Sunday, March 01, 2026

Aurora Borealis over Sweden

Aurora Borealis over Sweden

Photographer P-M Hedén: "Such a lovely landscape by the east coast of Sweden. Very low water at the moment so we were standing on ground that normally is below water. And a little surprise with lovely Aurora in the icy landscape. Very cold, but very beautiful. 60 degrees latitude."

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

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

Sweden, formally the Kingdom of Sweden, is a Nordic country located on the Scandinavian Peninsula in Northern Europe. It borders Norway to the west and north, and Finland to the east.

Image Credit: P-M Hedén
Location: Norrtälje, Nothamn, Sweden 
P-M Hedén's website: https://www.nattbilder.se
Release Date: Feb. 14, 2026

#NASA #Astronomy #Space #Science #Planets #Earth #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Star #Photography #PMHedén #Photographer #CitizenScience #Norrtälje #Nothamn #Sweden #Sverige #STEM #Education

Planet Saturn & Moon Enceladus: Animation of Electrodynamic Interactions

Planet Saturn & Moon Enceladus: Animation of Electrodynamic Interactions

Animation of electrodynamic interactions between planet Saturn and moon Enceladus. The primary Alfvén wing is shown in blue, and the reflected Alfvén wings in magenta. The arrow indicates the corotation direction of the Enceladus plasma torus. Relative sizes of Saturn and Enceladus are not to scale. In plasma physics, an Alfvén wave, named after Hannes Alfvén, is a type of plasma wave in which ions oscillate in response to a restoring force provided by an effective tension on the magnetic field lines. Enceladus is the sixth-largest moon of Saturn and the 18th largest in the Solar System. It is about 500 kilometers (310 miles) in diameter, about a tenth of that of Saturn's largest moon, Titan.

NASA's Cassini spacecraft's up-close Grand Finale orbit showed a surprisingly powerful and dynamic interaction of plasma waves moving from Saturn to its rings and its moon Enceladus. The observations showed for the first time that the waves travel on magnetic field lines connecting Saturn directly to Enceladus. The field lines are like an electrical circuit between the two bodies with energy flowing back and forth. Much like air or water, plasma (the fourth state of matter) generates waves to carry energy. The Radio Plasma Wave Science (RPWS) instrument on board NASA's Cassini spacecraft recorded intense plasma waves during one of its closest encounters at Saturn.

"Enceladus is this little generator going around Saturn, and we know it is a continuous source of energy," said Ali Sulaiman, planetary scientist at the University of Iowa, Iowa City, and a former member of the RPWS team. "Now we find that Saturn responds by launching signals in the form of plasma waves, through the circuit of magnetic field lines connecting it to Enceladus hundreds of thousands of miles away."

The interaction of Saturn and Enceladus is unlike the relationship between Earth and its Moon. Enceladus is immersed within Saturn's magnetic field and is geologically active, emitting plumes of water vapor that become ionized and fill the environment around Saturn. Our own Moon does not interact in the same way with Earth. Similar interactions take place between Saturn and its rings, as they are also very dynamic.

Enceladus is covered by clean, freshly deposited snow hundreds of meters thick, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon reaches only −198 °C (75.1 K; −324.4 °F), far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide variety of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain. Enceladus was discovered on August 28, 1789, by William Herschel.

NASA's Cassini spacecraft arrived in the Saturn system in 2004 and ended its mission in 2017 by deliberately plunging into Saturn's atmosphere. This method was chosen because it is necessary to ensure protection and prevent biological contamination to any of the moons of Saturn thought to offer potential habitability.

The Cassini-Huygens mission was a cooperative project of NASA, European Space Agency (ESA) and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, managed the mission for NASA's Science Mission Directorate, Washington. JPL designed, developed and assembled the Cassini orbiter. The RPWS instrument was built by the University of Iowa, working with team members from the U.S. and several European countries.

