New submitter louisfreeman shares a report from Space.com: A newly discovered car-sized asteroid just made the closest-known flyby to Earth without hitting our planet. On Sunday (Aug. 16), the asteroid, initially labeled ZTF0DxQ and now formally known to astronomers as 2020 QG, swooped by Earth at a mere 1,830 miles (2,950 kilometers) away. That gives 2020 QG the title of closest asteroid flyby ever recorded that didn't end with the space rock's demise. What's slightly concerning is the fact that the flyby wasn't expected.

The Palomar Observatory didn't detect the zooming asteroid until about six hours after the object's closest approach. "The asteroid approached undetected from the direction of the sun," Paul Chodas, the director of NASA's Center for Near Earth Object Studies, told Business Insider. "We didn't see it coming."

fahrbot-bot shares a report from ScienceAlert: NASA is actively monitoring a strange anomaly in Earth's magnetic field: a giant region of lower magnetic intensity in the skies above the planet, stretching out between South America and southwest Africa. This vast, developing phenomenon, called the South Atlantic Anomaly, has intrigued and concerned scientists for years, and perhaps none more so than NASA researchers. The space agency's satellites and spacecraft are particularly vulnerable to the weakened magnetic field strength within the anomaly, and the resulting exposure to charged particles from the Sun.

The primary source is considered to be a swirling ocean of molten iron inside Earth's outer core, thousands of kilometers below the ground. A huge reservoir of dense rock called the African Large Low Shear Velocity Province, located about 2,900 kilometers (1,800 miles) below the African continent, disturbs the field's generation, resulting in the dramatic weakening effect -- which is aided by the tilt of the planet's magnetic axis. It's not just moving, however. Even more remarkably, the phenomenon seems to be in the process of splitting in two, with researchers this year discovering that the SAA appears to be dividing into two distinct cells, each representing a separate centre of minimum magnetic intensity within the greater anomaly. Just what that means for the future of the SAA remains unknown, but in any case, there's evidence to suggest that the anomaly is not a new appearance.

"The moon is drifting away," reports the New York Times. Every year, it gets about an inch and a half farther from us. Hundreds of millions of years from now, our companion in the sky will be distant enough that there will be no more total solar eclipses.

For decades, scientists have measured the moon's retreat by firing a laser at light-reflecting panels, known as retroreflectors, that were left on the lunar surface, and then timing the light's round trip. But the moon's five retroreflectors are old, and they're now much less efficient at flinging back light. To determine whether a layer of moon dust might be the culprit, researchers devised an audacious plan: They bounced laser light off a much smaller but newer retroreflector mounted aboard a NASA spacecraft that was skimming over the moon's surface at thousands of miles per hour. And it worked...

Dust can be kicked up by meteorites striking the moon's surface. It coated the astronauts' moon suits during their visits, and it is expected to be a significant problem if humans ever colonize the moon. While it has been nearly 50 years since a retroreflector was placed on the moon's surface, a NASA spacecraft launched in 2009 carries a retroreflector roughly the size of a paperback book. That spacecraft, the Lunar Reconnaissance Orbiter, circles the moon once every two hours, and it has beamed home millions of high-resolution images of the lunar surface...

In 2017, Dr. Erwan Mazarico, a planetary scientist at NASA Goddard Space Flight Center and his collaborators began firing an infrared laser from a station near Grasse, France — about a half-hour drive from Cannes — toward the orbiter's retroreflector. At roughly 3 a.m. on Sept. 4, 2018, they recorded their first success: a detection of 25 photons that made the round trip... After accounting for the smaller size of the orbiter's retroreflector, Dr. Mazarico and his colleagues found that it often returned photons more efficiently than the Apollo retroreflectors... "For me, the dusty reflector idea is more supported than refuted by these results" he said.
Laser-reflection measurements over long periods of time and across several reflectors "have revealed that the Moon has a fluid core," NASA notes. "Scientists can tell by monitoring the slightest wobbles as the Moon rotates."

