Saturday, January 10, 2026

Pandora Satellite, CubeSats to Explore Exoplanets & Beyond | NASA Goddard

Pandora Satellite, CubeSats to Explore Exoplanets & Beyond | NASA Goddard

The Pandora spacecraft with an exoplanet and two stars in the background. This is an artist’s concept of NASA’s Pandora mission. Pandora will help scientists untangle signals from exoplanet atmospheres—worlds beyond our solar system—and their stars.
Pandora spacecraft, fully integrated, with blue-lit background
This view of the fully integrated Pandora spacecraft was taken May 19, 2025, following the mission’s successful environmental test campaign at Blue Canyon Technologies in Lafayette, Colorado. The next step is to ready the vehicle for shipping to the launch site. Visible are star trackers (center), multilayer insulation blankets (white), the end of the telescope (top), and the solar panel (right) in its launch configuration.
This view looks down the barrel of Pandora’s 17-inch-wide (45 centimeters) telescope and was captured April 12, 2025, at Lawrence Livermore National Laboratory in California. The concentric black circles are optical baffles designed to prevent stray light bouncing around the telescope tube from reaching the detectors. At center, part of the ceiling appears in Pandora’s main mirror. Above it, attached to the tube by four supports, is the secondary mirror, which bounces light through the main mirror and into the telescope’s detectors.
Pandora’s 17-inch-wide (45 centimeters) telescope and its associated systems are seen April 12, 2025, at Lawrence Livermore National Laboratory in California as the instrument package nears completion.
The spacecraft bus for the Pandora mission was developed at Blue Canyon Technologies in Lafayette, Colorado, and completed on March 31, 2025. The bus provides Pandora’s structural, power, and support systems. Two star trackers (top left) enable the spacecraft’s precise and stable pointing for science observations. The large bracket extending above the main box supports Pandora’s single articulating solar array.
The spacecraft bus for the Pandora mission was developed at Blue Canyon Technologies in Lafayette, Colorado, and completed on March 31, 2025. The bus provides Pandora’s structural, power, and support systems. Two star trackers (top left) enable the spacecraft’s precise and stable pointing for science observations. The large bracket extending above the main box supports Pandora’s single articulating solar array.

A new NASA spacecraft called Pandora is awaiting launch ahead of its journey to study the atmospheres of exoplanets, or worlds beyond our solar system, and their stars. Along for the ride are two shoebox-sized satellites called BlackCAT (Black Hole Coded Aperture Telescope) and SPARCS (Star-Planet Activity Research CubeSat), as NASA innovates with ambitious science missions that take low-cost, creative approaches to answering questions like, “How does the universe work?” and “Are we alone?”

All three missions are set to launch January 11, 2026, on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg in California. The launch window opens at 8:19 a.m. EST (5:19 a.m. PST). SpaceX will livestream the event.

“Pandora’s goal is to disentangle the atmospheric signals of planets and stars using visible and near-infrared light,” said Elisa Quintana, Pandora’s principal investigator at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “This information can help astronomers determine if detected elements and compounds are coming from the star or the planet—an important step as we search for signs of life in the cosmos.”

BlackCAT and SPARCS are small satellites that will study the transient, high-energy universe and the activity of low-mass stars, respectively.

Pandora will observe planets as they pass in front of their stars as seen from our perspective, events called transits.

As starlight passes through a planet’s atmosphere, it interacts with substances like water and oxygen that absorb characteristic wavelengths, adding their chemical fingerprints to the signal.

However, while only a small fraction of the star’s light grazes the planet, telescopes also collect the rest of the light emitted by the star’s facing side. Stellar surfaces can sport brighter and darker regions that grow, shrink, and change position over time, suppressing or magnifying signals from planetary atmospheres. Adding a further complication, some of these areas may contain the same chemicals that astronomers hope to find in the planet’s atmosphere, such as water vapor.

All these factors make it difficult to be certain that important detected molecules come from the planet alone.

Pandora will help address this problem by providing in-depth study of at least 20 exoplanets and their host stars during its initial year. The satellite will look at each planet and its star 10 times, with each observation lasting a total of 24 hours. Many of these worlds are among the over 6,000 discovered by missions like NASA’s TESS (Transiting Exoplanet Survey Satellite).

Pandora will collect visible and near-infrared light using a novel, all-aluminum 17-inch-wide (45-centimeter) telescope jointly developed by Lawrence Livermore National Laboratory in California and Corning Incorporated in Keene, New Hampshire. Pandora’s near-infrared detector is a spare developed for NASA’s James Webb Space Telescope.

Each long observation period will capture a star’s light both before and during a transit and help determine how stellar surface features impact measurements.

“These intense studies of individual systems are difficult to schedule on high-demand missions, like Webb,” said engineer Jordan Karburn, Pandora’s deputy project manager at Livermore. “You also need the simultaneous multiwavelength measurements to pick out the star’s signal from the planet’s. The long stares with both detectors are critical for tracing the exact origins of elements and compounds scientists consider indicators of potential habitability.”