NASA's Cassini Mission: 
https://solarsystem.nasa.gov/cassini


Video Credits: Europlanet
Design & Animation: Fabrice Etifier, École Polytechnique
Duration: 20 seconds
Release Date: Feb. 9, 2026

#NASA #FoN #Astronomy #Space #Science #Planet #Saturn #Moons #Enceladus #ElectrodynamicInteractions #Astrobiology #SolarSystem #CassiniMission #CassiniSpacecraft #JPL #Caltech #UnitedStates #ESA #Italy #Italia #ASI #Europe #History #STEM #Education #Animation #HD #Video

Earthgazing | NASA Crew-12 Commander, Astronaut & Scientist Jessica Meir

Earthgazing | NASA Crew-12 Commander, Astronaut & Scientist Jessica Meir


Expedition 74 Flight Engineer and NASA Astronaut Jessica Meir: "In awe to be gazing down on our precious blue gem from above once again. Here are some of my first views out of the SpaceX Dragon window . . . Hello Earth!"

NASA astronaut Jessica Meir is the commander of NASA’s SpaceX Crew-12 mission. This is her second spaceflight. After her arrival to the International Space Station, she joined Expedition 74/75, kicking off a long-duration science expedition aboard the orbiting laboratory. She was selected as a NASA astronaut in 2013. The Caribou, Maine, native earned a bachelor’s degree in biology Brown University, a master’s degree in space studies from the International Space University, and a doctorate in marine biology from Scripps Institution of Oceanography in San Diego. 

On her first spaceflight, Meir spent 205 days as a flight engineer during Expedition 61/62, and she completed the first three all-woman spacewalks with fellow NASA astronaut Christina Koch, totaling 21 hours and 44 minutes outside of the station. Since then, she has served in various roles, including assistant to the chief astronaut for commercial crew (SpaceX), deputy for the Flight Integration Division, and assistant to the chief astronaut for the human landing system.

NASA Astronaut/Dr. Jessica Meir's Biography:
https://www.nasa.gov/people/jessica-u-meir/


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.

Credit: NASA's Johnson Space Center/Jessica Meir
Image Date: Feb. 14, 2026
Release Date: Feb. 23, 2026

#NASA #Space #ISS #Earth #OverviewEffect #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

Comet C/2024 E1 (Wierzchos): View from Namibia

Comet C/2024 E1 (Wierzchos): View from Namibia

C/2024 E1 (Wierzchoś) is a hyperbolic Oort cloud comet, discovered on March 3, 2024 by Polish astronomer Kacper Wierzchoś. It reached perihelion (closest approach to the Sun) on January 20, 2026, with apparent magnitude of around +6.5, visible in larger binoculars. It has a highly eccentric orbit with an inbound orbital period of millions of years and an outbound orbit of around 200,000 years. Cometary emission activity for C/2024 E1 has been driven by carbon dioxide (CO2) outgassing. It crossed the celestial equator on November 17, 2025. As of February 15, 2026, the comet is about apparent magnitude 7.

Namibia, officially the Republic of Namibia, is a country in southern Africa. Its borders include the Atlantic Ocean to the west, Angola and Zambia to the north, Botswana to the east and South Africa to the south; in the northeast, approximating a quadripoint, Zimbabwe lies less than 200 meters (660 feet) away along the Zambezi River near Kazungula, Zambia.


Image Credit: Gerald Rhemann and Michael Jäger
Telescope: ASA Astrograph 12" f3.6 Camera: ZWO ASI 6200 MM Pro Exp.Time: LRGB 7.8/5/5/5 min
Location: Farm Tivoli, Namibia
Image Date: Feb. 2, 2026

#NASA #Astronomy #Space #Science #Comets #C2024E1Wierzchoś #OortCloud #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #GeraldRhemann #MichaelJäger #Astrophotographers #FarmTivoli #Namibia #Africa #STEM #Education

China's "Space Mouse" Births Third Healthy Litter | China Space Station

China's "Space Mouse" Births Third Healthy Litter | China Space Station


A female mouse that spent time aboard China's Tiangong Space Station last year has birthed her third consecutive healthy litter back on Earth, providing scientists with invaluable data on mammalian reproduction after spaceflight. Four mice were sent to the Tiangong space station as part of the Shenzhou-21 mission on Oct. 31, 2025, marking China's first small-mammal experiment in orbit. The rodents spent approximately two weeks in a specialized habitat in microgravity conditions before returning to Earth on Nov. 14, 2025.

Shortly after their return, one female conceived and delivered her first litter of nine pups on Dec. 10. She has since birthed two additional healthy litters, the second of which resulted in 10 pups and the third in another nine.

