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Using the NASA/ESA/CSA James Webb Space Telescope, scientists observed the region above Jupiter’s iconic Great Red Spot to discover a variety of previously unseen features. The region, previously believed to be unremarkable in nature, hosts a variety of intricate structures and activity.

Three weeks after it lifted off from the far side of the moon, China’s Chang’e-6 spacecraft dropped off a capsule containing first-of-its-kind lunar samples for retrieval from the plains of Inner Mongolia.

The gumdrop-shaped sample return capsule floated down to the ground on the end of a parachute, with the descent tracked on live television. After today’s touchdown, at 2:07 p.m. local time (0607 GMT), members of the mission’s recovery team checked the capsule and unfurled a Chinese flag nearby.

Chang’e-6, which was launched in early May, is the first robotic mission to land and lift off again from the moon’s far side — the side that always faces away from Earth. It’s also the first mission to bring dirt and rocks from the far side back to Earth.

“The Chang’e-6 lunar exploration mission achieved complete success,” Zhang Kejian, director of the China National Space Administration, said from mission control. Chinese President Xi Jinping extended congratulations to the mission team, the state-run Xinhua news service reported.

Chang’e-6 followed a flight plan similar to the one used for Chang’e-5, a mission that brought back samples from the moon’s Earth-facing side in 2020. After entering lunar orbit, the spacecraft sent a lander down to the moon’s South Pole-Aitken Basin region.

The lander used an onboard drill and robotic arm to collect and store samples on its ascent stage. It also gathered data about its surroundings with a radon detector, a negative-ion detector and a mini-rover. Data and telemetry were relayed between Chang’e-6 and Earth via China’s Queqiao-2 satellite.

On June 4, Chang’e-6’s ascent stage lifted off for a rendezvous with the orbiting spacecraft. The samples were transferred to a re-entry capsule, and the spacecraft left lunar orbit several days ago for the trip back to Earth. The re-entry capsule was released as the spacecraft sped about 5,000 kilometers (3,100 miles) over the South Atlantic Ocean, CNSA said in a mission update.

After an initial round of processing at the landing site in China’s Inner Mongolia region, the capsule is due to be airlifted to Beijing, where the mission’s precious cargo will be removed for distribution to researchers.

The samples are expected to include volcanic rock and other materials that could shed fresh light on the moon’s origins and compositional differences between the near side and the far side. Scientists may also learn more about resources in the moon’s south polar region. That region is of high interest because it’s thought to harbor deposits of water ice that could be used to support future lunar settlements.

NASA is targeting the south polar region for a series of robotic missions — leading up to a crewed landing during the Artemis 3 mission, which is currently scheduled for 2026. China has its own lunar ambitions, including plans for sending astronauts to the lunar surface by 2030.

The post China’s Chang’e-6 Probe Drops Off Samples From Moon’s Far Side appeared first on Universe Today.

China's Chang'e 6 mission has successfully returned samples from the moon's far side to Earth, notching another spaceflight first for the nation.

When stars reach the end of their life cycle, they shed their outer layers in a supernova. What is left behind is a neutron star, a stellar remnant that is incredibly dense despite being relatively small and cold. When this happens in binary systems, the resulting neutron stars will eventually spiral inward and collide. When they finally merge, the process triggers the release of gravitational waves and can lead to the formation of a black hole. But what happens as the neutron stars begin merging, right down to the quantum level, is something scientists are eager to learn more about.

When the stars begin to merge, very high temperatures are generated, creating “hot neutrinos” that remain out of equilibrium with the cold cores of the merging stars. Ordinarily, these tiny, massless particles only interact with normal matter via weak nuclear forces and possibly gravity. However, according to new simulations led by Penn State University (PSU) physicists, these neutrinos can weakly interact with normal matter during this time. These findings could lead to new insights into these powerful events.

Pedro Luis Espino, a postdoctoral researcher at Penn State and the University of California, Berkeley, led the research. He was joined by fellow astrophysicists from PSU, the Theoretical Physics Institute at the Friedrich Schiller University Jena, the University of Trent, and the Trento Institute for Fundamental Physics and Applications (INFN-TIFPA). A paper describing their simulations, “Neutrino Trapping and Out-of-Equilibrium Effects in Binary Neutron-Star Merger Remnants,” recently appeared in the journal Physical Reviews Letters.