Pandora is the first satellite to launch in the agency’s Astrophysics Pioneers program, which seeks to do compelling astrophysics at a lower cost while training the next generation of leaders in space science.

After launching into low Earth orbit, Pandora will undergo a month of commissioning before embarking on its one-year prime mission. All the mission’s data will be publicly available.

“The Pandora mission is a bold new chapter in exoplanet exploration,” said Daniel Apai, an astronomy and planetary science professor at the University of Arizona in Tucson where the mission’s operations center resides. “It is the first space telescope built specifically to study, in detail, starlight filtered through exoplanet atmospheres. Pandora’s data will help scientists interpret observations from past and current missions like NASA’s Kepler and Webb space telescopes. And it will guide future projects in their search for habitable worlds.”

The BlackCAT and SPARCS missions will take off alongside Pandora through NASA’s Astrophysics CubeSat program, the latter supported by the Agency's CubeSat Launch Initiative.

CubeSats are a class of nanosatellites that come in sizes that are multiples of a standard cube measuring 3.9 inches (10 centimeters) across. Both BlackCAT and SPARCS are 11.8 by 7.8 by 3.9 inches (30 by 20 by 10 centimeters). CubeSats are designed to provide cost-effective access to space to test new technologies and educate early career scientists and engineers while delivering compelling science.

The BlackCAT mission will use a wide-field telescope and a novel type of X-ray detector to study powerful cosmic explosions like gamma-ray bursts, particularly those from the early universe, and other fleeting cosmic events. It will join NASA’s network of missions that watch for these changes. Abe Falcone at Pennsylvania State University in University Park, where the satellite was designed and built, leads the mission with contributions from Los Alamos National Laboratory in New Mexico. Kongsberg NanoAvionics US provided the spacecraft bus.

The SPARCS CubeSat will monitor flares and other activity from low-mass stars using ultraviolet light to determine how they affect the space environment around orbiting planets. Evgenya Shkolnik at Arizona State University in Tempe leads the mission with participation from NASA’s Jet Propulsion Laboratory in Southern California. In addition to providing science support, JPL developed the ultraviolet detectors and the associated electronics. Blue Canyon Technologies fabricated the spacecraft bus.

Pandora is led by NASA Goddard. Livermore provides the mission’s project management and engineering. Pandora’s telescope was manufactured by Corning and developed collaboratively with Livermore, which also developed the imaging detector assemblies, the mission’s control electronics, and all supporting thermal and mechanical subsystems. The near-infrared sensor was provided by NASA Goddard. Blue Canyon Technologies provided the bus and performed spacecraft assembly, integration, and environmental testing. NASA’s Ames Research Center in California’s Silicon Valley will perform the mission’s data processing. Pandora’s mission operations center is located at the University of Arizona, and a host of additional universities support the science team.

Image Credits: NASA's Goddard Space Flight Center / Conceptual Image Lab
NASA / BCT / Jordan Karburn, LLNL
Release Date: Jan. 9, 2026

#NASA #Space #Astronomy #Science #SmallSat #Stars #StarSystems #Exoplanets #ExoplanetTransits #PlanetaryAtmospheres #Astrobiology #Habitability #Astrophysics #NASAPandoraMission #PandoraMission #SpaceExploration #MilkyWayGalaxy #Universe #GSFC #LLNL #UnitedStates #STEM #Education

Greenland Ice Sheet: Ice Velocity (2014–2024) | Europe's Sentinel-1 Earth Satellite

Greenland Ice Sheet: Ice Velocity (2014–2024) | Europe's Sentinel-1 Earth Satellite

This map, based on Copernicus Sentinel-1 Earth satellite data, shows the speed ice is moving horizontally on the Greenland Ice Sheet. Sentinel-1’s year-round acquisitions of the ice sheet's marginal zones, along with dedicated winter mapping campaigns that include the interior ice sheet, enable the production of annual ice sheet-wide velocity maps. These maps are derived using offset tracking, a data analysis technique that compares satellite images of the same location at distinct times to ‘track’ ground movement.
This map, based on Copernicus Sentinel-1 data, shows the speed ice is moving horizontally on the Jakobshavn Glacier in Greenland. Half-way up the western coast of Greenland, it is one of the fastest outlet glaciers in the world with velocities reaching, at times, up to 50 meters or 164 feet per day.

First Image: This map, based on Copernicus Sentinel-1 Earth satellite data, shows the speed ice is moving horizontally on the Greenland Ice Sheet. Sentinel-1’s year-round acquisitions of the ice sheet's marginal zones, along with dedicated winter mapping campaigns that include the interior ice sheet, enable the production of annual ice sheet-wide velocity maps. These maps are derived using offset tracking, a data analysis technique that compares satellite images of the same location at distinct times to ‘track’ ground movement.

