate as the Earth.

It is a great place observe the larger Universe. A spacecraft would not have to make constant orbits of the Earth that result in it passing in and out of the Earth's shadow and causing it to heat up and cool down, distorting its view. Free from this restriction and far away from the heat radiated by Earth, L2 provides a much more stable viewpoint.


Credit: ESA/Webb, NASA, CSA, STScI, P. Tiranti, H. Melin, M. Zamani (ESA/Webb)
Release Date: Feb. 19, 2026

#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #NIRSpec #Planets #Uranus #Atmosphere #Aurora #SolarSystem #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education

Planet Uranus: Auroral Activity | Time-lapse Rotation | James Webb Space Telescope

Planet Uranus: Auroral Activity Time-lapse Rotation | James Webb Space Telescope

This timelapse video is believed to be the only dataset to date that has continuously observed a full rotation of Uranus by a single telescope, facilitated by Webb’s uniquely positioned orbit at L2 that observed the planet for approximately 17 hours. This time-lapse video consists of over 1200 slices of multi-object spectroscopy data. These observations provide the most detailed view to date of Uranus’ vertical upper atmosphere, showing where temperatures and ion densities peak, and revealing clear auroral structures shaped by the planet’s unusual magnetic field.

L2 is one of the so-called Lagrangian points, discovered by mathematician Joseph Louis Lagrange. Lagrangian points are locations in space where gravitational forces and the orbital motion of a body balance each other. Therefore, they can be used by spacecraft to 'hover'. L2 is located 1.5 million kilometers directly 'behind' the Earth as viewed from the Sun. It is about four times further away from the Earth than the Moon ever gets and orbits the Sun at the same rate as the Earth.

It is a great place observe the larger Universe. A spacecraft would not have to make constant orbits of the Earth that result in it passing in and out of the Earth's shadow and causing it to heat up and cool down, distorting its view. Free from this restriction and far away from the heat radiated by Earth, L2 provides a much more stable viewpoint.

An international team of astronomers have now uncovered how temperature and charged particles vary with height across the planet. Using Webb’s NIRSpec instrument, the team detected the faint glow from molecules high above the clouds. These unique data provide the most detailed portrait yet of where the planet’s auroras form, how they are influenced by its unusually tilted magnetic field, and how Uranus’s atmosphere has continued to cool over the past three decades. The results offer a new window into how ice-giant planets distribute energy in their upper layers.


Credit: ESA/Webb, NASA, CSA, STScI, P. Tiranti, H. Melin, M. Zamani (ESA/Webb)
Duration: 20 seconds
Release Date: Feb. 19, 2026


#NASA #ESA #Astronomy #Space #Science #JWST #JamesWebb #WebbTelescope #Planets #Uranus #Atmosphere #Aurora #SolarSystem #Universe #UnfoldTheUniverse #Europe #CSA #Canada #GSFC #STScI #UnitedStates #STEM #Education #HD #Video

Expedition 74: New Crewmates Arrive | International Space Station

Expedition 74: New Crewmates Arrive | International Space Station

NASA astronaut and SpaceX Crew-12 Commander Jessica Meir enters the International Space Station after docking aboard the Dragon spacecraft to join Expedition 74 and begin a long-duration microgravity research mission.
European Space Agency (ESA) astronaut and SpaceX Crew-12 Mission Specialist Sophie Adenot of France enters the International Space Station after docking aboard the Dragon spacecraft to join Expedition 74 and begin a long-duration microgravity research mission.
Roscosmos cosmonaut and SpaceX Crew-12 Mission Specialist Andrey Fedyaev of Russia enters the International Space Station after docking aboard the Dragon spacecraft to join Expedition 74 and begin a long-duration microgravity research mission.
NASA astronaut and SpaceX Crew-12 Pilot Jack Hathaway enters the International Space Station after docking aboard the Dragon spacecraft to join Expedition 74 and begin a long-duration microgravity research mission.
NASA astronaut and Expedition 74 Flight Engineer Jessica Meir configures the Microgravity Science Glovebox and swaps hard drives to support operations for the Zero Boil-Off Tank physics investigation. The experiment is testing ways to control a spacecraft’s fuel tank pressure due to cryogenic fuel propellants evaporating from the surrounding heat.
European Space Agency (ESA) astronaut and Expedition 74 Flight Engineer Sophie Adenot of France swaps hard drives inside the Advanced Space Experiment Processor-4 (ADSEP-4). Located aboard the International Space Station's Destiny laboratory module, the ADESP-4 houses and processes research samples for an array of microbiology and physics studies and can be operated onboard the Dragon and Cygnus spacecraft, as well as the orbital outpost.
NASA Crew-12 emblem

