Friday, April 11, 2025

Dark Energy Breakthrough Sheds New Light on Universe's Accelerated Expansion

Dark Energy Breakthrough Sheds New Light on Universe's Accelerated Expansion

Chinese and international astronomers have achieved a breakthrough in dark energy research, offering fresh insights into the physical mechanisms behind the accelerated expansion of the universe.

The findings, announced by the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) on Wednesday, April 9, 2025, suggest potential new physics beyond the standard cosmological model.

Dark energy remains one of the most profound mysteries in modern physics. Since the discovery of accelerated cosmic expansion in the late 1990s, scientists have attributed this phenomenon to an enigmatic cosmic component called dark energy. Yet its true nature remains a mystery.

The standard cosmological model interprets dark energy as a static vacuum energy. While successfully explaining a large number of cosmological observations for over two decades, recent advancements in observational precision have exposed inconsistencies among different datasets under this framework, challenging its completeness and opening avenues for alternative theories.

Leading this quest is the Dark Energy Spectroscopic Instrument (DESI), a global collaboration involving over 70 institutions. Utilizing a four-meter optical telescope, DESI maps the universe's 3D large-scale structure by measuring redshifts of tens of millions of celestial objects.

The Galaxy Survey and Cosmology Group at NAOC, led by Zhao Gongbo, and the Wide-field Survey and Galaxy Physics Group at NAOC, led by Zou Hu, have been involved in the DESI project for over a decade.

In the latest study, Zhao's team, leading the DESI collaboration, has achieved significant breakthroughs in the dynamical properties of dark energy.

By employing a novel methodology independently developed by the researchers, the team conducted an in-depth analysis of the latest cosmological distance measurements from DESI observations, combined with data from supernovae and cosmic microwave background radiation. Their findings revealed that the equation of state for dark energy changes as the universe evolves.

This result confirms the previous conclusion of the DESI collaboration derived through distinct analytical approaches, that dark energy is likely to have dynamic properties. The conclusion implies that dark energy may not be a constant vacuum energy, but rather exhibits more complex evolutionary behavior.

The study not only pioneers new research pathways for unraveling the physical essence of dark energy, but also provides pivotal clues for constructing a more comprehensive theoretical framework in cosmology.

"The standard cosmological model suggests that dark energy is the vacuum energy proposed by Einstein over a century ago. Like vaccum energy, dark energy was assumed to be constant over time. However, we have found evidence that dark energy evolves over time, disproving the idea that vacuum energy could be a form of dark energy. Such a discovery would represent a revolutionary breakthrough in fundamental physics," said Zhao.

DESI, managed by the U.S. Department of Energy's Lawrence Berkeley National Laboratory, involves more than 900 researchers from 70 institutions worldwide.


Video Credit: CCTV
Duration: 1 minute
Release Date: April 11, 2025

#NASA #Astronomy #Space #Science #Galaxies #Astrophysics #Cosmology #CosmologicalModels #DarkEnergy #DarkMatter #GravitationalLensing #Cosmos #Universe #DESI #UnitedStates #China #中国 #NAOC #STEM #Education #Visualization #HD #Video

Side Boosters for NASA's Artemis II SLS Moon Rocket Complete

Side Boosters for NASA's Artemis II SLS Moon Rocket Complete

With stacking of the right-hand forward assembly, the Space Launch System (SLS) solid rocket boosters for NASA's Artemis II mission are complete. The 17-story-tall twin boosters provide more than 75% of thrust at liftoff from NASA Kennedy’s Launch Pad 39B. Next to stack on mobile launcher 1 is the core stage, currently inside the Vehicle Assembly Building (VAB) at NASA's Kennedy Space Center in Florida.

The Artemis II test flight will be sending NASA astronauts Victor Glover, Christina Koch, and Reid Wiseman, as well as Canadian Space Agency (CSA) astronaut Jeremy Hansen, on a ten-day journey around the Moon and back.

Artemis II will launch no earlier than April 2026.