The study shows rapid flow of ice, moving at average speeds of up to 15 meters (49 feet) per day, from glaciers and ice sheets at points around the Greenland Ice Sheet. Half-way up the western coast of Greenland, Sermeq Kujalleq (also known as the Jakobshavn Glacier), is one of the fastest outlet glaciers in the world with velocities reaching, at times, up to 50 meters (164 feet) per day. The North-East Greenland Ice Stream (NEGIS), is also clearly visible and begins far inland at the ‘ice divide’, shown as a dark blue band of nearly stagnant ice in Greenland’s interior.

Second Image: This map, based on Copernicus Sentinel-1 data, shows the speed ice is moving horizontally on the Jakobshavn Glacier in Greenland. Half-way up the western coast of Greenland, it is one of the fastest outlet glaciers in the world with velocities reaching, at times, up to 50 m per day.

Sentinel-1’s year-round acquisitions of the ice sheet's marginal zones, along with dedicated winter mapping campaigns that include the interior ice sheet, enable the production of annual ice sheet-wide velocity maps. These maps are derived using offset tracking, a data analysis technique that compares satellite images of the same location at different times to ‘track’ ground movement.

Greenland (called Tartupaluk in Inuktitut and Greenlandic) is an autonomous territory of the Kingdom of Denmark and is the largest of the kingdom's three constituent parts by land area, the others being Denmark proper and the Faroe Islands. It shares a small 1.2 km border with Canada on Hans Island. Citizens of Greenland are full citizens of Denmark and of the European Union. Greenland is one of the Overseas Countries and Territories of the European Union and is part of the Council of Europe. It is the world's largest island and lies between the Arctic and Atlantic oceans, east of the Canadian Arctic Archipelago.


Credits: European Space Agency (ESA), (Data source: Wuite, J. et al. 2025).
Release Date: Jan. 8, 2026

#NASA #Space #Science #Satellites #CopernicusProgramme #Sentinel1 #Earth #AtlanticOcean #ArcticOcean #IceSheets #MeltingIce #IceVelocity #Greenland #Tartupaluk #Grønland #Denmark #Danmark #EuropeanUnion #EU #InternationalCooperation #Environment #Climate #ClimateChange #GlobalHeating #EarthObservation #STEM #Education

Comet C/2023 A3 (Tsuchinshan–ATLAS) above Uluru

Comet C/2023 A3 (Tsuchinshan–ATLAS) above Uluru

C/2023 A3 (Tsuchinshan–ATLAS) is a comet from the solar system's Oort cloud discovered by the Purple Mountain Observatory east of Nanjing, China, on January 9, 2023, and independently found by the automated Asteroid Terrestrial-impact Last Alert System (ATLAS) in South Africa on February 22, 2023. ATLAS is funded by NASA's planetary defense office, and developed and operated by the University of Hawaii's Institute for Astronomy. C/2023 A3 passed perihelion (closest approach to the Sun) at a distance of 0.39 AU (58 million km; 36 million miles) on September 27, 2024.

The Oort cloud is theorized to be a vast cloud of icy planetesimals surrounding the Sun at distances ranging from 2,000 to 200,000 AU (0.03 to 3.2 light-years).

Uluru, also known as Ayers Rock, is a large sandstone monolith. It crops out near the center of Australia in the southern part of the Northern Territory, 335 km (208 mi) southwest of Alice Springs. Uluru is sacred to the Pitjantjatjara, the Aboriginal people of the area, known as the Aṉangu. The area around the formation is home to an abundance of springs, waterholes, rock caves and ancient paintings. Uluru is listed as a UNESCO World Heritage Site.

Uluru is one of Australia's most recognizable natural landmarks and has been a popular destination for tourists since the late 1930s. It is also one of the most important indigenous sites in Australia.

The comet was captured on October 2, 2024, approximately five minutes after the onset of astronomical dawn.

Note: The foreground was photographed separately from the same location under moonlight conditions (Moon age ≈ 10 days) on Dec 1, 2025, using the same equipment.


Image Credit: Cullen Pan
Capture Location: Uluru-Kata Tjuta National Park, Northern Territory, Australia
Image Details: 
Sony A1 · Sigma 35mm F1.2 DG DN | Single exposure: ISO 3200 · f/1.8 · 10 s 
Exposure: ISO 800 · f/2.5 · 8 s
Image Date: Oct. 2, 2024


#NASA #Space #Astronomy #Science #Planet #Earth #Comets #CometTsuchinshanATLAS #C2023A3 #OortCloud #SolarSystem #Astrophotography #UluruKataTjutaNationalPark #NorthernTerritory #Australia #UnitedStates #China #中国 #SouthAfrica #STEM #Education

Friday, January 09, 2026

NASA & SpaceX Target Date for Crew-11 Earth Return | International Space Station

NASA & SpaceX Target Date for Crew-11 Earth Return | International Space Station

 International Space Station Configuration. Seven spacecraft are parked at the space station including the SpaceX Dragon cargo craft, the SpaceX Crew-11 Dragon spacecraft, JAXA’s HTV-X1 cargo craft, Northrop Grumman’s Cygnus cargo craft, the Soyuz MS-28 crew ship, and the Progress 92 and 93 resupply ships.