NASA astronauts Jessica Meir and Jack Hathaway, European Space Agency (ESA) astronaut Sophie Adenot of France, and Roscosmos cosmonaut Andrey Fedyaev of Russia have entered the International Space Station to begin their long-duration science expedition after opening the hatches at 5:14 p.m. EST on Feb. 14, 2026, between the space station and the SpaceX Dragon spacecraft.

Meir, Hathaway, Adenot, and Fedyaev now join Expedition 74 crew, including NASA astronaut Chris Williams and Roscosmos cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev of Russia already aboard the orbiting laboratory.


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Image Credit: NASA's Johnson Space Center (JSC)
Dates: Feb. 14-16, 2026

#NASA #Space #ISS #SpaceX #SpaceXCrew12 #CrewDragonSpacecraft #Astronauts #JessicaMeir #Crew12Commander #JackHathaway #SophieAdenot #France #Europe #ESA #Cosmonauts #AndreyFedyaev #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #Expedition75 #JSC #UnitedStates #STEM #Education

Wednesday, February 18, 2026

Shenzhou-21 Astronauts Grow Cherry Tomatoes | China Space Station

Shenzhou-21 Astronauts Grow Cherry Tomatoes | China Space Station

Chinese astronauts could be set to enjoy an upgraded diet in the future as the crew members of the Shenzhou-21 mission get ready to reap a bountiful harvest of freshly-grown tomatoes from their very own in-orbit vegetable garden aboard the Tiangong Space Station.

Amid the ongoing Spring Festival holiday, when millions of Chinese gather for family reunions and enjoy grand festive dinners to welcome the Chinese New Year back on Earth, the astronauts in space may soon be able to tuck into some tasty foods of their own, as their prized tomatoes enter their ripe season.

The three crew members had already enjoyed something of a first in space when they indulged in a special space barbecue after bringing a hot-air oven to space back in November 2025, sharing in a mouthwatering meat feast with the predecessor crew of Shenzhou-20 during their brief handover period aboard the space station.

Now, however, they are focusing their efforts on healthier ingredients. So far, ten batches of seven plant species, including lettuce, cherry tomatoes and sweet potatoes, have been cultivated at the space station, providing astronauts with more fresh fruits and vegetables and the chance for a much more balanced nutritional intake during their six-month-long mission.

Astronaut Zhang Hongzhang introduced the unique  looking contraption that is being used to carefully cultivate cherry tomatoes.

"This tomato cultivation device is called 'water aeroponic cultivation' and was developed by a research team from the China Astronaut Research and Training Center (CARTC). It can significantly increase the utilization rate of water through water evaporation. On the other hand, an LED spectrum has been specially customized, that can significantly improve the efficiency of energy utilization. As a result, we can see a thriving picture of space tomatoes growing," said Zhang.

The cultivation device was delivered to the space station by the Tianzhou-9 cargo craft in July last year. It is mainly used to verify key technologies for efficient plant aeroponic cultivation in a microgravity environment.

"Currently in orbit, we take care of it and record its growing data every day. While providing valuable planting data in orbit, it will be of very good reference value to the cultivation of space crops in later missions," said astronaut Wu Fei.

Relying on the cultivation device, researchers can systematically carry out research on multiple subjects, such as in-orbit efficient plant cultivation, fruit and vegetable production and evaluation in space, atmospheric regeneration capacity and efficiency, and in-orbit plant care models.

The aeroponic cultivation experiments are also planned to be carried out on wheat, carrots and medicinal and edible plants in the future.

Launched into space on October 31 last year, the Shenzhou-21 crew is now over 100 days into its six-month space mission. All tasks including scientific experiments, equipment maintenance and health management are progressing smoothly, according to China's space agency—the China National Space Administration (CNSA).