Check the NASA Artemis II Mission page for updates:

Learn more about NASA's Space Launch System (SLS) rocket: nasa.gov/sls

Follow updates on the Artemis blog: 

Credit: NASA
Duration: 1 minute, 26 seconds
Release Date: April 11, 2025

#NASA #ESA #Space #Moon #ArtemisProgram #ArtemisII #CrewedMission #Astronauts #NASASLS #SpaceLaunchSystem #SRB #DeepSpace #MoonToMars #Science #SpaceEngineering #SpaceTechnology #HumanSpaceflight #SolarSystem #SpaceExploration #NorthropGrumman #KSC #Florida #UnitedStates #Europe #STEM #Education #HD #Video

NASA's Space to Ground: Changing Space | Week of April 11, 2025

NASA's Space to Ground: Changing Space Week of April 11, 2025


NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. 

Updates: NASA Flight Engineer Don Pettit joined station Commander Alexey Ovchinin and Flight Engineer Ivan Vagner of Roscosmos (Russia), and checked their Sokol launch and entry suits for leaks. The trio wore the suits when they launched together aboard the Soyuz MS-26 crew ship and docked to the Rassvet module on Sept. 11, 2024. They will wear the suits again when they return to Earth on April 19, 2025, inside the Soyuz MS-26 completing a seven-month space research mission.

The next cargo mission from SpaceX is due to launch later this month replenishing Expedition 72 with new science experiments and crew supplies. Pettit and Kim worked together preparing for the Dragon spacecraft’s arrival gathering items for stowage aboard Dragon when it returns to Earth about four weeks later. Pettit also assisted Kim, who is in his third day aboard the orbital lab, as he worked out on the advanced resistive exercise device for the first time.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Roscosmos cosmonaut Alexey Ovchinin (Russia)
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy
NASA Flight Engineers: Don Pettit, 
Anne McClain, Nichole Ayers, Jonny Kim
JAXA Flight Engineer: Takuya Onishi

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.

Learn more about the important research being operated on Station:

For more information about STEM on Station:

Video Credit: NASA's Johnson Space Center
Duration: 4 minutes, 27 seconds
Release Date: April 11, 2025

#NASA #Space #ISS #Science #Astronauts #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #MicrogravityResearch #InternationalCooperation #Expedition72 #UnitedStates #STEM #Education #HD #Video

Thursday, April 10, 2025

Perseverance Rover Mars Sample#25: Sapphire Canyon | NASA/JPL

Perseverance Rover Mars Sample#25: Sapphire Canyon | NASA/JPL

Meet the 25th Martian sample collected by NASA’s Mars Perseverance rover—“Sapphire Canyon”—a sample taken from a vein-filled rock named “Cheyava Falls.” The arrowhead-shaped rock contains compelling features that may help answer whether Mars was home to microscopic life in the distant past. 

As of early April 2024, the Perseverance rover has collected and sealed 28 scientifically selected samples inside pristine tubes as part of the Mars Sample Return (MSR) campaign. The next stage is to get them to Earth for study. 

Considered one of the planetary science community’s highest priorities, MSR would be the first effort to bring back pieces of another planet and provides the best opportunity to answer fundamental questions about Mars' early evolution, its potential for ancient life, and its climate, while also unlocking mysteries that we have yet to even conceive. NASA is teaming with the European Space Agency (ESA) on this important endeavor. 

A key objective for Perseverance's mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet's geology and past climate, pave the way for human exploration of the Red Planet, as well as be the first mission to collect and cache Martian rock and regolith (broken rock and dust).

Read about all the carefully selected samples: https://science.nasa.gov/mission/mars-2020-perseverance/mars-rock-samples/

Learn more about the Mars Sample Return campaign: https://science.nasa.gov/mission/mars-sample-return/

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars


Video Credit: NASA's Jet Propulsion Laboratory (JPL)
Duration: 1 minute, 28 seconds
Release Date: April 10, 2025

#NASA #ESA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #PerseveranceRover #Mars2020 #SapphireCanyon #CheyavaFalls #MarsSampleReturn #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

NASA Espacio A Tierra | Preembarque para vuelos espaciales: 4 de abril de 2025

NASA Espacio A Tierra | Preembarque para vuelos espaciales: 4 de abril de 2025

Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional.