NASA and SpaceX are targeting no earlier than 5 p.m. EST, Wednesday, Jan. 14, 2026, for the undocking of the agency’s SpaceX Crew-11 Mission spacecraft from the International Space Station, pending weather conditions. 

On Jan. 8, NASA announced its decision to return the agency’s SpaceX Crew-11 mission to Earth from the space station earlier than originally planned as teams monitor a medical concern with a crew member currently living and working aboard the orbital laboratory that remains stable. Due to medical privacy, it is not appropriate for NASA to share more details about the crew member. 

NASA astronauts Zena Cardman and Mike Fincke, Japan Aerospace Exploration Agency (JAXA) astronaut Kimiya Yui, and Roscosmos cosmonaut Oleg Platonov of Russia will splash down off the coast of California at approximately 3:40 a.m. on Thursday, Jan. 15.

Mission managers continue monitoring conditions in the recovery area, as undocking of the SpaceX Dragon depends on spacecraft readiness, recovery team readiness, weather, sea states, and other factors. NASA and SpaceX will select a specific splashdown time and location closer to the Crew-11 spacecraft undocking. 

NASA’s coverage is as follows (all times Eastern and subject to changed based on operations): 

Wednesday, Jan. 14 
3 p.m. – Hatch closure coverage begins
3:30 p.m. – Hatch closing 
4:45 p.m. – Undocking coverage begins
5 p.m. – Undocking

Thursday, Jan. 15 
2:15 a.m. – Return coverage begins
2:50 a.m. – Deorbit burn 
3:40 a.m. – Splashdown 
5:45 a.m. – Return to Earth media news conference

NASA will set share more details about its coverage plans in the coming days.


Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

Credit: NASA's Johnson Space Center
Release Date: 
Jan. 9, 2025

#NASA #Space #ISS #Science #Planets #Earth #SpaceXCrew11 #Spacewalks #EVA #Astronauts #MikeFincke #ZenaCardman #KimiyaYui #CrewHealth #AstronautHealth #UnitedStates #Japan #JAXA #UnitedStates #Cosmonauts #OlegPlatonov #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education

Medical Issue Postpones Crew Spacewalks 94 & 95 | International Space Station

Medical Issue Postpones Crew Spacewalks 94 & 95 | International Space Station

Japan Aerospace Exploration Agency (JAXA) flight engineer Kimiya Yui, reflected in the visor of a crewmate’s helmet. 
Flight engineer and NASA astronaut Zena Cardman: "Kimiya Yui is a technical master, but I love him even more for his selfless nature, bottomless patience, and perfect blend of humor and humility. When I’m having a rough day, Kimiya somehow shows up at exactly the right moment with a piece of chocolate, saying 'thank you for your hard work'–and everything becomes magically better. This week marked Yui-san’s 300th cumulative day in space, and I feel so lucky to have shared some of that time with him."
NASA Astronaut and Expedition 74 Flight Engineer Zena Cardman is pictured in her pressurized spacesuit, checking its communication and power systems ahead of a spacewalk originally planned for Thursday, Jan. 8, 2025. At upper right, Japan Aerospace Exploration Agency (JAXA) Astronaut and Flight Engineer Kimiya Yui assists Cardman as she tests the operations of her spacesuit inside the International Space Station’s Quest airlock.
At center, Japan Aerospace Exploration Agency (JAXAastronaut and Expedition 74 Flight Engineer Kimiya Yui assists NASA astronauts Zena Cardman (left) and Mike Fincke (right), the station’s flight engineer and commander respectively, during spacesuit checks inside the International Space Station’s Quest airlock.
NASA astronaut and Expedition 74 Commander Mike Fincke is pictured in his pressurized spacesuit, checking its communication and power systems ahead of a spacewalk originally planned for Thursday, Jan. 8, 2025. Partially obscured at left, Japan Aerospace Exploration Agency (JAXA) Astronaut and Expedition 74 Flight Engineer Kimiya Yui assists NASA Flight Engineer Zena Cardman as she tests the operations of her spacesuit inside the International Space Station’s Quest airlock.
NASA astronaut and Expedition 74 Commander Mike Fincke poses inside the International Space Station’s Quest airlock next to a spacesuit. The helmet is secured with a protective cover designed to prevent scratches and contamination when the suit is not in use, ensuring the visor remains clear for spacewalks.
International Space Station Expedition 74 Crew Mission Emblem

Updates: NASA announced on Thursday, January 8, 2026, its decision to return the agency’s SpaceX Crew-11 mission to Earth from the International Space Station earlier than originally planned as teams monitor a medical concern with a crew member currently living and working aboard the orbital laboratory. As NASA reviews Crew-11 return dates, the agency also is working with SpaceX, and its international partners, to review the options available to advance launch opportunities for the Crew-12 mission. The agency anticipates a decision on a target Crew-11 return date in the coming days.

