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Science Dispatches

93 Stories Available
50 years after Viking 1's historic Mars landing, NASA is looking to the Red Planet's skies
Science
Space.com·9h ago

50 years after Viking 1's historic Mars landing, NASA is looking to the Red Planet's skies

Astronomers have discovered an unusually massive, dense exoplanet that challenges conventional ideas about how rocky planets form.Called GJ 523b, the exoplanet is about 2.5 times wider than Earth but packs roughly 23 times our planet's mass into that relatively compact size. Worlds this large and dense are sometimes referred to as "mega-Earths," an informal term for unusually massive, predominantly rocky planets. GJ 523b's high density suggests it contains relatively little atmosphere despite being large enough that astronomers would normally expect it to have accumulated a substantial gaseous envelope, according to a statement from the University of Wisconsin–Madison."This isn't what we expected at all," Max Kroft, lead author of the study, said in the statement. "Dense planets like this aren't uncommon, but they're usually small rocky planets similar to Earth or Mercury. This planet is two and a half times bigger than the Earth."GJ 523b was initially identified as a candidate by NASA's Transiting Exoplanet Survey Satellite (TESS), which searches for periodic dips in starlight caused when planets cross, or transit, their host stars. Researchers followed up with observations from the ground-based WIYN 3.5-meter Telescope at Kitt Peak National Observatory in Arizona, using a spectrograph to measure the planet's gravitational tug on its star.Combining those observations, the team calculated that GJ 523b has a mass about 23.5 times that of Earth, a radius 2.55 times larger and a density of about 126.82 grams per cubic inch. It circles its star every 17.75 days. The planetary system is also relatively young, at an estimated nearly 170 million years old, according to the study.That combination of size, mass and youth poses a puzzle for planet formation models. Planets begin by building cores of rock and metal, which can then pull in hydrogen and helium from the disk of gas and dust surrounding a young star. In our own solar system, giant planets such as Jupiter and Saturn are thought to have begun rapidly accumulating their massive gaseous envelopes once their growing cores reached roughly 20 times Earth's mass.GJ 523b is already about 23 times Earth's mass, putting it beyond that threshold. Yet instead of developing into a gas-rich world, its unusually high density suggests it has relatively little gas and remains predominantly rocky — raising the question of why it followed such a different path."The question is, why didn't this planet do that, if it's 20 times the size of Earth?" Kroft said in the statement.One possibility is that GJ 523b initially formed with a thick atmosphere that was later stripped away. Another is that it formed through a collision between two planets, creating a larger rocky world while blasting much of their gaseous envelopes into space, according to the statement.Astronomers have used the term "mega-Earth" for more than a decade to describe exceptionally massive rocky worlds, though it has never represented a formally established class of exoplanets. Finding more examples like GJ 523b could help reveal whether these unusual worlds are rare exceptions or part of a broader population."It's hard to infer things about planet formation in general from a sample size of one," Kroft said in the statement. "We're not going to get to 10,000 of these overdense planets, but if we can get to 20 or 30, maybe some trends might pop out."The findings have been submitted to The Astronomical Journal and are currently available on the preprint server arXiv and have not yet been peer reviewed.

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A stray SpaceX rocket stage could slam into the moon this August, amateur astronomer says
Science
Space.com·17h ago

A stray SpaceX rocket stage could slam into the moon this August, amateur astronomer says