Aprende más sobre la ciencia a bordo de la estación espacial: https://www.nasa.gov/international-space-station/space-station-research-and-technology/ciencia-en-la-estacion/

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: 
https://www.nasa.gov/suscribete

Producción: NASA
Duration: 4 minute, 24 seconds
Release Date: April 10, 2025

#NASA #Space #ISS #Science #NASAenespañol #español #Astronauts #JonnyKim #Japan #日本 #JAXA #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #HumanSpaceflight #SpaceLaboratory #MicrogravityResearch #InternationalCooperation #Expedition72 #UnitedStates #STEM #Education #HD #Video

US & Russian Soyuz MS-27: See the Rocket? | International Space Station

US & Russian Soyuz MS-27 Launch: See the Rocket? | International Space Station

Soyuz MS-27 launch photographed by Expedition 72 flight engineer and cosmonaut Ivan Vagner of Russia from the International Space Station.

The Soyuz MS-27 spacecraft and its crew—NASA astronaut Jonny Kim, along with Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritskiy of Russia—successfully launched from the Baikonur Cosmodrome in Kazakhstan at 1:47 a.m. EDT (10:47 a.m. Baikonur time) on April 8, 2025, to the International Space Station. At 4:57 a.m. EDT, the Soyuz MS-27 spacecraft docked to the International Space Station’s Prichal module. 

The trio joined Expedition 72, including NASA astronauts Nichole Ayers, Anne McClain, and Don Pettit, Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, and Roscosmos cosmonauts Alexey Ovchinin, Kirill Peskov, and Ivan Vagner of Russia. The newly arrived crew members will spend approximately eight months aboard the orbital laboratory, returning to Earth in December 2025.

Less than two weeks after the new crew’s arrival, NASA Flight Engineer Don Pettit will return to Earth with Expedition 72 Commander Alexey Ovchinin and Flight Engineer Ivan Vagner. Ovchinin and Vagner are Roscosmos cosmonauts. The veteran crewmates will board the Soyuz MS-26 crew ship, undock from the Rassvet module, and parachute to a landing in the steppe of Kazakhstan less than three-and-a-half hours later ending a seven-month mission.

Japan Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi will take over command of the space station from Ovchinin the day before he leaves with Pettit and Vagner. Expedition 72 will end and Expedition 73 will officially begin the moment the Soyuz MS-26 undocks from Rassvet.

Expedition 72 Updates:

Expedition 72 Crew
Station Commander: Roscosmos cosmonaut Alexey Ovchinin (Russia)
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy
NASA Flight Engineers: Don Pettit, 
Anne McClain, Nichole Ayers, Jonny Kim
JAXA Flight Engineer: Takuya Onishi

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: Roscosmos/Cosmonaut Ivan Vagner
Capture Date: April 8, 2025

#NASA #Space #ISS #Science #Roscosmos #Роскосмос #SoyuzRocket #SoyuzMS27Spacecraft #Союз #BaikonurCosmodrome #Kazakhstan #Cosmonauts #SergeyRyzhikov #AlexeyZubritskiy #Astronaut #JonnyKim #HumanSpaceflight #UnitedStates #Russia #Россия #Expedition73 #SpaceLaboratory #STEM #Education

Have We Been to Planet Uranus? We Asked a NASA Expert

Have We Been to Planet Uranus? We Asked a NASA Expert

Have We Ever Been to Uranus? In 1986, NASA’s Voyager 2 spacecraft gave us our first and only close-up look at this ice giant. What it found was a bizarre, tilted world with extreme seasons, swirling methane clouds, narrow dusty rings and icy moons that could even hide oceans beneath their crusts.

Not only could Uranus hold clues about our own solar system but also the many similar-sized planets found throughout the galaxy.

A NASA scientist explains why Uranus is worth a second visit. 

Explore more about Uranus: https://science.nasa.gov/uranus/

Voyager 2, now in interstellar space, is almost 13 billion miles (21 billion kilometers) from Earth.