Four Expedition 74 crew members are preparing for their return to Earth aboard the SpaceX Dragon crew spacecraft. SpaceX Crew-11 members have begun checking the fit and operability of their Dragon pressure suits. Fit verification is necessary because the spine lengthens and body fluids shift toward the head in microgravity, affecting torso and limb dimensions. The quartet also tested the suits’ audio and video communication systems.

Dragon Commander Zena Cardman will lead Pilot Mike Fincke, both NASA astronauts, and Mission Specialists Kimiya Yui of Japan Aerospace Exploration Agency (JAXA) and Oleg Platonov of Roscosmos (Russia) back to Earth inside Dragon. On Jan. 9, 2026, the foursome began collecting their personal items and packing them for stowage aboard the spacecraft.

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

Image Credit: NASA's Johnson Space Center
Release Dates: 
Dec. 3, 2026 to Jan. 7, 2025

#NASA #Space #ISS #Science #Planets #Earth #SpaceXCrew11 #Spacewalks #EVA #Astronauts #MikeFincke #ZenaCardman #KimiyaYui #CrewHealth #AstronautHealth #UnitedStates #Japan #JAXA #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education

Steady Progress in Scientific Research & Applications in 2025 | China Space Station

Steady Progress in Scientific Research & Applications in 2025 | China Space Station

China's Tiangong Space Station, launched in 2021, made steady progress in the development of scientific research and its application during 2025, according to a report issued by China Manned Space Engineering Office (CMSEO) on Thursday, January 8, 2026.

The report focuses on areas, such as space life sciences and human research, microgravity physics, and new space technologies and applications. It features 33 representative scientific research and application outcomes that have shown remarkable progress, alongside relevant popular science activities.

Since China's crewed space program entered the application and development phase, China has successfully completed six crewed spaceflight missions, four cargo supply missions, and five spacecraft return missions. Notably, it has successfully conducted its first emergency mission.

Six astronaut crews, totaling 18 astronauts, have been stationed in orbit, performing 13 extravehicular activities (EVAs) and multiple EVAs using payloads, in addition to numerous extravehicular maintenance tasks. These efforts have reset the world record for the longest single extravehicular activity (spacewalk) by astronauts.

The selection of the fourth batch of reserve astronauts, including payload experts from Hong Kong and Macao special administrative regions (SARs), was completed, and the development of a low-cost cargo transportation system was initiated.

Preliminary statistics indicate that in 2025, scientific teams across various fields published over 230 high-level SCI papers and obtained more than 70 patents. Through in-depth experimental research and application exploration, several results have been transferred, converted, and promoted, significantly advancing the rapid development of space science and applications in China.

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, 29 seconds
Release Date: Jan. 9, 2025

#NASA #Space #Science #China #中国 #Shenzhou21Mission #神舟二十一号 #Shenzhou21 #Taikonauts #Astronauts #ZhangLu #WuFei #ZhangHongzhang #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #MicrogravityResearch #CSU #CAS #CMSA #中国载人航天工程办公室 #CMSEO #HumanSpaceflight #STEM #Education #HD #Video

Aurora Borealis over Tromsø, Norway | Earth Science

Aurora Borealis over Tromsø, Norway | Earth Science



Astrophotographer Eva Kristiansen: :"Frozen at minus ten degrees, wrapped in absolute silence, the heavens burn as the northern lights spilled their colors across the night."

On Earth, auroras are mainly created by particles originally emitted by the Sun in the form of solar wind. When this stream of electrically charged particles gets close to our planet, it interacts with the magnetic field that acts as a gigantic shield. While it protects Earth’s environment from solar wind particles, it can also trap a small fraction of them. Particles trapped within the magnetosphere—the region of space surrounding Earth in which charged particles are affected by its magnetic field—can be energized and then follow the magnetic field lines down to the magnetic poles. There, they interact with oxygen and nitrogen atoms in the upper layers of the atmosphere, creating the flickering, colorful lights visible in the polar regions here on Earth.

Earth auroras have different names depending on the pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

The Colors of the Aurora (U.S. National Park Service)

Norway, officially the Kingdom of Norway, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. The country shares a long eastern border with Sweden, and is bordered by Finland and Russia to the northeast.

Image Credit: Eva Kristiansen
Image Details: Nikon D850 Nikkor 14-24mm
Image Date: Jan. 8, 2026

#NASA #Space #Astronomy #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #SolarSystem #Sun #Astrophotography #Astrophotographer #EvaKristiansen #Tromsø #Norway #Norge #UnitedStates #STEM #Education

Earth City Lights & Starlink Satellites with Star Trails | International Space Station

Earth City Lights & Starlink Satellites with Star Trails | International Space Station

NASA astronaut and former International Space Station flight engineer Don Pettit: "Starlink satellites cutting white flashes into a star trail time exposure, creating unique photographic artifacts."