The dwarf planet Ceres -- long believed to be a barren space rock -- is an ocean world with reservoirs of sea water beneath its surface, the results of a major exploration mission showed on Monday. The Guardian reports: Ceres is the largest object in the asteroid belt between Mars and Jupiter and has its own gravity, enabling the Nasa Dawn spacecraft to capture high-resolution images of its surface. Now a team of scientists from the United States and Europe have analyzed images relayed from the orbiter, captured about 35km (22 miles) from the asteroid. They focused on the 20-million-year-old Occator crater and determined that there is an "extensive reservoir" of brine beneath its surface.

Using infrared imaging, one team discovered the presence of the compound hydrohalite -- a material common in sea ice but which until now had never been observed off of Earth. Maria Cristina De Sanctis, from Rome's Istituto Nazionale di Astrofisica said hydrohalite was a clear sign Ceres used to have sea water. "We can now say that Ceres is a sort of ocean world, as are some of Saturn's and Jupiter's moons," she told AFP. The team said the salt deposits looked like they had built up within the last 2 million years -- the blink of an eye in space time. This suggests that the brine may still be ascending from the planet's interior, something De Sanctis said could have profound implications in future studies.

Writing in an accompanying comment article, Julie Castillo-Rogez, from the California Institute of Technology's Jet Propulsion Laboratory, said the discovery of hydrohalite was a "smoking gun" for ongoing water activity. "That material is unstable on Ceres' surface, and hence must have been emplaced very recently," she said. In a separate paper, US-based researchers analyzed images of the Occator crater and found that its mounds and hills may have formed when water ejected by the impact of a meteor froze on the surface.

schwit1 writes: Researchers at NASA's Glenn Research Center have now demonstrated a method of inducing nuclear fusion without building a massive stellarator or tokamak. In fact, all they needed was a bit of metal, some hydrogen, and an electron accelerator.

The team believes that their method, called lattice confinement fusion, could be a potential new power source for deep space missions. They have published their results in two papers in Physical Review C...

"What we did was not cold fusion," says Lawrence Forsley, a senior lead experimental physicist for the project. Cold fusion, the idea that fusion can occur at relatively low energies in room-temperature materials, is viewed with skepticism by the vast majority of physicists. Forsley stresses this is hot fusion, but "We've come up with a new way of driving it."
The article contains a good description of the technical details, and end by summarizing the hopes of the project's analytical physicist and nuclear diagnostics lead. "This method of fusion offers a potentially reliable source for craft operating in places where solar panels may not be useable, for example.

"And of course, what works in space could be used on Earth."

NASA is "reconsidering how we talk about space," reports CNET: NASA gave two examples of cosmic objects it'll no longer use nicknames for. Planetary nebula NGC 2392 has been called the "Eskimo Nebula." "'Eskimo' is widely viewed as a colonial term with a racist history, imposed on the indigenous people of Arctic regions," NASA explained. NASA already added a note to a 2008 image release showing NGC 2392 that explains the decision to retire the nickname.

The agency will also use only the official designations of NGC 4567 and NGC 4568 to refer to a pair of spiral galaxies that were known as the "Siamese Twins Galaxy."

This reexamination of cosmic names is ongoing.
CNN explains NASA's rationale: "Nicknames are often more approachable and public-friendly than official names for cosmic objects, such as Barnard 33, whose nickname 'the Horsehead Nebula' invokes its appearance," NASA said in a release this week. "But often seemingly innocuous nicknames can be harmful and detract from the science...."

The space agency says it "will use only the official, International Astronomical Union designations in cases where nicknames are inappropriate."

Thomas Zurbuchen, associate administrator of NASA's Science Mission Directorate in Washington, DC, said, "Science is for everyone, and every facet of our work needs to reflect that value."

Researchers at NASA's Glenn Research Center have now demonstrated a method of inducing nuclear fusion without building a massive stellarator or tokamak. In fact, all they needed was a bit of metal, some hydrogen, and an electron accelerator. IEEE Spectrum reports: The team believes that their method, called lattice confinement fusion, could be a potential new power source for deep space missions. They have published their results in two papers in Physical Review C. "Lattice confinement" refers to the lattice structure formed by the atoms making up a piece of solid metal. The NASA group used samples of erbium and titanium for their experiments. Under high pressure, a sample was "loaded" with deuterium gas, an isotope of hydrogen with one proton and one neutron. The metal confines the deuterium nuclei, called deuterons, until it's time for fusion.