Learn more about NASA's Voyager 2 Mission:
https://science.nasa.gov/mission/voyager/voyager-2/

Credit: NASA
Producers: Scott Bednar, Pedro Cota, Jessie Wilde
Editor: Daniel Salazar
Duration: 1 minute, 49 seconds
Release Date: April 10, 2025

#NASA #Space #Astronomy #Science #Sun #SolarSystem #SolarWind #Planet #Uranus #Moons #MagneticField #Atmosphere #Voyager2Mission #Voyager2 #Voyager2Spacecraft #InterplanetarySpacecraft #UranusSystemFlyby #JPL #Caltech #UnitedStates #STEM #Education #HD #Video

NASA’s Perseverance Mars Rover Studies Trove of Rocks on Crater Rim | JPL

NASA’s Perseverance Mars Rover Studies Trove of Rocks on Crater Rim | JPL

This mosaic showing the Martian surface outside of Jezero Crater was taken by NASA’s Perseverance on Dec. 25, 2024, at the site where the rover cored a sample dubbed “Silver Mountain” from a rock likely formed during Mars’ earliest geologic period. 
Sealing the “Green Gardens” sample—collected by NASA’s Perseverance Mars rover from a rock dubbed “Tablelands” along the rim of Jezero Crater on Feb. 16, 2025—presented an engineering challenge. The sample was finally sealed on March 2, 2025.

The diversity of rock types along the rim of Jezero Crater offers a wide glimpse of Martian history.

Scientists with NASA’s Perseverance rover are exploring what they consider a veritable Martian cornucopia full of intriguing rocky outcrops on the rim of Jezero Crater. Studying rocks, boulders, and outcrops helps scientists understand the planet’s history, evolution, and potential for past or present habitability. Since January, the rover has cored five rocks on the rim, sealing samples from three of them in sample tubes. It has also performed up-close analysis of seven rocks and analyzed another 83 from afar by zapping them with a laser. This is the mission’s fastest science-collection tempo since the rover landed on the Red Planet more than four years ago.

Perseverance climbed the western wall of Jezero Crater for 3½ months, reaching the rim on Dec. 12, 2024, and is currently exploring a roughly 445-foot-tall (135-meter-tall) slope the science team calls “Witch Hazel Hill.” The diversity of rocks they have found there has gone beyond their expectations.

“During previous science campaigns in Jezero, it could take several months to find a rock that was significantly different from the last rock we sampled and scientifically unique enough for sampling,” said Perseverance’s project scientist, Katie Stack Morgan of NASA’s Jet Propulsion Laboratory in Southern California. “But up here on the crater rim, there are new and intriguing rocks everywhere the rover turns. It has been all we had hoped for and more.”

This is because Jezero Crater’s western rim contains tons of fragmented once-molten rocks that were knocked out of their subterranean home billions of years ago by one or more meteor impacts, including possibly the one that produced Jezero Crater. Perseverance is finding these formerly underground boulders juxtaposed with well-preserved layered rocks that were “born” billions of years ago on what would become the crater’s rim. And just a short drive away is a boulder showing signs that it was modified by water nestled beside one that saw little water in its past.

Oldest Sample Yet?
Perseverance collected its first crater-rim rock sample, named “Silver Mountain,” on Jan. 28. (NASA scientists informally nickname Martian features, including rocks and, separately, rock samples, to help keep track of them.) The rock it came from, called “Shallow Bay,” most likely formed at least 3.9 billion years ago during Mars’ earliest geologic period, the Noachian, and it may have been broken up and recrystallized during an ancient meteor impact.

About 360 feet (110 meters) away from that sampling site is an outcrop that caught the science team’s eye because it contains igneous minerals crystallized from magma deep in the Martian crust. (Igneous rocks can form deep underground from magma or from volcanic activity at the surface, and they are excellent record-keepers—particularly because mineral crystals within them preserve details about the precise moment they formed.) However, after two coring attempts (on Feb. 4 and Feb. 8) fizzled due to the rock being so crumbly, the rover drove about 520 feet (160 meters) northwest to another scientifically intriguing rock, dubbed “Tablelands.”

Data from the rover’s instruments indicates that Tablelands is made almost entirely of serpentine minerals, which form when large amounts of water react with iron- and magnesium-bearing minerals in igneous rock. During this process, called serpentinization, the rock’s original structure and mineralogy change, often causing it to expand and fracture. Byproducts of the process sometimes include hydrogen gas. This can lead to the generation of methane in the presence of carbon dioxide. On Earth, such rocks can support microbial communities.

Coring Tablelands went smoothly. Nevertheless, sealing it became an engineering challenge.