NASA astronaut Don Pettit 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: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

Image Credit: NASA's Johnson Space Center/D. Pettit
Release Date: 
Dec 31, 2025

#NASA #Space #Astronomy #Science #Stars #StarTrails #ISS #Planets #Earth #SpaceX #StarlinkSatellites #Atmosphere #Airglow #Aurora #Astronauts #DonPettit #AstronautPhotography #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education

Deep Space & Earth Airglow Views | International Space Station

Deep Space & Earth Airglow Views | International Space Station

NASA astronaut and former International Space Station flight engineer Don Pettit: "Deep space views orbiting the Pacific Ocean. The two vastest frontiers we have known, waiting to be explored!"

NASA astronaut Don Pettit 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.

You will notice red and green airglow in this image. Airglow occurs when atoms and molecules in the Earth's upper atmosphere, excited by sunlight, emit light to shed their excess energy. Or, it can happen when atoms and molecules that have been ionized by sunlight collide with and capture a free electron. In both cases, they eject a particle of light—called a photon—in order to relax again. The phenomenon is similar to auroras, but where auroras are driven by high-energy particles originating from the solar wind, airglow is energized by ordinary, day-to-day solar radiation. 

Unlike episodic and fleeting auroras, airglow shines constantly throughout Earth’s atmosphere, and the result is a tenuous bubble of light that closely encases our entire planet. (Auroras, on the other hand, are usually constrained to Earth’s poles.) Just a tenth as bright as all the stars in the night sky, airglow is far more subdued than auroras, too dim to observe easily except in orbit or on the ground with clear, dark skies and a sensitive camera.

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, Chris Williams

Image Credit: NASA's Johnson Space Center/D. Pettit
Release Date: Jan. 7, 2026

#NASA #Space #Astronomy #Science #Stars #DeepSpace #ISS #Planets #Earth #Atmosphere #Airglow #PacificOcean #Astronauts #DonPettit #AstronautPhotography #UnitedStates #Japan #JAXA #Cosmonauts #Russia #Roscosmos #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition71 #Expedition72 #STEM #Education

Catching Light Day & Night | Gemini South Telescope in Chile

Catching Light Day & Night | Gemini South Telescope in Chile


Optical telescopes use mirrors to capture as much light as possible from the night sky. The larger the mirror, the more light it can collect and the more distant, dim, and detailed targets the telescope can resolve. Gemini South is no exception. Perched on the mountain of Cerro Pachón in Chile, Gemini South is one half of the International Gemini Observatory, supported in part by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab.

The starry sky keeps Gemini busy throughout the night, but the light collection does not stop at sunrise. Gemini South is surrounded by an array of 668 solar panels. These panels collect enough energy from the sunlight to cover 28% of the power required to operate Gemini South. Solar panels at telescopes operated by NSF NOIRLab and other upgrades are part of a wider observatory plan to improve the efficient use of energy across all NOIRLab locations.

Petr Horálek, the photographer, is a NOIRLab Audiovisual Ambassador.


Credit: International Gemini Observatory/NOIRLab/NSF/AURA/P. Horálek (Institute of Physics in Opava)
Release Date: Jan. 7, 2026


#NASA #Astronomy #Space #Science #Stars #Galaxies #MilkyWayGalaxy #Cosmos #Universe #InternationalGeminiObservatory #GeminiSouthTelescope #GMOS #OpticalAstronomy #SolarPanels #Astrophotography #PetrHorálek #Astrophotographer #GeminiObservatory #NOIRLab #AURA #NSF #CerroPachón #Chile #UnitedStates #STEM #Education

China's Zhurong Mars Rover Finds Longer Liquid Water Existence | CNSA

China's Zhurong Mars Rover Finds Longer Liquid Water Existence | CNSA

Photo released on June 11, 2021 by the China National Space Administration (CNSA) shows a 'selfie' of China's first Mars rover Zhurong with the landing platform.
Zhurong rover image from December 2021.
Zhurong rover image showing its landing platform from June 2021.
Zhurong rover image from June 2021.
Zhurong rover image from June 2021.
Zhurong rover panorama from July 2021.
Zhurong rover panorama from December 2021.

Tianwen-1/Zhurong Rover Mars Mission emblem

Summary: Data from China’s Zhurong Mars rover show that significant water-related activity existed on Mars about 750 million years ago, much later than previously believed. Zhurong’s ground-penetrating radar detected a uniform sedimentary layer about 4 meters thick at its landing site in Utopia Planitia, indicating formation in a shallow sea or large lake. The rover traveled 1,921 meters between 2021 and 2022, collecting key data that challenge the view that Mars became fully arid around 3 billion years ago. Researchers said the findings provide new evidence for Mars’ climatic evolution and potential habitability.

China was the first country to successfully send an orbiter, lander, and rover to Mars on its first attempt. China is only the second country after the United States to successfully land and operate a spacecraft on Mars. 

The 240-kilogram Zhurong rover is solar-powered, carries six scientific instruments, and traveled up to 200 meters per Martian day.

By studying the detection data of China's first Mars rover, Zhurong, Chinese geologists have found that the Martian surface had still exhibited significant aqueous activity approximately 750 million years ago.

This discovery shows that water existed on Mars several hundred million years longer than previously thought.