"During the loading process, the metal lattice starts breaking apart in order to hold the deuterium gas," says Theresa Benyo, an analytical physicist and nuclear diagnostics lead on the project. "The result is more like a powder." At that point, the metal is ready for the next step: overcoming the mutual electrostatic repulsion between the positively-charged deuteron nuclei, the so-called Coulomb barrier. To overcome that barrier requires a sequence of particle collisions. First, an electron accelerator speeds up and slams electrons into a nearby target made of tungsten. The collision between beam and target creates high-energy photons, just like in a conventional X-ray machine. The photons are focused and directed into the deuteron-loaded erbium or titanium sample. When a photon hits a deuteron within the metal, it splits it apart into an energetic proton and neutron. Then the neutron collides with another deuteron, accelerating it. At the end of this process of collisions and interactions, you're left with a deuteron that's moving with enough energy to overcome the Coulomb barrier and fuse with another deuteron in the lattice.

Key to this process is an effect called electron screening, or the shielding effect. Even with very energetic deuterons hurtling around, the Coulomb barrier can still be enough to prevent fusion. But the lattice helps again. "The electrons in the metal lattice form a screen around the stationary deuteron," says Benyo. The electrons' negative charge shields the energetic deuteron from the repulsive effects of the target deuteron's positive charge until the nuclei are very close, maximizing the amount of energy that can be used to fuse. Aside from deuteron-deuteron fusion, the NASA group found evidence of what are known as Oppenheimer-Phillips stripping reactions. Sometimes, rather than fusing with another deuteron, the energetic deuteron would collide with one of lattice's metal atoms, either creating an isotope or converting the atom to a new element. The team found that both fusion and stripping reactions produced useable energy.

PolygamousRanchKid shares a report from CNET: NASA's Doug Hurley and his crewmate Bob Behnken had a satellite phone at their disposal after splashdown on Sunday. At a press conference later that day, Hurley filled us in on what they did with their spare time as they floated around. "Five hours ago we were in a spaceship bobbing around making prank satellite phone calls to whoever we could get ahold of," Hurley said. "Which was kind of fun, by the way." Hurley suggested the satellite phone bill should go to SpaceX founder Elon Musk, who was sitting nearby. Hurley and Behnken didn't elaborate on the content of the prank calls, but here's hoping they tried to order a pizza for delivery to GO Navigator, the SpaceX recovery ship that fished them out of the water.

After travelling all night to return from the International Space Station, two NASA astronauts will splashdown in the Gulf of Mexico at 11:48 PT, reports CNET. "There will be about an hour of excitement prior to that moment as Crew Dragon deorbits and re-enters Earth's atmosphere..."

That 11-minute deorbiting burn should begin in five minutes (at 10:56 PT), and you can watch it live on SpaceX's YouTube channel before the splashdown 52 minutes later. CNET notes that "This will be the first crew recovery at sea of NASA astronauts since 1975 at the end of the Apollo moon exploration era, the space agency tweeted on Sunday." The reentry process is dramatic. "Crew Dragon will be traveling at orbital velocity prior to reentry, moving at approximately 17,500 miles per hour. The maximum temperature it will experience on reentry is approximately 3,500 degrees Fahrenheit," said NASA in a statement on July 24...

If Crew Dragon passes these final tests, then SpaceX will be able to provide regular, operational flights to the ISS starting later this year. And it would end NASA's reliance on Russian spacecraft for the first time since the shuttle era.
After splashdown the crew "will spend up to an hour floating inside the capsule before joint recovery teams from SpaceX and NASA retrieve them for a helicopter trip ashore," reports Reuters.

A post-splashdown news conference is then scheduled about 30 minutes later at 1:30 p.m. PT.