"What we see now are the male mouse and female mouse that returned from space mission. This is the first litter of male and female pups born on Dec. 10, 2025. This is the second litter of male and female pups, born to our space mice on Jan. 5 of this year. Currently, the third litter has also been born. They were born on Feb. 18 of this year and are still in the nursing period, so they are being housed in the same cage as the female space mouse," said Wang Yixi, an engineer at the Institute of Zoology (IOZ) of the Chinese Academy of Sciences (CAS).

Researchers at the Institute of Zoology have observed intriguing behavioral variations across the three litters.

The first exhibited more cautious, "socially anxious" behavior, hiding in sheltered areas frequently. The second showed greater confidence, exploring their environment more readily. By the third litter, the offspring demonstrated progressively improved adaptation to ground living conditions, according to the report.

Overall, each successive litter has shown improved adaptation to ground living conditions compared to the previous one. These subtle changes provide important evidence for the study of space life reproduction, according to the researchers.

"The pups from the second litter, born on Jan. 5, are now showing less fear of people. They build their own cotton-made nest in the red room, but unlike the first litter, they don't drag all the cotton into the red room. They spend more time foraging for food freely and are more active. This also indicates that our mice are gradually adapting to the ground environment with each generation," Wang said.

The size of each litter has exceeded typical terrestrial litters of five to seven pups, China Media Group reported on Saturday.

"Normally, our strain of mice can have only five to seven pups per litter. However, the female mouse that returned from space station had nine pups in her first litter, 10 in her second, and nine in her third, significantly more than the offspring produced by our ground mice that have never been to space. We will also analyze the hormone levels and some blood parameters of the mice, hoping to uncover more mechanisms from these observations," said Li Tianda, associate researcher at the Institute of Zoology.

Mice have approximately 85 percent genetic similarity to humans and have rapid reproductive cycles, making them ideal models for the study of potential risks to human reproduction during long-term space missions.

Researchers will continue to monitor these "space pups" closely, tracking growth curves and testing whether they themselves can reproduce normally, searching for potential generational impacts.

According to the research plan, the scientific team will conduct longer-duration space experiments with mice, mirroring human orbital missions that last over six months to study their physiological responses and spatial adaptability, per the report.


Video Credit: CCTV
Duration: 2 minutes
Release Date: March 1, 2026

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

Saturday, February 28, 2026

Comet C/2024 E1 (Wierzchos): View from Chile

Comet C/2024 E1 (Wierzchos): View from Chile

Astrophotographer Alan Tough: "Captured remotely from Chile on February 7th at 10:03 p.m. local time."

C/2024 E1 (Wierzchoś) is a hyperbolic Oort cloud comet, discovered on March 3, 2024 by Polish astronomer Kacper Wierzchoś. It reached perihelion (closest approach to the Sun) on January 20, 2026, with apparent magnitude of around +6.5, visible in larger binoculars. It has a highly eccentric orbit with an inbound orbital period of millions of years and an outbound orbit of around 200,000 years. Cometary emission activity for C/2024 E1 has been driven by carbon dioxide (CO2) outgassing. It crossed the celestial equator on November 17, 2025. As of February 15, 2026, the comet is about apparent magnitude 7.


Image Credit: Alan Tough
Release Date: Feb. 28, 2026

#NASA #Astronomy #Space #Science #Comets #C2024E1Wierzchos #OortCloud #SolarSystem #MilkyWayGalaxy #Cosmos #Universe #Astrophotography #AlanTough #Astrophotographers #Chile #STEM #Education

Aurora Borealis by Moonlight over Norway

Aurora Borealis by Moonlight over Norway



Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

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: Ivar Sandland
Location: Bodø, Northern Norway
Image Details: Clear skies once again. 60% waxing gibbous Moon. Sony A7IV. Sony GM 14mm F1.8 1.3sec/ISO 1250
Ivar's website: https://en.nordlandturselskap.no
Date: Feb. 24, 2026

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

Antlia Dwarf Galaxy Peppers the Sky with Stars | Hubble Space Telescope

Antlia Dwarf Galaxy Peppers the Sky with Stars | Hubble Space Telescope

The myriad faint stars that comprise the Antlia Dwarf galaxy are more than four million light-years from Earth, but this NASA/European Space Agency Hubble Space Telescope image offers such clarity that they could be mistaken for much closer stars in our own Milky Way. This very faint and sparsely populated small galaxy was only discovered in 1997.

