Blue Ghost Mission 1 Moon Landing: 1-Year Anniversary | Firefly Aerospace
Learn more about CLPS: https://www.nasa.gov/clps
Duration: 2 minutes
Release Date: June 2, 2025
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Blue Ghost Mission 1 Moon Landing: 1-Year Anniversary | Firefly Aerospace
Learn more about CLPS: https://www.nasa.gov/clps
Spiral Galaxy NGC 941 in Cetus | Subaru Telescope
NGC 941 is a spiral galaxy about 55 million light-years away in the constellation Cetus. This faint galaxy is classified as an intermediate spiral, exhibiting characteristics between a barred spiral with a central bar and an unbarred spiral. Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars that extends from the core and leads into spiral arms. They account for about half of all known spiral galaxies, including the Milky Way.
NGC 941 has a diameter of approximately 55,000 light years. The galaxies NGC 926, NGC 934, NGC 936, NGC 955 are located in the same sky area. NGC 941 was discovered by German-British astronomer William Herschel on January 6, 1785.
#NASA #Astronomy #Space #Science #SubaruTelescope #すばる望遠鏡 #NAOJ #国立天文台 #HyperSuprimeCam #HSC #Galaxies #Galaxy #NGC941 #Galaxy #Supernovae #SN2005ab #CetusConstellation #Cosmos #Universe #Japan #日本 #MaunaKea #Hawaii #UnitedStates #STEM #Education
Aurora Australis over Western Australia
"Another one from [the] spectacular worldwide aurora event on May 11, 2024. This was taken at Stirling Dam, 1.5 hours south of Perth in Western Australia."
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.
Spiral Galaxy UGC 3912: A Suspected Galactic Encounter | Hubble
This Hubble Space Telescope image is of the spiral galaxy UGC 3912, located approximately 60–63 million light-years away in the constellation Canis Minor. It is classified as a spiral galaxy. However, UGC 3912’s distorted shape typically indicates a gravitational encounter with another galaxy. When galaxies interact—brushing up against each other’s gravitational fields or even collide— their stars, dust, and gas can be pulled into new paths. UGC 3912 may have been an organized-looking spiral once, but it looks like it has been smudged out of shape.
Fortunately, when galaxies interact, the individual stars and objects that orbit them remain whole even though their orbits can change so dramatically that the entire galaxy’s shape is altered. This is because the distances between stars in galaxies are so vast that they do not crash into one another, just continue serenely along their new orbits.
Astronomers have been studying UGC 3912 as part of an investigation into supernovae activity—when stars at least eight times larger than our Sun explode at the end of their lives. Hubble is examining one of the several types of supernovae, a hydrogen-rich phenomenon known as Type II. Though ample Type II supernovae have been observed, they exhibit enormous diversity in their brightness and spectroscopy and are not well understood.
Image Description: "A scattered grouping of blue and violet stars shines near the lower half of the image. Distant galaxies fill the black background of space, and bright stars with diffraction spikes are visible throughout."
The Hubble Space Telescope is a partnership between the European Space Agency (ESA) and NASA.
Aurora at Dawn | International Space Station
NASA astronaut and former International Space Station flight engineer Don Pettit shared this photo. 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.
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.
Cosmonaut Photos: The Bahamas | International Space Station
These images were shared by Expedition 74 Station Commander and Cosmonaut Sergey Kud-Sverchkov of Russia aboard the International Space Station: "Let's brighten up the cold, snowy days with the turquoise waters of a tropical sea! 🏝 This time, let's take a look at the Bahamas. Honestly, it's hard to tear your eyes away from the Bahamas (or Lucayan Islands, as they're also known)—the colors and shapes are so amazing . . . Have a nice day everyone!"
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.
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.
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
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.
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.
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.
#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
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.
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.
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.
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.
#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
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.
'Double Boomerang' Galaxy PKS 2014−55 | South Africa's MeerKAT Radio Telescope
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/