Flick Maneuver
“This happened once before, when there was enough powdered rock at the top of the tube that it interfered with getting a perfect seal,” said Kyle Kaplan, a robotics engineer at JPL. “For Tablelands, we pulled out all the stops. Over 13 sols,” or Martian days, “we used a tool to brush out the top of the tube 33 times and made eight sealing attempts. We even flicked it a second time.”

During a flick maneuver, the sample handling arm—a little robotic arm in the rover’s belly—presses the tube against a wall inside the rover, then pulls the tube away, causing it to vibrate. On March 2, the combination of flicks and brushings cleaned the tube’s top opening enough for Perseverance to seal and store the serpentine-laden rock sample.

Eight days later, the rover had no issues sealing its third rim sample, from a rock called “Main River.” The alternating bright and dark bands on the rock were like nothing the science team had seen before.

Up Next
Following the collection of the Main River sample, the rover has continued exploring Witch Hazel Hill, analyzing three more rocky outcrops (“Sally’s Cove,” “Dennis Pond,” and “Mount Pearl”). And the team isn’t done yet.

“The last four months have been a whirlwind for the science team, and we still feel that Witch Hazel Hill has more to tell us,” said Stack. “We’ll use all the rover data gathered recently to decide if and where to collect the next sample from the crater rim. Crater rims—you gotta love ’em.”

More About Perseverance
A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover is characterizing the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet and is the first mission to collect and cache Martian rock and regolith.

NASA’s Mars Sample Return Program, in cooperation with the European Space Agency (ESA), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Mars Exploration Program portfolio and the agency’s Moon to Mars exploration approach. This includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

NASA’s Jet Propulsion Laboratory, managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars


Credit: NASA/JPL-Caltech/ASU/MSSS
Release Date: April 10, 2025

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #STEM #Education

International Day of Women and Girls in Science 2025 | United Nations

International Day of Women and Girls in Science 2025 | United Nations

In celebration of International Day of Women and Girls in Science, 15 women astronauts were honored at ‘Uplifting Women in STEM’, an event hosted by the Permanent Mission of the Republic of Poland to the United Nations, RiseNow.US and Spotlight Initiative, at the United Nations in New York, February 11, 2025. The event highlighted the contributions of women and girls in science and the importance of ensuring that they are safe from gender-based violence and gender discrimination. Women in science tend to be at elevated risk for gender-based violence.


Image Credit: United Nations Spotlight Initiative / Radhika Chalasani
Image Date: Feb. 11, 2025
Release Date: April 9, 2025

#NASA #Space #Science #Astronomy #UnitedNations #UN #STEM #Education #Women #WomenInSTEM #Girls #GirlsInSTEM #Astronauts #NASAAstronauts #CadyColeman #CivilianAstronauts #CommercialAstronauts #SianProctor #SharonHagle #NewYorkCity #NewYork #UnitedStates #InternationalCooperation #UpliftingWomenInSTEM

Drier Lunar Far Side Offers Insight on Moon's Evolution: Chinese Study

Drier Lunar Far Side Offers Insight on Moon's Evolution: Chinese Study

The latest discovery from rock samples returned by China's Chang'e-6 lunar mission reveals that the Moon's mantle contains less water on the far side compared to the near side, suggesting that the "hidden hemisphere," that always faces away from Earth, tends to be much drier.

Published in the journal Nature on Wednesday, April 9, 2025, a new study by Chinese scientists found that the water content in each gram of the thick rocky layer beneath the Moon's far side surface is less than 2 micrograms, the lowest record ever reported.

Previous studies on samples from the lunar near side have shown that the water concentrations within the Moon's interior could reach up to 200 micrograms per gram.

"Currently, we have measured the water content in the basaltic mantle source region of Chang'e 6, and it is approximately less than 2 micrograms per gram. The result we have obtained from the near side of the Moon is around 7.5 micrograms per gram. This means that the water content in the mantle on the far side of the Moon is even lower than that on the near side," said Hu Sen, a research fellow from the Institute of Geology and Geophysics of the Chinese Academy of Sciences.The global scientific community widely believes that the Moon was formed when a Mars-sized object collided with Earth 4.5 billion years ago. During this extremely hot impact event, the Moon was thought to be depleted of water and other volatile elements.

Over the past two decades, there has been debate about whether the water content in the Moon's mantle, the middle layer between its surface and its core, is abundant or scarce, and all the published estimates were derived from the near side samples of the Moon.