Although small, the Antlia Dwarf is a dynamic site featuring stars across many stages of evolution, from young to old. The freshest stars are only found in the central regions where there is significant ongoing star formation. Older stars and globular clusters are found in the outer areas.

It is not entirely clear whether the Antlia Dwarf is a member our galactic neighborhood, called the Local Group. It probably lies just beyond the normally accepted outer limits of the group. Although it is fairly isolated, some believe it has interacted with other star groups. Evidence comes from galaxy NGC 3109, close to the Antlia Dwarf (but not visible in this image). Both galaxies feature rifts of stars moving at comparable velocities; a telltale sign that they were gravitationally linked at some point in the past.

This picture was created from observations in visible and infrared light taken with the Wide Field Channel of Hubble’s Advanced Camera for Surveys. The field of view is approximately 3.2 by 1.5 arcminutes.


Credit: ESA/Hubble & NASA
Release Date: Feb. 27, 2012

#NASA #ESA #Astronomy #Space #Science #Galaxies #DwarfGalaxies #AntliaDwarfGalaxy #InteractingGalaxies #NGC3109 #AntliaConstellation #Cosmos #Universe #HubbleSpaceTelescope #HST #Europe #GSFC #STScI #UnitedStates #STEM #Education

ʻOumuamua' Visualization—First Known Interstellar Object to Visit Solar System

ʻOumuamua' Visualization—First Known Interstellar Object to Visit Solar System

A visualization of 'Oumuamua', the first known interstellar object detected passing through our Solar System. This cosmic wanderer may have been traveling for billions of years before astronomers spotted it. Interstellar comet 3I/ATLAS raced through our solar system at 130,000 miles per hour. It was only the third interstellar object ever discovered.

Interstellar objects are objects that originate outside of, and are observed passing through, our Solar System. Ranging from tens of meters to a few kilometers in size, these objects are pieces of cosmic debris leftover from the formation of their host star’s planetary systems. As these remnants orbit their star, the gravity of nearby larger planets and passing nearby stars can launch them out of their home systems and into interstellar space, where they can cross paths with other solar systems.

When discovered, it was about 410 million miles (670 million kilometers) away from the Sun, within the orbit of Jupiter. The origin of Comet 3I/ATLAS remains unknown. Since this is the third interstellar object ever discovered, its name begins with the number 3 and the letter I. Comet 3I/ATLAS posed no known threat to Earth. Meanwhile, it has provides a fascinating and rare opportunity for scientists to study these interstellar interlopers.


Credit: NOIRLab/NSF/AURA/T. Matsopoulos/ESO/M. Kornmesser
Duration: 1 minute
Release Date: Feb. 9, 2026

#NASA #Astronomy #Space #Science #InterstellarObjects #InterplanetaryBodies #Comets #InterstellarComet3I #3IATLAS #SolarSystem #Planets #Cosmos #Universe #NOIRLab #NSF #AURA #UnitedStates #STEM #Education #HD #Video

'Double Boomerang' Galaxy PKS 2014−55 | South Africa's MeerKAT Radio Telescope

'Double Boomerang' Galaxy PKS 2014−55 South Africa's MeerKAT Radio Telescope

The detail provided in this radio image obtained with the MeerKAT telescope indicates that this galaxy's shape is best described as a ‘double boomerang’. Two powerful jets of radio waves, indicated in blue color, each extend 2.5 million light years into space (comparable to the distance between the Milky Way and the Andromeda galaxy, our nearest major neighbor). Eventually, they are ‘turned back’ by the pressure of tenuous intergalactic gas. As they flow back towards the central galaxy, they are deflected by its relatively high gas pressure into the shorter, horizontal, arms of the boomerang. The background image shows visible light from myriad galaxies in the distant universe. 
Annotated image showing X-shaped giant radio galaxy PKS 2014-55, observed with the South African Radio Astronomy Observatory’s MeerKAT telescope, indicating the old X-shaped radio jets, the younger jets closer to the central black hole, and the region of influence dominated by the central galaxy’s stars and gas. The curved arrows denote the direction of the backflow that forms the horizontal components of the X.