"NASA and SpaceX are going ahead with plans to bring NASA astronauts Doug Hurley and Bob Behnken home from the International Space Station for a splashdown this weekend, even though Hurricane Isaias is heading for Florida's Atlantic coast," reports GeekWire.

"Fortunately, SpaceX's Dragon capsule is heading for waters off Florida's other coast." NASA said weather conditions are all systems go for the targeted site in the Gulf of Mexico, close to Pensacola, as well as for an alternate site off the coast of Panama City, Fla. That opened the way for preparations to proceed for the Dragon Endeavour to undock at 7:34 p.m. ET (4:34 p.m. PT) today, with a splashdown set for 2:41 p.m. ET (11:41 a.m. PT) Sunday.

The plan could be adjusted, before or after the docking, if the weather forecast changes. NASA and SpaceX had made plans for seven potential splashdown targets, but due to Isaias' strength, NASA concentrated on the westernmost sites.
Live coverage has begun online, and will continue for the next 19 hours.

Tomorrow's splashdown "will mark the first return of a commercially built and operated U.S. spacecraft from orbit," reports GeekWire, "and the first at-sea return of U.S. astronauts since the topsy-turvy splashdown of NASA's Apollo-Soyuz crew in 1975..."

"The next SpaceX Crew Dragon launch to the space station is scheduled for as early as next month. And Bob Behnken's wife, NASA astronaut Megan McArthur, is due to be part of a Dragon crew heading for the station next spring."

An anonymous reader quotes Newsweek: A hypothetical spacecraft made from an extremely thin layer of a synthetic foam could technically make it to our closest neighboring star Proxima Centauri in just 185 years, scientists have said. If Voyager were to make the same journey, it would take around 73,000 years, according to NASA.

In a study that is due to be published in the journal Astronomy & Astrophysics, René Heller from the Max Planck Institute for Solar System Research, Germany, and colleagues, propose the spacecraft as a precursor to interstellar travel — beyond our own solar system. They estimate a prototype would cost around $1 million, while the launch of an interplanetary mission would be around $10 million.

The spacecraft would be made from aerographite. This is a carbon-based foam that is around 15,000 times more lightweight than aluminium. It is versatile and light enough that it could be used to create solar sails — "which harness energy from the sun for propulsion, a process called solar photon pressure... In most cases, photons would have little impact on an object. But if the target is an ultralight material, such as aerographite, then the target can actually be pushed to significant speed," he said.

"We found out that a thin layer of aerographite, with a thickness of about 1 millimeter (0.04 inches), can be pushed to speeds that are sufficiently high to let it escape the solar system. Once it has gained an initial push from the solar radiation pressure, it will simply float through space...."

Heller said these spacecraft could travel far faster than any probe ever sent by humans before.

An anonymous reader quotes The Los Angeles Times: On Dec. 9, 1968, the then-small world of computer engineering was shaken to its core by a presentation of new technologies projected onto a screen in a San Francisco hall. The attendees at the historic event saw demonstrations of video conferencing, the first public use of a computer mouse, hyperlinking in which clicking a word in a document transported the user to an entirely new document — and more. The man who was the star of the hands-on show seen in the hall was Douglas Engelbart, whose team at the research center SRI in Menlo Park, California, had been developing them for years.

But the man who had designed what is known now as "The Mother of All Demos" and was working behind the scenes to make sure they all worked was William K. English, who died Sunday at the age of 91. Bill English played an indispensable role in more than Engelbart's demo... In 1965 the lab received a NASA grant to invent a technology for moving a cursor and selecting an item on a display screen; Engelbart developed the concept, but it was English who designed the first prototype &mdash the mouse...

English essentially choreographed Engelbart's presentation. Just as important, he made sure there were no technical glitches. That was a challenge, since Engelbart would be in San Francisco demonstrating a system that was being operated 30 miles away in Menlo Park, the two sites connected via a microwave relay. The event went off virtually without a hitch, and a new world was born. "Doug wasn't doing it," recalls Roberta, who had worked as Engelbart's secretary. "It was all Bill." Engelbart died in 2013.
English also participated in an early research project "into the psychological effects of LSD," according to the article.