The Chang'e-6 lunar probe, launched in early May 2024, landed in the Moon's South Pole-Aitken Basin and returned to Earth in late June with more than 1,935 grams of the first-ever samples from the less-known far side of the Moon.

The Moon samples used in this study weigh 5 grams, consisting of 578 particles ranging in size from 0.1 to 1.5 millimeters. These particles were carefully sieved and hand-selected, with 28 percent of them being mare basalt fragments.

The newly found disparity in the Moon's internal water content is of great significance. It may offer a fresh insight into the Moon's formation and evolution.

"The water on the Moon we are talking about is mostly water from the Moon's interior, which is related to the processes of its origin, evolution, and formation. Our country's Chang'e 7 mission will focus on issues related to lunar surface water in the future," said Hu.

The findings of this study also hold significant implications for future lunar exploration tasks, as water on the Moon is key to long-term human settlement.


Video Credit: CCTV
Duration: 55 seconds
Release Date: April 10, 2025

#NASA #CNSA #Space #Astronomy #Science #China #中国 #Moon #Change6 #嫦娥六号 #LunarSampleReturn #Change5 #嫦娥五号 #Geology #FarSide #WaterContent #H2O #SouthPole #NearSide #SpaceTechnology #SpaceResearch #SpaceExploration #SolarSystem #CLEP #InternationalCooperation #STEM #Education #HD #Video

Wednesday, April 09, 2025

Antarctica at The Terminator | Fram2 Mission to Earth's Poles | SpaceX

Antarctica at The Terminator | Fram2 Mission to Earth's Poles | SpaceX

Fram2 Mission Specialist and Medical Officer Eric Philips (Australia): "The sharp horizon bookending this clip shows the stark contrast between Earth and the void of space. In the middle we see the annual polar night over central Antarctica, caused by the South Pole’s annual tilt away from the sun."

The line that separates day from night on Earth is known as the terminator.

The Fram2 Mission crew members were the first humans to view the Earth’s polar regions from space.

The Fram2 crew successfully returned to Earth on Friday, April 4, 2025 in their SpaceX Dragon spacecraft, splashing down off the coast of California.

The Crew
This was the first human spaceflight for Mission Commander Chun Wang (Malta), Vehicle Commander Jannicke Mikkelsen (Norway), Vehicle Pilot Rabea Rogge (Germany), plus Mission Specialist and Medical Officer Eric Philips (Australia).

The Fram2 Mission was named in honor of Fram "Forward", the first exploration ship to complete voyages to the Arctic and Antarctica between 1893 and 1912. Framonaut Vehicle Commander Jannicke Mikkelsen of Norway carried a small piece of that ship to orbit.

Learn more about the Fram2 Mission and its crew: 

Video Credit: Eric Philips/Fram2 Mission
Duration: 23 seconds
Release Date: April 9, 2025

#NASA #SpaceX #Space #Science #Planet #Earth #Fram2 #PolarRegions #Antarctica #Terminator #PolarOrbit #CrewDragonSpacecraft #SpaceTechnology #Astronauts #EricPhilips #ChunWang #JannickeMikkelsen #RabeaRogge #HumanSpaceflight #CommercialSpace #UnitedStates #Australia #Germany #Deutschland #Norway #Norge #STEM #Education #HD #Video

Cascading Meteors over Kitt Peak National Observatory in Arizona

Cascading Meteors over Kitt Peak National Observatory in Arizona


This image captures the mesmerizing Geminids meteor shower above the National Science Foundation (NSF) McMath Pierce Solar Telescope at the U.S. National Science Foundation Kitt Peak National Observatory (KPNO), a Program of NSF NOIRLab, as the Milky Way rises high into the sky. The annual Geminids shower happens when Earth passes through the debris trail of asteroid 3200 Phaethon in December and this debris collides with our atmosphere to then explode into fiery streaks of light. The Geminids is unusual among meteor showers because it is one of two major showers not caused by a comet. Two telescopes at KPNO are used to study asteroids: the UArizona 0.9-meter and 1.8-meter Spacewatch telescopes. The University of Arizona’s Spacewatch Program was founded to explore populations of small objects in the Solar System and to study the statistics of asteroids and comets to investigate the dynamical evolution of the Solar System.