PKS 2014−55 is a Seyfert 2 elliptical galaxy presenting strong emission lines. It is an X-shaped radio galaxy discovered by the MeerKAT radio telescope in South Africa that is located 800 million light-years away from Earth. A radio galaxy is a galaxy with giant regions of radio emission extending well beyond its visible structure. These energetic radio lobes are powered by jets from its active galactic nucleus. This galaxy has jets extending 2.5 million light years across. Then the jets are “reversed” by the pressure of intergalactic gas, later deflected by gas pressure to form an “X” shape.

Many galaxies far more active than the Milky Way have enormous twin jets of radio waves extending far into intergalactic space. Normally, these go in opposite directions, coming from a massive black hole at the center of the galaxy. However, a few are more complicated and appear to have four jets forming an ‘X’ on the sky.

Several possible explanations have been proposed to understand this phenomenon. These include changes in the direction of spin of the black hole at the centre of the galaxy, and associated jets, over millions of years; two black holes each associated with a pair of jets; and material falling back into the galaxy being deflected into different directions forming the other two arms of the ‘X’. MeerKAT observations of one such galaxy, PKS 2014-55, strongly favor the latter explanation as they show material “turning the corner” as it flows back towards the host galaxy.

This work was carried out by a team from the South African Radio Astronomy Observatory (SARAO), the (US) National Radio Astronomy Observatory (NRAO), the University of Pretoria, and Rhodes University.

Previous studies of these unusual galaxies lacked the high quality imaging provided by the MeerKAT telescope. This telescope array consists of 64 radio dishes located in the Karoo semi-desert in the Northern Cape province of South Africa. Computers combined the data from these antennas into a telescope 8 km in diameter, and provided images in the radio band of unprecedented quality for PKS 2014-55 which enabled solving the mystery of its shape. 

The South African Radio Astronomy Observatory (SARAO), a facility of the National Research Foundation, is responsible for managing all radio astronomy initiatives and facilities in South Africa, including the MeerKAT radio telescope in the Karoo, and the geodesy and VLBI activities at the HartRAO facility. 

Learn more about MeerKAT: https://www.sarao.ac.za/science/meerkat/


Image Credit: South African Radio Astronomy Observatory (SARAO)/NRAO/AUI/NSF/DES
Release Date: May 7, 2020

#NASA #Astronomy #Space #Science #Stars #Galaxies #EllipticalGalaxies #PKS201455 #BlackHoles #TelescopiumConstellation #Cosmos #Universe #MeerKATRadioTelescope #RadioAstronomy #SARAO #SouthAfrica #NRAO #AUI #NSF #DES #UnitedStates #STEM #Education

Radio Astronomy: ALMA Antennas in The Atacama Desert of Northern Chile

Radio Astronomy: ALMA Antennas in The Atacama Desert of Northern Chile








The Atacama Large Millimeter/submillimeter Array (ALMA) is a powerful astronomical observatory located in the Atacama Desert of northern Chile, consisting of 66 high-precision antennas at an altitude of 5,000 meters (16,400 feet) that study the universe in millimeter and submillimeter wavelengths. ALMA antennas can be seen here on the Chajnantor Plateau (including after a snowstorm) during the Andean winter of 2026.

Radio telescopes look toward the heavens to view planets, comets, giant clouds of gas and dust, stars, and galaxies. By studying the radio waves originating from these sources, astronomers can learn about their composition, structure, and motion. Radio astronomy has the advantage that sunlight, clouds, and rain do not affect observations.

What is ALMA?
ALMA is an astronomical interferometer designed to observe electromagnetic radiation at millimeter and submillimeter wavelengths. It is composed of 66 radio telescopes situated on the Chajnantor Plateau at an altitude of 5,000 meters (16,400 feet), making it one of the highest astronomical observatories in the world. This location was chosen for its high elevation and low humidity, which are crucial for reducing atmospheric noise and improving signal quality. 

ALMA's primary goal is to study the cold, dark regions of the universe that are invisible to optical telescopes. It provides insights into various astronomical phenomena, including:

Star and Planet Formation: ALMA can penetrate dust clouds to reveal the processes involved in the birth of stars and planetary systems. 