But a few years after the legendary demo, English was recruited for Xerox's legendary Palo Alto Research Center, "where he helped midwife PARC's invention of the personal computer and other innovations... He subsequently left Xerox to join Sun Microsystems and later the pioneering electronic game console maker 3DO."

NASA is heading back to the Red Planet. The agency launched a new rover, a car-size robotic explorer named Perseverance, to Mars on an ambitious mission to scour the planet for evidence of ancient life. From a report: The rover, which launched into orbit Thursday at 7:50 a.m. ET, is designed to study the geology and climate of Mars. NASA says the mission and its subsequent discoveries could lay the groundwork for eventual human exploration of the Red Planet. Perseverance is loaded with seven scientific instruments to explore the Martian landscape and assess whether the planet was ever able to sustain life. The six-wheel rover is also carrying a small helicopter, dubbed Ingenuity, to perform experimental test flights in Mars' thin atmosphere, which, if successful, would mark a milestone in powered flight.

"For the first time ever, we're going to fly a helicopter on another planet," NASA Administrator Jim Bridenstine said Monday in a news briefing, adding that future missions to other worlds could use similar helicopters as airborne scouts. The Perseverance rover launched aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida. Typically, crowds gather along beaches near Cape Canaveral to witness NASA launches, but because of the coronavirus pandemic, the agency encouraged space fans to stay home and participate virtually, instead -- particularly as new infections continue to surge in Florida and across the country. Matt Wallace, the mission's deputy project manager at NASA's Jet Propulsion Laboratory in Pasadena, California, said the rover has already lived up to its name, as engineers persevered through the pandemic to ready the spacecraft for its much-anticipated launch. "Nothing prepared us for what we had to deal with in the middle of March as the pandemic struck -- not just our team, but communities across the country and the world," Wallace said. "At that point in the mission, we were in our final assembly activities."

Airbus-France will build the huge satellite that brings the first Martian rock samples back to Earth. The BBC reports: This material will be drilled on the Red Planet by the US space agency's next rover, Perseverance, before being blasted into orbit by a rocket. It'll be the Airbus satellite's job to grab the packaged samples and then ship them home. The joint American-European project is expected to cost billions and take just over a decade to implement. But scientists say it's probably the best way to confirm whether life has ever existed on the Red Planet. Any evidence is likely to be controversial and will need the powerful analytical tools only found in Earth laboratories to convince the doubters, the researchers argue.

The Airbus satellite will be a Goliath among spacecraft. The Earth Return Orbiter (ERO) will weigh 6.5 tonnes at launch in 2026 and use a mix of chemical and electric propulsion to get to Mars, orbit the planet and then return to Earth with its rock consignment. Thales Alenia Space of Italy will be a lead subcontractor working on this aspect of the design. The inclusion of a powerful ion engine will require a lot power, hence the use of immense solar arrays. These panels will give the satellite a "wingspan" of 39m, more than 120ft. But the really remarkable facet of the satellite's mission is the game of catch it will have to play high above Mars. Nasa will put a rocket on the planet later this decade to fire the rocks collected by Perseverance into orbit. The Airbus spacecraft will have to manoeuvre itself into a position to capture these samples that will be packaged inside a football-sized container. After ingesting this container, the satellite must then prepare it for return to Earth. "This is not just twice as difficult as any typical Mars mission; it's twice squared - when you think about the complexity involved," said Dr David Parker, the director of human and robotic exploration at the European Space Agency (Esa). "And this satellite that Airbus will build -- I like to call it 'the first interplanetary cargo ship,' because that's what it will be doing. It's designed to carry cargo between Mars and Earth," he told BBC News.

A tiny piece of Martian basalt the size of a 10p coin will be launched on board a U.S. robot probe on Thursday and propelled towards the red planet on a seven-month journey to its home world. The Guardian reports: This extraordinary odyssey, the interplanetary equivalent of sending coals to Newcastle, will form a key part of Nasa's forthcoming Mars 2020 expedition. Space engineers say the rock -- which has been donated by the Natural History Museum in London -- will be used to calibrate detectors on board the robot rover Perseverance after it lands and begins its search for signs of past life on the planet. "When you turn on instruments and begin to tune them up before using them for research, you calibrate them on materials that are going to be like the unknown substances you are about to study. So what better for studying rocks on Mars than a lump that originated there?" said Professor Caroline Smith, the Natural History Museum's principal curator of meteorites.