The study, conducted by a research team from the Institute of Geology and Geophysics (IGG) under the Chinese Academy of Sciences and published in the National Science Review, provides new evidence useful for a better understanding of Martian climatic evolution, geological processes, and potential habitability.

Zhurong successfully landed in the southern Utopia Planitia on Mars in May 2021. It had traveled 1,921 meters on the red planet by May 2022, collecting abundant scientific data in the process.

Zhurong also conducted a high-frequency quad-polarized ground-penetrating radar survey on Mars, similar to performing a detailed CT scan.

Previously, it was widely believed that Mars had entered a global arid phase about 3 billion years ago. However, data from Zhurong reveals that its landing site is extensively covered with a uniform sedimentary layer approximately 4 meters thick underground, including craters buried beneath.

"The uniform thickness and continuity of the sedimentary rule out the possibility of volcanic eruptions or wind-driven processes. The only reasonable explanation is that this area was in an aqueous sedimentary environment at that time, similar to a shallow sea or a large lake," said Liu Yike, the first author and corresponding author of the study.

Meanwhile, the radar also captured centimeter-scale layered sediments that formed in a water-based sedimentary environment, further supporting the existence of a shallow aquatic environment in this region in the past.

"Comprehensive analysis indicates that the landing site of Zhurong underwent a significant resurfacing event during the middle-late Amazonian Period, and that sustained aqueous activity still existed on Mars during this period," said Liu.

Zhurong Rover Mars Landing Date: May 14, 2021


Study Credit: Institute of Geology and Geophysics (IGG), Chinese Academy of Sciences
Image Credit: China National Space Administration (CNSA)
Release Date: Jan. 7, 2025


#NASA #CNSA #国家航天局 #Space #Astronomy #Science #Planets #Mars #天问 #UtopiaPlanitia #Atmosphere #Water #Lakes #WaterIce #Geology #Astrobiology #ZhurongRover #祝融 #Tianwen1 #天问一号 #MarsOrbiter #MarsSpacecraft #China #中国 #SolarSystem #SpaceExploration #Scientists #STEM #Education

Thursday, January 08, 2026

Nightflight: USA, Canada, Europe & The Middle East | International Space Station

Nightflight: USA, Canada, Europe & The Middle East | International Space Station

Expedition 74 flight engineer and Japan Aerospace Exploration Agency (JAXA) astronaut Kim Yui: "Today, I'd like to introduce a timelapse of the path from the United States across the Atlantic to Europe and the Middle East. I hope this video gives you all a boost of energy! Let's do our best today, too!"

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, 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: Japan Aerospace Exploration Agency (JAXA)/K. Yui
Duration: 35 seconds
Release Date: Jan. 8, 2026

#NASA #Space #ISS #Science #Planets #Earth #UnitedStates #Canada #Europe #MiddleEast #Astronauts #AstronautVideography #UnitedStates #Japan #日本 #JAXA #宇宙航空研究開発機構 #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education #HD #Video

Storm Goretti over Western Europe | Europe's Meteosat-12 Weather Satellite

Storm Goretti over Western Europe | Europe's Meteosat-12 Weather Satellite


This image shows Storm Goretti, a deep low-pressure system that is expected to bring very strong winds, rain, and snow to parts of Ireland, the UK, and France. Coastal areas, particularly in northern France, are also facing flood warnings.

The Meteosat weather satellites provide imagery for the early detection of fast-developing severe weather, weather forecasting and climate monitoring.

The image was captured by the  Flexible Combined Imager (FCI) instrument onboard Meteosat-12 on January 8, 2026. Meteosat-12 is in a geostationary orbit at an altitude of around 36,000 kilometers.

Launched on December 13, 2022, Meteosat-12 scans the full Earth disc every 10 minutes, delivering data more frequently and in sharper detail than its predecessor. It carries two main instruments: the Flexible Combined Imager (FCI) and Lightning Imager (LI). The FCI delivers imaging data in twice as many spectral channels than its predecessor and with an improved spatial resolution, providing more detailed views of fast-changing weather such as storms, fog, and rapidly forming clouds. The satellite also carries the LI, Europe’s first space-based instrument to detect lightning across Europe and Africa, day and night, helping forecasters assess storm development, intensity, and risk.

EUMETSAT has established cooperation with Earth observation satellite operators in Europe, China, India, Japan, South Korea and the United States.


United Nations: What is Climate Change?
https://www.un.org/en/climatechange/what-is-climate-change

Image Credit: European Organization for the Exploitation of Meteorological Satellites (EUMETSAT)
Release Date: Jan. 8, 2026

#NASA #ESA #EUMETSAT #Space #Science #Satellites #Planets #Earth #WesternEurope #StormGoretti #LowPressureSystems #Weather #Meteorology #Environment #Climate #ClimateChange #GlobalHeating #Meteosat12 #MeteosatSatellites #EarthObservation #Europe #EuropeanUnion #InternationalCooperation #CivilianSpace #STEM #Education

Mount Everest: New Year Views | International Space Station

Mount Everest: New Year Views | International Space Station


Expedition 74 flight engineer and NASA astronaut Zena Cardman: "Chomolungma, Everest from space. My first photo from our first orbit in 2026 was of sunrise painting the Himalaya. It’s a place I’ve never been, though I hope this isn’t the closest I’ll ever get to such mountains. From this distance, even Earth’s tallest peaks look like not much more than a wrinkled bedsheet, but my imagination is easily lost in the view. What incredible sculptures by the artist time. I’m left feeling both very big and very small, all at once. Happy New Year to all on my favorite planet!"