3200 Phaethon is an active Apollo (near-Earth) asteroid with an orbit that brings it closer to the Sun than any other named asteroid. For this reason, it was named after the Greek Hero, Phaëthon, son of the sun god Helios. It is 5.8 km (3.6 mi) in diameter and is the parent body of the Geminids meteor shower of mid-December.

Phaethon was the first asteroid to be discovered using images from a spacecraft. Simon F. Green and John K. Davies discovered it in images from October 11, 1983, while searching Infrared Astronomical Satellite (IRAS) data for moving objects. It was formally announced on October 14 in IAUC 3878 along with optical confirmation by Charles T. Kowal, who reported it to be asteroidal in appearance. Its provisional designation was 1983 TB, and it later received the numerical designation and name 3200 Phaethon in 1985.

The decommissioned NSF McMath-Pierce Solar Telescope was the largest solar telescope in the world and is now being given new life as a dynamic astronomy visualization and presentation center focused on astronomy funded by NSF. With the public opening scheduled for mid-2025, visitors can expect an experience built on NOIRLab’s foundational principle of Discovering Our Universe Together.

Rob Sparks, the photographer, is a NOIRLab Audiovisual Ambassador.


Credit: KPNO/NOIRLab/NSF/AURA/R. Sparks
Release Date: April 2, 2025

#NASA #Space #Astronomy #Science #SolarSystem #Asteroids #3200Phaethon #Meteors #MeteorShower #Geminids #Gemini #Constellation #Universe #MPST #SolarTelescope #KPNO #KittPeak #Tucson #Arizona #NOIRLab #AURA #NSF #UnitedStates #Astrophotography #RobSparks #Astrophotographer #STEM #Education

Using ‘X-Ray Eyes’ to Find Hidden Black Holes | NASA’s NuSTAR Mission

Using ‘X-Ray Eyes’ to Find Hidden Black Holes NASA’s NuSTAR Mission

Most supermassive black holes in the universe are hiding, but NASA’s NuSTAR mission can find them by using high-energy X-rays. In this video, NuSTAR lead scientist Peter Boorman explains how this space telescope penetrates thick gas and dust to reveal black holes that other telescopes cannot see. Watch to learn as well what finding and studying black holes can reveal about the way galaxies grow and evolve. 

Short for Nuclear Spectroscopic Telescope Array, NuSTAR has been operating since 2012. Recently, scientists combined 10 years of data with measurements from other missions, including the Infrared Astronomical Satellite (IRAS), and they now estimate at least 35 percent of the feeding supermassive black holes in the universe are hidden. Determining the number of hidden versus unobscured black holes can help scientists understand how they get so big.

More About the Mission

NuSTAR launched on June 13, 2012. A Small Explorer mission led by Caltech in Pasadena, California, and managed by JPL for NASA’s Science Mission Directorate in Washington, it was developed in partnership with the Danish Technical University (DTU) and the Italian Space Agency (ASI). The telescope optics were built by Columbia University, NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and DTU. The spacecraft was built by Orbital Sciences Corp. in Dulles, Virginia. NuSTAR’s mission operations center is at the University of California, Berkeley, and the official data archive is at NASA’s High Energy Astrophysics Science Archive Research Center. ASI provides the mission’s ground station and a mirror data archive. Caltech manages JPL for NASA.

For more information on NuSTAR, visit:
www.nustar.caltech.edu


Credit: NASA/JPL-Caltech/Goddard Space Flight Center Conceptual Image Lab; footage from “A Journey to the Center of the Milky Way: Stellar Orbits around its Central Black Hole”: data provided by Andrea Ghez and the UCLA Galactic Center Group, data obtained with the W. M. Keck Telescopes, visualization by NCSA Advanced Visualization Lab, permission granted by NCSA and additional use requires additional NCSA permission;footage from “Zoom into Our Black Hole Seen in a New Light”: ESO/L. Calçada, N. Risinger, DSS, VISTA, VVV Survey/D. Minniti DSS, Nogueras-Lara et al., Schoedel, NACO, GRAVITY Collaboration, EHT Collaboration
Duration: 2 minutes, 32 seconds
Release Date: April 9, 2025