The first stage of LandSpace's Zhuque-3 rocket rests on its landing pad shortly after its historic touchdown on Aug. 18, 2026. (Image credit: LandSpace) China just notched another big spaceflight milestone.The Beijing startup LandSpace successfully landed the first stage of its Zhuque-3 rocket this evening (Aug. 18), becoming the first Chinese company ever to do so during an orbital launch.It was just the second Chinese orbital rocket touchdown overall. The first was pulled of on July 10 by a Long March 10B, which is built by the state-owned China Aerospace Science and Technology Corporation (CASC).The Long March 10B had some help returning to Earth, settling softly into a net-like device affixed to a ship at sea. But Zhuque-3 came down on terra firma and stayed upright thanks to a set of landing legs, like those sported by SpaceX's workhorse Falcon 9 rocket."This mission marks China's first-ever successful recovery attempt of the first stage of an orbital-class launch vehicle using landing legs, and China's first successful booster recovery on land," LandSpace said via X this evening."It is a pivotal flight test for Zhuque-3 as it transitions from the technological demonstration and verification phase toward the engineering application phase of reusability," the company added. "This mission further verified the design correctness and reliability of the Zhuque-3 reusable launch vehicle system, validated its first-stage recovery capability and engineering maturity."Zhuque-3 broadly resembles the Falcon 9, which made its first landing way back in 2015 and now has more than 600 of them under its belt. Both feature a reusable booster and an expendable upper stage, and they're about the same height — 230 feet (70 meters) for the Falcon 9 and 216 feet (66 m) for Zhuque-3.Their lifting power is similar as well. Zhuque-3 can haul about 40,350 pounds (18,300 kilograms) to low Earth orbit, while the Falcon 9's LEO payload capacity is 50,265 pounds (22,800 kg).The two rockets use two very different fuels, however — a combination of liquid oxygen (LOX) and rocket-grade kerosene for the Falcon 9, compared to LOX and liquid methane for Zhuque-3. This "methalox" mixture is also used by Starship, the fully reusable megarocket that SpaceX is developing to help humanity settle the moon and Mars, among other spaceflight tasks. LandSpace's Zhuque-3 rocket launches on its second-ever mission on Aug. 18, 2026. The flight was a success, and Zhuque-3's first stage returned to Earth for a landing — the first ever for a private Chinese orbital rocket. (Image credit: LandSpace)Today's launch — which occurred from the Dongfeng Commercial Space Innovation Pilot Zone in northwest China at 7:35 p.m. EDT (2335 GMT; 7:35 a.m. on Aug. 19 Beijing time) — was the second overall for the Zhuque-3. The rocket first flew on Dec. 2, 2025, on a mostly successful debut; Zhuque-3's upper stage reached orbit as planned, which is rare for a first flight.LandSpace tried to bring the booster back for a touchdown that day as well, but the attempt failed. Zhuque-3 suffered "an abnormal combustion" as it neared the ground, according to the state-run outlet Xinhua (translation by Google), and ended up exploding near the designated landing pad.Today's mission, however, was an unqualified success for the Zhuque-3: The rocket's upper stage delivered a satellite called Honghu 03, which was developed by Hongqing Technology, to its designated orbit, LandSpace wrote in another X post today.MISSION SUCCESS | ZhuQue-3 Y2 Reusable Launch Vehicle Achieved Full Success in Orbital Insertion and First-Stage RecoveryOn August 19, 2026, at 07:35 (UTC+8), the ZhuQue-3 (ZQ-3) Y2 reusable launch vehicle lifted off from the Dongfeng Commercial Space Innovation Pilot Zone.… pic.twitter.com/fshijOxgtcAugust 19, 2026Zhuque-3 is part of a concerted Chinese push toward rocket reusability, an efficiency-boosting feature that has helped make the Falcon 9 the world's leading launcher by far. (The SpaceX

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Astronomers capture highest-resolution image ever of the Sun’s surface
Science
Space.com·Yesterday