Artist’s conception of a neutron star merger. This process also creates heavy elements. Credit: Tohoku University

Originally predicted by Einstein’s Theory of General Relativity, gravitational waves (GW) are essentially ripples in spacetime caused by the collapse of stars or the merger of compact objects (such as neutron stars and black holes). Neutron stars are so named because their incredible density fuses protons and electrons together, creating stellar remnants composed almost entirely of neutrons. For years, astronomers have studied GW events to learn more about binary companions and what happens at the moment they merge. Said Pedro Luis Espino, a postdoctoral researcher at Penn State and the University of California, Berkeley, explained in a Penn State press release:

“For the first time in 2017, we observed here on Earth signals of various kinds, including gravitational waves, from a binary neutron star merger. This led to a huge surge of interest in binary neutron star astrophysics. There is no way to reproduce these events in a lab to study them experimentally, so the best window we have into understanding what happens during a binary neutron star merger is through simulations based on math that arises from Einstein’s theory of general relativity.”

While neutron stars are effectively cold, they can become extremely hot during a merger, especially at the interface (the point where the two stars are making contact). In this region, temperatures can reach the trillions of degrees Kelvin, but the stars’ density prevents photons from escaping to dissipate the heat. According to David Radice, an assistant professor of astronomy and astrophysics at the Eberly College of Science at Penn State and one of the team leaders, this heat may be dissipated by neutrinos, which are created during the collision as neutrons are smashed to form protons, electrons, and neutrinos.

“The period where the merging stars are out of equilibrium is only 2 to 3 milliseconds, but like temperature, time is relative here, the orbital period of the two stars before the merge can be as little as one millisecond,” he said. “This brief out-of-equilibrium phase is when the most interesting physics occurs, once the system returns to equilibrium, the physics is better understood.”

To investigate this, the research team created supercomputer simulations that modeled the merger and associated physics of binary neutron stars. Their simulations showed that even neutrinos can be trapped by the heat and density of the merger, that the hot neutrinos are out of equilibrium with the still cool cores, and can interact with the matter of the stars. Moreover, their simulations indicate that the physical conditions present during a merger can affect the resulting GW signals. Said Espino:

“How the neutrinos interact with the matter of the stars and eventually are emitted can impact the oscillations of the merged remnants of the two stars, which in turn can impact what the electromagnetic and gravitation wave signals of the merger look like when they reach us here on Earth. Next-generation gravitation-wave detectors could be designed to look for these kinds of signal differences. In this way, these simulations play a crucial role allowing us to get insight into these extreme events while informing future experiments and observations in a kind of feedback loop.”

This is certainly good news for gravitational wave astronomy and for scientists hoping to use GW events to probe the interiors of neutron stars. Knowing what conditions are present during mergers based on the type of GW signals produced could also provide new insight into supernovae, Gamma-ray Bursts, Fast Radio Bursts, and the nature of Dark Matter.

Further Reading: PSU, Physical Review Letters

The post Simulating the Last Moments Before Neutron Stars Merge appeared first on Universe Today.

NOAA's GOES-U weather satellite has been cleared for its planned liftoff today (June 25) atop a SpaceX Falcon Heavy rocket.

Sleeping cuckoo bees, colourful cotton harlequin bugs and a thorny lacewing trapped in amber appear in some of the best entries to the Royal Entomological Society Photography Competition

Sleeping cuckoo bees, colourful cotton harlequin bugs and a thorny lacewing trapped in amber appear in some of the best entries to the Royal Entomological Society Photography Competition

China's Chang'e 6 probe is scheduled to return to Earth on June 25, and scientists are starting to get excited about what its far side moon samples can tell us.

More than 50 million people living near airports in Europe may be at risk of health impacts from a little-studied form of air pollution produced at high levels by aircraft engines

More than 50 million people living near airports in Europe may be at risk of health impacts from a little-studied form of air pollution produced at high levels by aircraft engines

Using the ALMA radio telescope array, astronomers have investigated the disks of gas and dust around young binary stars to better understand how these systems procure planets.

Eva Granger firmly believes that anyone can launch a career at NASA. As the events and milestones lead for the Orion Program’s strategic communications team, she dedicates her time to engaging with the public and educating them not only about the Orion spacecraft but also about the various opportunities to contribute to the agency’s mission.