#NASA #Astronomy #Space #Science #NuSTARMission #SpaceTelescope #Stars #Galaxies #BlackHoles #XrayAstronomy #Astrophysics #Cosmos #Universe #JPL #Caltech #GSFC #UnitedStates #STEM #Education #Animation #HD #Video

Planet Mars Images: April 6-9, 2025 | NASA's Curiosity & Perseverance Rovers

Planet Mars Images: April 6-9, 2025 | NASA's Curiosity & Perseverance Rovers

MSL - Sol 4505
MSL - Sol 4503
MSL - Sol 4503
MSL - Sol 4502
MSL - Sol 4502
Mars 2020 - Sol 1467
Mars 2020 - Sol 1469
Mars 2020 - Sol 1466

Celebrating 12+ Years on Mars (2012-2024)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 4+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: April 6-9, 2025

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #MSSS #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Dark Matter Gravitational Lensing | NOIRLab

Dark Matter Gravitational Lensing | NOIRLab

This visualization shows dark matter distorting the light from background galaxies. 

Most of the universe is made of stuff we have never seen. Its gravity drives normal matter (gas and dust) to collect and build up into stars, galaxies, and massive galaxy clusters. Visible matter reveals itself by shining brightly, but astronomers detect dark matter by its gravitational influence on the light we see. By looking at the area around massive galaxy clusters, astronomers can identify warped background galaxies gravitationally lensed by the cluster and reverse-engineer their distortions. 

Learn more about dark matter at NASA:

https://science.nasa.gov/mission/hubble/science/science-highlights/shining-a-light-on-dark-matter/


Credit: NOIRLab/NSF/AURA
Duration: 53 seconds
Release Date: April 8, 2025

#NASA #Astronomy #Space #Science #Galaxies #Astrophysics #DarkMatter #GravitationalLensing  #Cosmos #Universe #NOIRLab #AURA #NSF #UnitedStates #STEM #Education #Visualization #HD #Video

Asteroid 2024 YR4: Moon Impact Risk Assessment | NOIRLab's Gemini South

Asteroid 2024 YR4: Moon Impact Risk Assessment | NOIRLab's Gemini South


This composite image of asteroid 2024 YR4 was captured with the Gemini South telescope in Chile, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab. On February 7, 2025, using the Gemini Multi-Object Spectrograph (GMOS), a team of astronomers took images of the asteroid (the hazy dot at the center of the image) through four filters. Colorful star trails surround the asteroid, showing the passing of time and the motion of the night sky in a still image. The observations allowed the team to determine its composition, orbital characteristics and 3D shape.

2024 YR4 was first detected on December 27, 2024, by the Asteroid Terrestrial-impact Last Alert System (ATLAS). At the time, the asteroid made a close approach to Earth, passing at a distance of just 0.017 astronomical units (approximately 2.5 million kilometers, or 1.5 million miles). Initial uncertainty regarding its trajectory warranted further investigation, leading astronomers to secure critical special Director's Discretionary Time on Gemini South for follow-up observations using the Gemini Multi-Object Spectrograph (GMOS) on February 7, 2025.

In late January 2025, one month after its discovery, 2024 YR4 rose above the International Asteroid Warning Network (IAWN) notification threshold of 1% probability of a future impact with Earth, projected for December 22, 2032. This potential threat gained international attention among the public and the media. With further analysis, the Earth impact probability then dropped below 1% in late February. While the asteroid will miss Earth during this encounter, there remains a few percent chance it could hit the Moon instead.

Interested in characterizing the now famous asteroid, the team of astronomers, led by Bryce Bolin of Eureka Scientific, used the Gemini South telescope in Chile, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation and operated by NSF NOIRLab, to capture images of it in multiple wavelengths.

Learn about the International Asteroid Warning Network (IAWN):
https://iawn.net

Credit: International Gemini Observatory / NOIRLab / NSF / AURA / M. Zamani
Release Date: April 8, 2025

#NASA #Astronomy #Space #Science #SolarSystem #Planet #Earth #Moon #Asteroids #Asteroid2024YR4 #PlanetaryDefense #IAWN #CislunarRiskAssessment #GeminiSouthTelescope #InternationalGeminiObservatory #Chile #NOIRLab #AURA #NSF #UnitedStates #STEM #Education