Galaxy Evolution: The array allows astronomers to observe distant galaxies and understand their formation and development over cosmic time. 

Chemical Composition: ALMA helps in studying the complex molecules present in interstellar gas and dust, providing clues about the chemistry of the universe. 

Recent Discoveries
ALMA has been instrumental in significant astronomical discoveries, such as pinpointing the moment when planets began to form around stars beyond our solar system. It has also contributed to understanding the early universe by observing the first stars and galaxies that emerged after the cosmic "dark ages". 

ALMA is an international partnership that includes the European Southern Observatory (ESO), the U.S. National Science Foundation, along with institutions from Japan, Canada, South Korea, and Chile. With its advanced technology and favorable observing location, ALMA continues to be a leading facility in radio astronomy, providing valuable data that expands our understanding of the cosmos.


Image Credits: Sergio Otarola, Yerko Villalon
Dates: Feb. 3-26, 2026

#NASA #Astronomy #RadioAstronomy #Science #Space #Nebulae #Stars #Planets #Asteroids #Comets #Galaxies #MilkyWayGalaxy #Cosmos #Universe #ALMA #ChajnantorPlateau #AtacamaDesert #Chile #ESO #Europe #UnitedStates #STEM #Education

Aurora Australis: View from Western Australia

Aurora Australis: View from Western Australia

Photographer Trevor Dobson: "This is a rare (for me!) single shot image of the Aurora Australis taken during the worldwide aurora event of May 11, 2024."

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Image Credit: Trevor Dobson
Location: Stirling Dam, Western Australia
Image Details: Nikon d5500, 13mm, ISO 500, f/4, 30 seconds
Image Date: May 11, 2024
Release Date: Feb. 28, 2026

#NASA #Space #Astronomy #Science #SolarSystem #Earth #Aurora #AuroraAustralis #Science #CitizenScience #Astrophotographer #TrevorDobson #Astrophotography #StirlingDam #WesternAustralia #Australia #STEM #Education

China Preps for 2030 Crewed Moon Landings, Confirms Human Spaceflight Progress

China Preps for 2030 Crewed Moon Landings, Confirms Human Spaceflight Progress

China has announced several milestones in its space program with six manned flights, four cargo resupply missions, and seven spacecraft returns completed. The Tiangong Space Station has hosted 18 astronauts for extended stays, completing 13 spacewalks and breaking world records for the longest single spacewalk by Chinese astronauts Cai Xuzhe and Song Lingdong on December 17, 2024.

Training for the fourth batch of ten astronaut candidates, including pilots and payload specialists from Hong Kong and Macau for the first time, began in late 2024 with participation in space station missions expected by 2026.

China is on track for its first crewed Moon landing by 2030 with progress on the Long March 10 rocket, Mengzhou spacecraft, and Lanyue lunar lander. Meanwhile, the follow-up Chang'e-7 mission to the Moon, expected to be launched in August 2026, will search for water ice at the lunar south pole using a "hopping" probe.

An astronaut training agreement was also signed with Pakistan as part of China’s effort to promote international cooperation for its International Lunar Research Station (ILRS). China remains open to collaborative projects for its Tiangong Space Station. It could become the only one left when the NASA-led International Space Station retires between 2030 and 2032.


Video Credit: SMG
Duration: 1 minute, 16 seconds
Release Date: Feb. 28, 2026

#NASA #Space #Science #China #中国 #Moon #ILRS #MengzhouSpacecraft #梦舟 #Lanyuelunarlander #揽月 #CrewSpacecraft #LongMarch10 #长征十号 #ReusableRockets #ChinaMannedSpaceAgency #中华人民共和国 #HumanSpaceflight #LunarMissions #Taikonauts #Astronauts #SpaceTechnology #SpaceExploration #STEM #Education #HD #Video

SpaceX CRS-33 Cargo Dragon Spacecraft Departure | International Space Station

SpaceX CRS-33 Cargo Dragon Spacecraft Departure | International Space Station





A SpaceX Dragon spacecraft departed the International Space Station on February 26, 2026, carrying several thousand pounds of science experiments and lab hardware for return and analysis on Earth. Dragon completed a six-month stay attached to the Harmony module's forward port where it docked in August 2025 delivering over 5,500 pounds of new science, supplies, and hardware to resupply the orbital residents.