“I have met so many people who don’t think aerospace is possible for them, but it’s easy to clear up that assumption. There are artists, nurses, psychologists, administrative assistants, and more working at NASA,” she said. “There are opportunities for everyone to build a life and career here, and telling someone that, and seeing something spark, is always rewarding.”

Eva Granger, events and milestones lead for the Orion Program’s strategic communications team. Image courtesy of Eva Granger

When Granger started working as a full-time contractor in October 2023 at Johnson Space Center in Houston, she was already familiar with her role. An internship in 2022 gave her experience with the program’s event planning and coordination, as well as an exciting opportunity to support and staff the Artemis I launch at NASA’s Kennedy Space Center in Florida.

“During those few days, I met individuals who flew from all over the world to watch the launch. The commitment and excitement that I felt from the global audience was tangible, and impressed on me the importance and impact of the work we do,” she said. “It’s one thing to know the world is watching, but it’s a whole different experience to meet them and be told they’re rooting for your program.”

Eva Granger (far left) stands with fellow Orion Program interns and Orion Program Manager Howard Hu in front of the Artemis III crew module in the Neil Armstrong Operations & Checkout Building at NASA’s Kennedy Space Center in Florida. Image courtesy of Eva Granger

Granger is an active member of Johnson’s Out & Allied Employee Resource Group (ERG) and is currently working to organize the group’s participation in the Houston Pride Parade. “We want to have fun with the parade, but it also gives us an avenue to put together an event that is visible and that anyone at Johnson can attend and be excited about together,” she said.

She believes that continually being present and engaged is the best way to support and champion an equitable and inclusive environment. “The ERG has been amazing in giving us a structured opportunity to make a difference,” she said. “If we show up at the JSC Chili Cookoff or at intern events, people know that we’re here. It shows our closeted friends that there is a support network here at Johnson, and it allows the greater Johnson community to learn about our group and engage with us.”

Eva Granger (front row, left) with Out & Allied ERG volunteers at the Montrose Center’s Hatch Prom for LGBTQI+ youth. Image courtesy of Eva Granger

The ERG also provides valuable professional development resources and networking opportunities. “As a young professional, it is crucial to have mentors, and Out & Allied is full of people who are excited to spend their time building up our members and our community,” Granger said.

She encourages colleagues to connect with others outside their usual social and professional circles as a way to support diversity and inclusion. “There are hundreds of people on campus and all of them have something interesting to share if you stop and say hi,” she said. “Little interactions go a long way.”

First looks would tell most observers that supermassive black holes (SMBHs) and very young stars have nothing in common. But that’s not true. Astronomers have detected a supermassive black hole (SMBH) whose growth is regulated the same way a baby star’s is: by magnetic winds.

Supermassive Black Holes are so massive that comprehending them is difficult. They can be billions of times more massive than our Sun, a number so easy to say that it trivializes their true magnitude. They grow so large through two mechanisms: mergers and accretion.

Black holes can’t be seen directly, but their existence is confirmed by observing how they alter their surroundings. SMBHs are so massive that they alter the orbits and velocities of nearby stars, a phenomenon astronomers have clearly observed. SMBHs are also visible as active galactic nuclei when they’re actively accreting material. Lastly, when black holes merge, they release gravitational waves that we can detect with facilities like LIGO/Virgo.

But there are lots of unanswered questions about how black holes grow by accretion. To try to understand how an SMBH accretes gas and acquires mass, a team of researchers observed ESO320-G030, a nearby galaxy only 120 million light years away.

Their results are in a paper titled “A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030.” The paper is published in the journal Astronomy and Astrophysics, and the lead author is Mark Gorski, a postdoc at Northwestern University.

One outstanding issue in the study of SMBHs concerns black hole feedback. Not all of the material that enters an SMBH’s accretion disk falls into the hole. Some is released by astrophysical jets. This is part of a process called black hole feedback, and it shapes how the black hole grows and how quickly its galaxy forms new stars.

ESO 320-G030 is interesting not only because it hosts an SMBH but also because it’s forming new stars at a rapid rate, about ten times as fast as the Milky Way. To try to understand all the processes in the galaxy’s nucleus, a team of researchers used the Atacama Large Millimetre/submillimetre Array (ALMA) to observe molecules being transported from the galaxy’s center outward.

“How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution,” the authors write in their research article. “One potential way to regulate nuclear growth is through a galactic wind that removes gas from the nucleus.”