Astronomers capture highest-resolution image ever of the Sun’s surface

A view of the moon's shadow darkening Earth's surface during the Aug. 12 total solar eclipse, as seen by ESA's MTG-I1 satellite. (Image credit: ©ESA/Eumetsat) The Aug. 12 total solar eclipse didn't only plunge millions of people across Greenland, Iceland and Spain into a false twilight — a fleet of spacecraft orbiting our planet managed to capture the magic, too.August's total solar eclipse occurred as the moon passed directly between the sun and Earth during its monthly new moon phase. Those lucky enough to be in the path of totality watched on in awe as the moon progressively swallowed the light of the sun, ultimately revealing our star's tenuous atmosphere against a prematurely darkened evening sky.It was a show of truly epic proportions — and maybe one whose scale can be particularly appreciated when viewed through the mechanical eyes of NASA and European Space Agency (ESA) spacecraft that observe our planet and sun from afar. Read on to see some breathtaking views of the Aug. 12 total solar eclipse from orbit.The Aug. 12 total solar eclipse, seen from spaceOur first view comes courtesy of NASA astronaut Jessica Meir, who captured the moon taking a bite out of the sun from the Russian segment of the International Space Station (ISS) on Aug. 12. The partially eclipsed sun as photographed by NASA astronaut Jessica Meir from the Russian segment of the International Space Station on Aug. 12. (Image credit: NASA/Jessica Meir via X)"Given the location of the @Space_Station at the time of the total solar eclipse today, we saw only a partial eclipse, with a peak of around 18% sun coverage," Meir said in an X post accompanying the photographs.Given the location of the @Space_Station at the time of the total solar eclipse today, we saw only a partial eclipse, with a peak of around 18% sun coverage. Here’s how it looked from a window in the Russian segment about 45 minutes ago. Photo of the sun taken with a Nikon Z9,… pic.twitter.com/BUrMQVR808August 12, 2026Around the same time, photographer Joel Kowsky managed to line up a beautiful shot of the ISS as it passed across the face of our eclipsed star in the skies over Hodgdon, Maine.This gif shows the ISS' silhouette moving across the sun's face during a partial solar eclipse on Aug. 12, 2026. (Image credit: NASA/Joel Kowsky)The dual spacecraft of the European Space Agency's Proba-3 mission also captured a lovely (though largely redundant) view of the moon moving to occult the sun's disk, which, in this case, was already perfectly hidden behind the lead spacecraft's coronograph!Both Proba-3 spacecraft are designed to fly in perfect formation in line with the sun. The "Occulter" spacecraft, closest to the sun, is equipped with a large sunshield, or coronagraph. This coronagraph blocks the sun's disk for the more distant member in the Proba-3 formation, allowing that spacecraft to image our star's atmosphere in incredible detail. The sun's disk is pictured hidden behind the coronograph of the lead Proba-3 spacecraft with the moon's silhouette above, just hours before the Aug. 12 total solar eclipse. (Image credit: ESA/Proba-3/ASPIICS under CC BY-SA 3.0 IGO, alterations made in Canva by Anthony Wood.)Thanks to their unique setup, for a brief moment on Aug. 12, the Proba-3 spacecraft recorded a rare double eclipse, as the moon and its artificial mimic simultaneously hid light emanating from our parent star.Sitting about 22,370 miles (36,000 kilometers) above Earth's surface, ESA's Meteosat Third Generation Imager Satellite (MGT-I1) caught a spectacular view of the moon's shadow darkening our planet.Solar eclipse as seen from space! From its vantage point in space, the Meteosat Third Generation Imager satellite (MTG-I1) captured the Moon’s dark shadow as it passed over Earth’s surface – converging with the advancing twilight shadow as dusk fell over Europe.… pic.twitter.com/dAQVyuXiIPAugust 13, 2026The moon's shadow can be seen arcing south in the satellite imagery, before eventually co

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They really launched this tiny spacecraft (Well, sort of.) | Space photo of the day for May 11, 2026
Science
USA Today·Yesterday

They really launched this tiny spacecraft (Well, sort of.) | Space photo of the day for May 11, 2026

Rockets launch almost every day in the US. Here's why even more are ahead USA Today What’s launching from Florida this week? SpaceX rocket launch schedule Yahoo How SpaceX’s Launch Boom Is Reshaping Space Coast Nightlife Space Coast Daily Pictures: 52 Space Coast launches and counting in 2026 Orlando Sentinel Space Coast launch schedule: sun-sentinel.com

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ScienceSpace.com·2d ago

Guest Column: Where have the long-spined black sea urchins gone?