Dragon parachuted to a splashdown in the Pacific Ocean off the coast of California at 11:44 p.m. PST on Thursday where NASA and SpaceX support personnel awaited the science and cargo-packed spacecraft. This marked the completion of SpaceX’s 33rd Commercial Resupply Services (CRS-33) mission to the International Space Station.

Expedition 74 Flight Engineer and NASA Astronaut: "A view of a (cargo) Dragon from a (crew) Dragon. The SpaceX cargo Dragon 33 vehicle departed from the International Space Station today. We’ve been busy packing it full of experiment samples, hardware, and items that need to be returned to Earth. Goodbye Dragon! Thanks for your hefty delivery to the ISS, you served us well!"

Learn more about NASA's Commercial Resupply Missions:
https://www.nasa.gov/international-space-station/commercial-resupply/


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/Jessica Meir
Date: Feb. 26, 2026

#NASA #Space #ISS #Science #Earth #SpaceX #CargoDragonSpacecraft #CRS33 #Astronauts #JessicaMeir #UnitedStates #France #Europe #ESA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #InternationalCooperation #Expedition74 #JSC #STEM #Education

Friday, February 27, 2026

Northern Lights over Finland

Northern Lights over Finland

Photographer Elmar Junker: "Best I ever saw. Dynamic, over whole sky. Samsung S23 in night mode."

Also known as the northern lights (aurora borealis) or southern lights (aurora australis), auroras are colorful, dynamic, and often visually delicate displays of an intricate dance of particles and magnetism between the Sun and Earth called space weather. When energetic particles from space collide with atoms and molecules in the atmosphere, they can cause the colorful glow that we call auroras.

Learn more about auroras: 
https://science.nasa.gov/sun/auroras/

Finland is a Nordic country in Northern Europe. It borders Sweden to the northwest, Norway to the north, and Russia to the east, with the Gulf of Bothnia to the west and the Gulf of Finland to the south, opposite Estonia.

Image Credit: Elmar Junker
Location: Äkäslompolo, Finland
Release Date: Feb. 14, 2026

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China Preparing for Crewed Moon Landings by 2030

China Preparing for Crewed Moon Landings by 2030

China is gearing up for crewed Moon landings by 2030. The China Manned Space Agency (CMSA) says key projects, including the Long March 10 rocket, Mengzhou spacecraft, and Lanyue lander, are progressing smoothly.

A low-altitude demonstration and verification flight test for the Long March-10 carrier rocket and a maximum dynamic pressure abort flight test for the new-generation crewed spaceship system Mengzhou were successfully conducted at the Wenchang Spacecraft Launch Site in south China's Hainan province on Feb. 11, 2026.

Zhou Jianping, chief designer of China's crewed space program, underscored the significance of these successful tests.

"This was a highly significant flight test, especially the retrieval technologies, which are entirely new to us. Achieving success on the very first attempt represents a leapfrog development," said Zhou.

"This laid the foundation for completing verification flights for the crewed lunar exploration program, and eventually, lunar landings. Efforts to build the equipment and facilities required for a comprehensive launch and test system are progressing as planned. It is estimated that by the end of this year, China will fully achieve testing and launch capabilities for the crewed lunar exploration program," said Zhong.

It was the first ignition flight of the Long March-10 rocket, and saw the spacecraft power through Max Q—the most dangerous phase of ascent, when aerodynamic stress reaches its peak.

Both the return capsule and the rocket's first stage landed in their designated recovery zones.

It was also the first completion of a sea landing and recovery of Mengzhou's return capsule that will bring China's spacefarers back to earth.

Mengzhou, meaning "Dream Vessel" in Chinese, is designed mainly for China's crewed lunar exploration but can also be used for space station operations. Its return capsule is capable of multiple reuses.

"We have successfully achieved a soft splashdown and retrieval from the sea. This marks a crucial and significant breakthrough in China's reusable carrier rocket technology and will also greatly promote the upgrading of China's carrier rocket technology," said Wang Zhifei, a researcher at China Aerospace Science and Technology Corporation.


Video Credit: CGTN
Duration: 33 seconds
Release Date: Feb. 27, 2026

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