ALMA’s strength lies in its ability to see through thick gas and dust and to observe light that straddles infrared light and radio waves. It can track cold molecules by the light they emit in these wavelengths. In this research, ALMA tracked HCN (hydrogen cyanide) as it travelled through ESO 320-G030’s nucleus.

“It is unclear whether galactic winds are powered by jets, mechanical winds, radiation, or via magnetohydrodynamic (MHD) processes,” the authors write. By using ALMA to observe HCN, the researchers hoped to bring clarity.

An artist’s conception of a supermassive black hole’s jets. Credit: NASA / Dana Berry / SkyWorks Digital

ESO 320-G030 is a particular type of galaxy. It’s a luminous infrared galaxy with a very compact nucleus obscured by dust. About 30% of these types of galaxies have extremely compact nuclei with growing SMBHs or unusual starbursts. There’s clearly a lot of action in the galaxy’s nucleus, so it’s a critical target for astrophysicists and astronomers.

“Since this galaxy is very luminous in the infrared, telescopes can resolve striking details in its centre,” said Susanne Aalto, Professor of Radio Astronomy at Chalmers University of Technology. “We wanted to measure light from molecules carried by winds from the galaxy’s core, hoping to trace how the winds are launched by a growing, or soon to be growing, supermassive black hole. By using ALMA, we were able to study light from behind thick layers of dust and gas.”

There’s a debate among astronomers over the nature of black hole feedback. Galaxies have AGN-driven outflows that inject gas back into a galaxy’s nucleus, but they can’t agree on the nature of the feedback. It could be jets, mechanical winds, or radiation. Observing ESO 320-G030 with ALMA’s molecule-observing ability is a chance to wade deeply into the debate.

ALMA was able to trace the behaviour of HCN due to excitational vibration. The observations result in maps of the molecule’s movement in the galaxy’s nucleus.

This figure from the research shows an intensity-weighted velocity field of HCN in ESO 320-G030’s nucleus. The authors write, “The rough location and direction of the outflow is indicated by the dashed arrows.” The contours in the figure show that the HCN-vib emission is “extended along the outflow and that the outflow is launched from similarly rotating sides of the nucleus.” Image Credit: Gorski et al. 2024

“We can see how the winds form a spiralling structure, billowing out from the galaxy’s centre. When we measured the rotation, mass, and velocity of the material flowing outwards, we were surprised to find that we could rule out many explanations for the power of the wind, star formation for example. Instead, the flow outwards may be powered by the inflow of gas and seems to be held together by magnetic fields,” said Aalto.

As the SMBH draws material into its rotating accretion disk, the rotation creates powerful magnetic fields. The magnetic fields lift matter away from the center, creating a spiralling MHD (magnetohydrodynamic) wind. As matter is removed by the wind, the disk rotation slows. Slower rotation allows more material to fall into the hole, letting the SMBH grow more massive.

Other winds and jets in the nucleus propel material away from black holes in galaxy nuclei, but this newly discovered wind feeds material into the black hole. “In this Letter, we present compelling evidence that the outflow in ESO 320-G030 is powered by a different mechanism, an MHD wind launched prior to the ignition of an AGN,” the authors write. Since an AGN is observed when an SMBH has accreted material into its disk and the material has been heated by rotation, the wind the researchers observed is likely responsible for feeding material into the black hole’s disk, some of which falls into the hole itself.

To the astronomers behind the work, the ALMA data images are a breathtaking new insight into the winds in ESO 320-G030’s galactic nucleus. “What is spectacular about the outflow morphology is that the launching regions are apparent and connected to the rotating nuclear structure in the innermost ~12 pc,” they write. The patterns revealed by ALMA hint at the presence of a magnetized rotating wind.

The wind’s rotating element is key. “The rotation of outflows is a strong indication of magnetic acceleration,” the authors explain. If magnetic acceleration is driving it, then the other phenomena astronomers debate—AGN, astrophysical jets, or radiation—can’t be responsible.

This newly discovered wind is similar to the winds around young protostars that are accreting material and actively growing.

Artist’s conception of a star being born within a protective shroud of gas and dust. New research shows that magnetic winds aid the growth of both protostars and SMBHs. Credit: NASA

“It is well-established that stars, in the first stages of their evolution, grow with the help of rotating winds – accelerated by magnetic fields, just like the wind in this galaxy. Our observations show that supermassive black holes and tiny stars can grow by similar processes, but on very different scales.” said lead author Gorski in a press release.