Mount Everest (known locally as Sagarmāthā[a] in Nepal and Qomolangma in Tibet) is Earth's highest mountain above sea level. It lies in the Mahalangur Himal sub-range of the Himalayas and marks part of the China–Nepal border at its summit. Its height was most recently measured in 2020 by Chinese and Nepali authorities as 8,848.86 m (29,031 ft 8+1⁄2 in).

Follow Expedition 74:

Expedition 74 Crew
Station Commander: Mike Fincke (NASA)
JAXA Flight Engineer (Japan): Kimiya Yui
Roscosmos (Russia) Flight Engineers: Oleg Platonov, Sergey-Kud Sverchkov, Sergei Mikaev
NASA Flight Engineers: Zena Cardman, 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/ Z. Cardman 
Release Date: Jan. 5, 2026

#NASA #Space #ISS #Science #Planets #Earth #MountEverest #Chomolungma #Nepal #TibetAutonomousRegion #西藏自治区 #China #中国 #Astronauts #AstronautPhotography #UnitedStates #Japan #JAXA #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #InternationalCooperation #Expedition74 #STEM #Education

Spiral Galaxy IC 342: Hidden by Gas & Dust in Camelopardalis

Spiral Galaxy IC 342: Hidden by Gas & Dust in Camelopardalis

Similar in size to large, bright spiral galaxies in our neighborhood, IC 342 is a mere 10 million light-years distant toward the long-necked, northern constellation Camelopardalis. A sprawling island universe, IC 342 would otherwise be a prominent galaxy in our night sky, but it is hidden from clear view and only glimpsed through the veil of stars, gas and dust clouds along the plane of our own Milky Way galaxy. Even though IC 342's light is dimmed and reddened by intervening cosmic clouds, this sharp telescopic image traces the galaxy's own obscuring dust, young star clusters, and glowing star forming regions along spiral arms that wind far from the galaxy's core. IC 342 has undergone a recent burst of star formation activity and is close enough to have influenced the evolution of the local group of galaxies and the Milky Way.


Image Credit & Copyright: Gaetan Maxant
Gaetan's website: https://app.astrobin.com/u/Gmaxt
Release Date: Jan. 8, 2026


#NASA #Astronomy #Space #Science #Galaxies #IC342 #Caldwell5 #CamelopardalisConstellation #Cosmos #Universe #Astrophotography #Astrophotographer #GaetanMaxant #CitizenScientist #GSFC #UnitedStates #STEM #Education #APoD

Spiral Galaxy IC 342 in Camelopardalis | Mayall Telescope

Spiral Galaxy IC 342 in Camelopardalis | Mayall Telescope

Spiral Galaxy IC 342 is located roughly 10 million light-years from Earth in the constellation Camelopardalis, “the giraffe.” Its face-on appearance in the sky—as opposed to our tilted and edge-on views of many other nearby galaxies, such as the large spiral galaxy Andromeda (M31)—makes IC 342 a prime target for studies of star formation and astrochemistry. The image, obtained in late 2006, was taken using the 64-megapixel Mosaic-1 digital imager on the Mayall 4-meter telescope. 

IC 342 (also known as Caldwell 5) is an intermediate spiral galaxy located relatively close to the Milky Way. Despite its size and actual brightness, its location behind dusty areas near the galactic equator makes it difficult to observe, leading to the nickname "The Hidden Galaxy", although it can readily be detected even with binoculars. If the galaxy were not obscured, it would be visible by naked eye. The dust makes it difficult to determine its precise distance; modern estimates range between 7 to 10 million light-years. The galaxy was discovered by William Frederick Denning in 1892. It is one of the brightest in the IC 342/Maffei Group, one of the closest galaxy groups to the Local Group. Edwin Hubble first thought it to be in the Local Group, but it was later determined not to be a member.

The Nicholas U. Mayall Telescope is a four-meter (158 inches) reflector telescope in Arizona named after the American observational astronomer of the same name. The telescope saw first light on February 27, 1973, and was the second-largest in the world at that time.


Credit: NOIRLab/NSF/AURA/T.A. Rector (NSF NOIRLab/University of Alaska Anchorage) & H. Schweiker (WIYN/NSF NOIRLab) 
Release Date: Feb. 21, 2007

#NASA #Astronomy #Space #Science #Galaxies #IC342 #Caldwell5 #CamelopardalisConstellation #Cosmos #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education