Scientists were confident that the rock they were returning to Mars originated on the planet, added Smith, who is also a member of the Mars 2020 science team. "Tiny bubbles of gas trapped inside that meteorite have exactly the same composition as the atmosphere of Mars, so we know our rock came from there." It is thought that the Martian meteorite was created when an asteroid or comet plunged into the planet about 600,000 to 700,000 years ago, spraying debris into space. One of those pieces of rubble swept across the solar system and eventually crashed on to Earth. That meteorite -- now known as SAU 008 -- was discovered in Oman in 1999 and has been in the care of the Natural History Museum since then.

Among the instruments fitted to the Perseverance rover is a high-precision laser called Sherloc, which will be used to decipher the chemical composition of rocks and determine if they might contain organic materials that indicate life once existed -- or still exists -- on Mars. The inclusion of a piece of SAU 008 is intended to ensure this is done with maximum accuracy. Once Perseverance has selected the most promising rocks it can find, it will dump them in caches on the Martian surface. These will then be retrieved by subsequent robot missions and blasted into space towards Earth for analysis.

"NASA's Juno Jupiter probe has captured unprecedented views of the largest moon in the solar system," reports Space.com: During a close flyby of Jupiter on Dec. 26, 2019, Juno mapped the north polar regions of the icy satellite Ganymede in infrared light, something no other spacecraft had done before. The data, which Juno gathered using its Jovian Infrared Auroral Mapper (JIRAM) instrument, show that Ganymede's northern reaches are very different than locales closer to the equator of the moon, which is bigger than the planet Mercury. "The JIRAM data show the ice at and surrounding Ganymede's north pole has been modified by the precipitation of plasma," Alessandro Mura, a Juno co-investigator at the National Institute for Astrophysics in Rome, said in a statement.

"It is a phenomenon that we have been able to learn about for the first time with Juno because we are able to see the north pole in its entirety."

This plasma consists of charged particles from the sun, which have been trapped by Jupiter's powerful magnetic field. Unlike any other moon, the 3,274-mile-wide (5,269 kilometers) Ganymede has a magnetic field of its own, which funnels the plasma toward its poles. A similar phenomenon occurs here on Earth, which explains why the auroras occur at high latitudes on our planet. But Ganymede has no atmosphere to obstruct and be lit up by these particles, so they slam hard into the ice at and around both poles.
The article notes that the $1.1 billion Juno probe "launched in August 2011 and arrived at Jupiter in July 2016."

"A European and NASA spacecraft has snapped the closest pictures ever taken of the sun," reports the Associated Press, "revealing countless little 'campfires" flaring everywhere. Scientists on Thursday released the first images taken by Solar Orbiter, launched from Cape Canaveral in February. The orbiter was about 48 million miles from the sun — about halfway between Earth and the sun — when it took the stunning high-resolution pictures last month... European Space Agency project scientist Daniel Muller described the observed multitude of "campfires" shooting into the corona, or sun's crown-like outer atmosphere, as quite possibly "the tiny cousins of the solar flares that we already know." Millions if not billions of times smaller, these tiny flares may be heating the corona, he said, long known to be hundreds of times hotter than the actual solar surface for unknown reasons... These so-called campfires, Berghmans noted, are "literally everywhere we look." Not yet well understood, they could be mini explosions, or nanoflares. More measurements are planned.

The $1.5 billion spacecraft will tilt its orbit as the mission goes on, providing unprecedented views of the sun's poles. This vantage point will allow it to capture the first pictures of the solar poles.