This could be a big step in understanding how SMBHs grow, but the authors know it’s only one step. They need to observe more SMBHs and gather more data before anything is conclusive.

“Far from all questions about this process are answered. In our observations we see clear evidence of a rotating wind that helps regulate the growth of the galaxy’s central black hole. Now that we know what to look for, the next step is to find out how common a phenomenon this is. And if this is a stage which all galaxies with supermassive black holes go through, what happens to them next?” asks lead author Gorski.

The post Growing Black Holes Have Much in Common With Baby Stars appeared first on Universe Today.

A Nigerian could soon make it to space for the first time ever, via Jeff Bezos' aerospace company Blue Origin.

It’s almost time for our summer hiatus. A time to catch up on all that reading. We’ll give you some book recommendations, and what we’re hoping to read during the summer.

The post #724: Summer Science & SciFi Reads appeared first on Astronomy Cast.

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Marcia Rieke, a scientist who worked on NASA’s James Webb Space Telescope and Hubble Space Telescope, has received the Gruber Foundation’s 2024 Cosmology Prize. Rieke will receive the award and gold laureate pin at a ceremony August 8, 2024, at the General Assembly of the International Astronomical Union in Cape Town, South Africa.

Marcia Rieke is Regents’ Professor of Astronomy at the University of Arizona and was the principal investigator for the Near-Infrared Camera (NIRCam) on the Webb telescope.University of Arizona

Rieke was awarded the prize “for her pioneering work on astronomical instrumentation to reveal the breadth and details of the infrared universe. Her contributions to flagship space missions have opened new avenues for understanding the history and mechanisms of star and galaxy formation. She enabled the development and delivery of premier instruments providing groundbreaking sensitivity to near-infrared wavelengths to both the Webb and the Hubble telescopes. Through these substantive contributions along with earlier work, Marcia Rieke has had a lasting impact on our understanding of the universe,” according to the Gruber Foundation’s announcement.

The Cosmology Prize honors a leading cosmologist, astronomer, astrophysicist, or scientific philosopher for theoretical, analytical, conceptual, or observational discoveries leading to fundamental advances in our understanding of the universe. Since 2001, the Cosmology Prize has been cosponsored by the International Astronomical Union. Presented annually, the Cosmology Prize acknowledges and encourages further exploration in a field that shapes the way we perceive and comprehend our universe.

Rieke is Regents’ Professor of Astronomy at the University of Arizona and was the principal investigator for the Near-Infrared Camera (NIRCam) on the Webb telescope.

As principal investigator for the NIRCam, Rieke was responsible for ensuring that the instrument was built and delivered on time and on budget. She worked with the engineers at Lockheed Martin who built NIRCam and helped them decipher and meet the instruments’ requirements.

“As principal investigator of the James Webb Space Telescope NIRCam instrument, Dr. Rieke’s vision, dedication, and leadership were inspirational to the entire team and a key contribution to the success of the Webb telescope,” said Lee Feinberg, Webb telescope manager and optics lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. 

Rieke’s research interests include infrared observations of the center of the Milky Way and of other galactic nuclei. She has served as the deputy principal investigator on the Near Infrared Camera and Multi-Object Spectrometer for the Hubble Space Telescope (NICMOS), and the outreach coordinator for NASA’s retired Spitzer Space Telescope.

“As a leading scientist on a premiere Hubble Space Telescope science camera, NICMOS, Dr. Rieke’s expertise enabled ground-breaking discoveries on everything from star formation to distant galaxies,” said Dr. Jennifer Wiseman, Hubble Space Telescope senior project scientist at NASA Goddard. “Subsequent cameras on Hubble, and infrared space telescopes like Spitzer and Webb, have built upon Dr. Rieke’s pioneering work.”

“Dr. Rieke has also poured herself into wide international scientific leadership, leading countless scientific panels that envision and shape the best instruments for future powerful astronomical discovery,” Wiseman said.