Shenzhou-21 Crew
Zhang Lu (张陆) - Commander & Pilot - 2nd spaceflight
Wu Fei (武飞)  Flight Engineer - 1st spaceflight
Zhang Hong Zhang (张洪章) - Payload Specialist - 1st spaceflight


Video Credit: CCTV
Duration: 1 minute
Release Date: Feb. 18, 2026


#NASA #Space #Science #China #中国 #CherryTomatoes #Tomatoes #Shenzhou21Mission #神舟二十一号 #Shenzhou21 #Taikonauts #Astronauts #ZhangLu #WuFei #ZhangHongzhang #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #MicrogravityExperiments #SpaceLaboratory #CNSA #国家航天局 #HumanSpaceflight #STEM #Education #HD #Video

Spring Festival Fireworks over Beijing, China | International Space Station

Spring Festival Fireworks over Beijing, China | International Space Station

Expedition 74 flight engineer and NASA astronaut Chris Williams "Happy Year of the Horse! I was fortunate to be looking out of the Cupola while we were passing over Beijing, and saw the twinkling of fireworks celebrating the Lunar New Year!"

Beijing, previously romanized as Peking, is the capital city of the People's Republic of China (PRC). It is located in Northern China, and is governed as a municipality. Beijing is mostly surrounded by Hebei province and neighbors the city of Tianjin to the southeast.


Expedition 74 Crew
Station Commander: Sergey-Kud Sverchkov (Russia)
Roscosmos (Russia) Flight Engineers: 
Andrey Fedyaev, Sergei Mikaev
European Space Agency Flight Engineer: Sophie Adenot
NASA Flight Engineers: Jessica Meir, Jack Hathaway, Chris Williams

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.


Video Credit: NASA's Johnson Space Center/C. Williams
Duration: 22 seconds
Release Date: Feb. 18, 2026


#NASA #Space #ISS #Science #Planets #Earth #Beijing #北京 #China #中国 #SpringFestival #Fireworks #Astronauts #ChrisWilliams #AstronautVideography #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education #HD #Video

How NASA's Perseverance Mars Rover Learned to ‘Self-Locate’ | JPL

How NASA's Perseverance Mars Rover Learned to ‘Self-Locate’ | JPL


NASA’s Perseverance rover can now precisely determine its own location on Mars without waiting for human help from Earth. This is possible thanks to a new technology called Mars Global Localization.

This technology rapidly compares panoramic images from the rover’s navigation cameras with onboard orbital terrain maps. It is done with an algorithm that runs on the rover’s Helicopter Base Station processor that was originally used to communicate with the Ingenuity Mars Helicopter. In a few minutes, the algorithm can pinpoint Perseverance’s position to within about 10 inches (25 centimeters). The technology will help the rover drive farther autonomously and keep exploring. 

Mars Global Localization was first used successfully for regular mission operations on Feb. 2, 2026, and the team expects related reliability techniques to inform future missions, including exploration on the Moon.


Video Credit: NASA's Jet Propulsion Laboratory
Duration: 1 minute, 35 seconds
Release Date: Feb. 18, 2026

#NASA #Space #Astronomy #Science #Planets #Mars #Astrobiology #Geology #PerseveranceRover #Mars2020 #JezeroCrater #MarsGlobalLocalization #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education #Animation #HD #Video

"Dark Galaxy" CDG-2 Detected in Perseus | Hubble Space Telescope

"Dark Galaxy" CDG-2 Detected in Perseus | Hubble Space Telescope



The low-surface-brightness galaxy CDG-2, shown in this image from the NASA/European Space Agency Hubble Space Telescope, is dominated by dark matter and contains only a sparse scattering of stars. This galaxy is nearly invisible, but by using advanced statistical techniques, scientists identified it by searching for tight groupings of stars called globular clusters at the center of this image.

The Hubble observations include those from programme 15235 (W. Harris).

Image Description: A field of space with a dozen white foreground stars and a number of small, yellow background galaxies.


Credit: NASA, ESA, D. Li (Utoronto), Image Processing: J. DePasquale (STScI)
Release Date: Feb. 18, 2026


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