IEEE Spectrum reports: There's still plenty that can disrupt radio communications... Rather than waiting for a human on Earth to tell the radio how to adapt its systems — during which the commands may have already become outdated — a radio with a neural network can do it on the fly. Such a device is called a cognitive radio. Its neural network autonomously senses the changes in its environment, adjusts its settings accordingly — and then, most important of all, learns from the experience... Worcester Polytechnic Institute and Penn State University, in cooperation with NASA, recently tested the first cognitive radios designed to operate in space and keep missions in contact with Earth. In our tests, even the most basic cognitive radios maintained a clear signal between the International Space Station (ISS) and the ground. We believe that with further research, more advanced, more capable cognitive radios can play an integral part in successful deep-space missions in the future, where there will be no margin for error...

Our own effort to create a proof-of-concept cognitive radio for space communications was possible only because of the state-of-the-art Space Communications and Navigation (SCaN) test bed on the ISS. NASA's Glenn Research Center created the SCaN test bed specifically to study the use of software-defined radios in space. The test bed was launched by the Japan Aerospace Exploration Agency and installed on the main lattice frame of the space station in July 2012... Ours would be the first-ever cognitive radio experiments conducted in space...

During the tests, the cognitive radio clearly showed that it could learn how to maintain a communications link. The radio autonomously selected settings to avoid losing contact, and the link remained stable even as the radio adjusted itself...

Overall, the success of our tests on the SCaN test bed demonstrated that cognitive radios could be used for deep-space missions.

"The U.S. wants to build nuclear power plants that will work on the moon and Mars, and on Friday put out a request for ideas from the private sector on how to do that," reports Time magazine: The U.S. Department of Energy put out the formal request to build what it calls a fission surface power system that could allow humans to live for long periods in harsh space environments.

The Idaho National Laboratory, a nuclear research facility in eastern Idaho, the Energy Department and NASA will evaluate the ideas for developing the reactor. The lab has been leading the way in the U.S. on advanced reactors, some of them micro reactors and others that can operate without water for cooling. Water-cooled nuclear reactors are the vast majority of reactors on Earth. "Small nuclear reactors can provide the power capability necessary for space exploration missions of interest to the Federal government," the Energy Department wrote in the notice published Friday...

The goal is to have a reactor, flight system and lander ready to go by the end of 2026... Officials say operating a nuclear reactor on the moon would be a first step to building a modified version to operate in the different conditions found on Mars.

"Researchers have spotted large waves of martian sand migrating for the first time," reports Science magazine.

"The discovery dispels the long-held belief that these 'megaripples' haven't moved since they formed hundreds of thousands of years ago. They're also evidence of stronger-than-expected winds on the Red Planet." It's pretty staggering that humans can detect these changes on Mars, says Ralph Lorenz, a planetary scientist at the Johns Hopkins University Applied Physics Laboratory who was not involved in the research. "We can now measure processes on the surface of another planet that are just a couple times faster than our hair grows...."

Since the early 2000s, Mars rovers and orbiters have repeatedly spotted megaripples on the Red Planet. But they didn't seem to change in any measurable way, which led some scientists to think they were relics from Mars's past, when its thicker atmosphere permitted stronger winds. Now, using images captured by NASA's Mars Reconnaissance Orbiter, Simone Silvestro, a planetary scientist at Italy's National Institute of Astrophysics in Naples, and his colleagues have shown that some megaripples do creep along — just very slowly. The researchers focused on two sites near the equator of Mars... Megaripples in both regions advanced by about 10 centimeters per year, the team reports in the Journal of Geophysical Research: Planets...

It's a surprise that megaripples move at all on Mars, says Jim Zimbelman, a planetary geologist at the Smithsonian Institution's Air and Space Museum. Just a few decades ago, there was no evidence that sands on Mars were mobile, he says. "None of us thought that the winds were strong enough...." Atmospheric models of Mars suggest winds capable of moving sand are rare. This discovery of migrating megaripples will force those models to be revised, the team suggests....

Megaripples on the move are beacons of windy conditions, which might in turn kick-start dust storms, the researchers suggest. Airborne dust can blanket solar panels, reducing their efficiency, and it can also gum up mechanical parts like gears. That's bad news for Mars rovers and human habitats alike.