“There’s a story beginning to emerge,” Rieke said about the science Webb has returned in the first two years of its mission. “But we still need some more pieces to the story.” For the duration of Webb’s lifetime, many of those pieces will emerge from the instrument that Rieke led.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

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Rob Gutro
NASA’s Goddard Space Flight Center

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After helium leaks and thruster problems with Boeing’s Starliner capsule, NASA has been pushing back the return date from the International Space Station. On Friday, the agency announced they no longer had a planned return date. Instead, they will keep testing the capsule, trying to understand its issues, and seeing if they can make any fixes. Plenty of supplies are on the station, so there’s no urgent need to bring the two astronauts back to Earth.

NASA decided to cancel the planned departure of Wednesday, June 26 because of conflicting timelines with a series of planned spacewalks on the ISS, set for today (Monday, June 24), and Tuesday, July 2. The delay also allows mission teams time to review propulsion and system data.

Boeing’s CTS-100 Starliner taking off from Cape Canaveral, Florida, on June 5th, 2024. Credit: NASA

After years of delays and two recent scrubbed launch attempts, Starliner finally launched on June 5, 2024 with NASA astronauts Butch Wilmore and Suni Williams on board. Although two of the spacecraft’s thrusters failed during the flight, the spacecraft managed to reach the ISS and delivered 227 kg (500 lbs) of cargo. Additionally, five small leaks on the service module were also detected, and the crew and ground teams have been working through safety checks.

“We are taking our time and following our standard mission management team process,” said Steve Stich, manager of NASA’s Commercial Crew Program in a NASA blog post. “We are letting the data drive our decision making relative to managing the small helium system leaks and thruster performance we observed during rendezvous and docking. Additionally, given the duration of the mission, it is appropriate for us to complete an agency-level review, similar to what was done ahead of the NASA’s SpaceX Demo-2 return after two months on orbit, to document the agency’s formal acceptance on proceeding as planned.”

This first crewed flight of Starliner was supposed to validate the spacecraft as part of NASA’s Commercial Crew Program (CCP), with the hope of it working alongside SpaceX’s Crew Dragon to make regular deliveries of cargo and crew to the ISS. This mission is the second time the Starliner has flown to the ISS and the third flight test overall. During the first uncrewed test flight (OFT-1), which took place back in December 2019, the Starliner launched successfully but failed to make it to the ISS. After making 61 corrective actions recommended by NASA, another attempt was made (OFT-2) on May 22nd, 2022. That flight successfully docked to the ISS, staying there for four days before undocking and landing in the White Sands Missile Range in New Mexico.

The seven Expedition 71 crew members gather with the two Crew Flight Test members for a team portrait aboard the space station. In the front from left are, Suni Williams, Oleg Kononenko, and Butch Wilmore. Second row from left are, Alexander Grebenkin, Tracy C. Dyson, and Mike Barratt. In the back are, Nikolai Chub, Jeanette Epps, and Matthew Dominick. Photo credit: NASA

Wilmore and Williams are now  working with the Expedition 71 crew, assisting with station operations as needed and completing add-on in-flight objectives for NASA’s certification of Starliner.

Stich said that despite all the issues, Starliner is performing well in orbit while docked to the space station.

“We are strategically using the extra time to clear a path for some critical station activities while completing readiness for Butch and Suni’s return on Starliner,” he said, “and gaining valuable insight into the system upgrades we will want to make for post-certification missions.”

Mission managers will evaluate future return opportunities for Starliner and NASA said they will host a media telecon with mission leadership following a readiness review. NASA added that Starliner is actually cleared for return in case of an emergency on the space station that would require the crew to leave orbit and come back to Earth.

The post NASA Doesn't Know When Starliner Will Return From Orbit appeared first on Universe Today.

Astronomers have measured supermassive black hole winds that existed when the universe was less than a billion years old, showing how these cosmic titans shape galaxies.

A Florida family has filed a claim with NASA after discarded components from the International Space Station crashed through their house.

Crews transport NOAA’s (National Oceanic and Atmospheric Administration) Geostationary Operational Environmental Satellite (GOES-U) from the Astrotech Space Operations facility to the SpaceX hangar at Launch Complex 39A at NASA’s Kennedy Space Center in Florida beginning on Friday, June 14, 2024, with the operation finishing early Saturday, June 15, 2024. The fourth and final weather-observing and environmental monitoring satellite in NOAA’s GOES-R Series will assist meteorologists in providing advanced weather forecasting and warning capabilities. The two-hour window for liftoff opens 5:16 p.m. EDT Tuesday, June 25, aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.