Planet Mars Images: April 9-11, 2025 | NASA's Curiosity & Perseverance Rovers
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Friday, April 11, 2025
Planet Mars Images: April 9-11, 2025 | NASA's Curiosity & Perseverance Rovers
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.
Duration: 1 minute
Release Date: April 11, 2025
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.
Duration: 1 minute, 26 seconds
Release Date: April 11, 2025
NASA's Space to Ground: Changing Space | Week of April 11, 2025
NASA's Space to Ground: Changing Space | Week of April 11, 2025
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.
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy
NASA Flight Engineers: Don Pettit, Anne McClain, Nichole Ayers, Jonny Kim
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.
Duration: 4 minutes, 27 seconds
Release Date: April 11, 2025
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/
https://science.nasa.gov/mission/mars-2020-perseverance
Duration: 1 minute, 28 seconds
Release Date: April 10, 2025
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
https://www.nasa.gov/suscribete
Release Date: April 10, 2025
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.
Roscosmos (Russia) Flight Engineers: Ivan Vagner, Kirill Peskov, Sergey Ryzhikov, Alexey Zubritskiy
NASA Flight Engineers: Don Pettit, Anne McClain, Nichole Ayers, Jonny Kim
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.
Capture Date: April 8, 2025
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.
https://science.nasa.gov/mission/voyager/voyager-2/
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
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.
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.
“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.
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.”
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.
https://science.nasa.gov/mission/mars-2020-perseverance
Release Date: April 10, 2025
International Day of Women and Girls in Science 2025 | United Nations
International Day of Women and Girls in Science 2025 | United Nations
Image Date: Feb. 11, 2025
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.
Duration: 55 seconds
Release Date: April 10, 2025
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.
Duration: 23 seconds
Release Date: April 9, 2025
Cascading Meteors over Kitt Peak National Observatory in Arizona
Cascading Meteors over Kitt Peak National Observatory in Arizona
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.
Release Date: April 2, 2025
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.
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.
www.nustar.caltech.edu
Duration: 2 minutes, 32 seconds
Release Date: April 9, 2025
Planet Mars Images: April 6-9, 2025 | NASA's Curiosity & Perseverance Rovers
Planet Mars Images: April 6-9, 2025 | NASA's Curiosity & Perseverance Rovers
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/
Release Date: April 8, 2025








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