The distant galaxy J0148-4214, seen in the light of ionized hydrogen. The image appears pixelated because of the great distance to the galaxy. The black circles denote the relative locations of the three black holes. (Image credit: Hannah Übler) A trio of heavyweight black holes are entangled in a dance of death that will quite possibly see them gradually all merge to form an even greater behemoth.Scientists have discovered the black holes in a galaxy that is so far away its light has taken 12.5 billion years to reach us, meaning we see it as it was less than 1.3 billion years after the Big Bang. And it's offering strong supporting evidence that one of the ways black holes grew so massive so quickly in the early universe was through mergers."This is the first evidence of three active black holes in a single galaxy in the distant universe," Hannah Übler, an astronomer at the Max Planck Institute for Extraterrestrial Physics in Germany who led the study, said in a statement. "It suggests that processes in the early universe were efficient at bringing massive black holes together, setting the stage for the massive black-hole mergers we expect to detect with future gravitational-wave observatories."The galaxy that plays host to the black holes is catalogued as J0148-4214 and is so far away (their redshift is 5.0167) that the James Webb Space Telescope (JWST), which made the discovery, could not see the black holes directly. Instead, the Integrated Field Spectroscopy unit on the JWST's Near Infrared Spectrometer (NIRSpec) measured the motion of hydrogen gas swirling around at high velocity in the accretion disks encircling each black hole."The JWST data allowed us not only to identify the three black holes, but also to estimate their masses, accretion rates and the stellar mass of the galaxy," Giovanni Mazzolari of the Max Planck Institute for Extraterrestrial Physics said in the statement. "We find a total stellar mass of about 1.3 billion suns, and the black holes represent a significant fraction of that."Two of the black holes reside at the center of J0148-4214, separated by 620 light-years. One of these black holes has a huge mass of 80 million times the mass of our sun, while its companion is a relative pipsqueak at 600,000 solar masses. Yet despite its diminutive stature, the smaller black hole is growing at a tremendous rate by accreting gas faster than the Eddington limit. This is the theoretical maximum rate at which material can fall towards a black hole; if the rate is any higher then the accretion disk around the black hole becomes so dense and hot that radiation from the disk blows material back out again, stifling the black hole's feeding frenzy. This means the smaller black hole will only be able to keep growing at this rate for a short time before negative feedback calls a halt.The third black hole is 5,500 light-years out from the center of J0148-4214 and has a mass two million times greater than the mass of our sun. This is about half the mass of the supermassive black hole at the center of our Milky Way galaxy, called Sagittarius A*. It's thought that this third black hole, and quite possibly the second one too, found their way into J0148-4214 via mergers between galaxies."These results are extremely exciting," said Roberto Maiolini of the University of Cambridge, who was a participant in the findings. "They suggest that black-hole merging may be an additional, fast route for their rapid growth in the early universe." An image of Sagittarius A*, the supermassive black hole at the heart of the Milky Way. (Image credit: EHT Collaboration)Mergers between black holes produce bursts of gravitational waves. Current gravitational-wave detectors — including The Laser Interferometer Gravitational-Wave Observatory (LIGO) in the United States, Virgo in Italy and KAGRA in Japan — are able to detect the high frequency, short wavelength gravitational waves from the mergers of stellar-mass black holes, the kind formed in cert

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Remembering 'Ulysses 31', the '80s cartoon that transported 'The Odyssey' to outer space
Science
Space.com·2d ago

Remembering 'Ulysses 31', the '80s cartoon that transported 'The Odyssey' to outer space

This artist's representation highlights the streamer feeding material onto the protoplanetary disk, GW Ori, creating misaligned dust rings. (Image credit: NSF/AUI/NSF NRAO/B.Saxton) A rare planet-forming disk around a young triple-star system in the Orion constellation has been tipped over by a river of gas over 1 trillion miles (1.6 trillion kilometers) long. The discovery, made at radio wavelengths with ALMA, the Atacama Large Millimeter/submillimeter Array in Chile, could explain why astronomers keep finding planets with orbits that are drastically misaligned with the rotational axes of their stars.GW Orionis is a triple system consisting of three pre-main sequence stars, meaning that they are still forming and contracting and have not yet initiated fusion reactions of hydrogen in their core. The stars are located roughly 1,300 light-years away, in the Lambda Orionis star-forming molecular ring in the constellation of Orion, the Hunter. Finding a planet-forming disk of gas and dust encircling all three stars in a system is very rare, and finding a disk consisting of three rings with misaligned orbits is even stranger."Previous studies of GW Orionis revealed that the system's inner, middle and outer rings are misaligned, with each ring tilted at a different angle," said Maria Galloway-Sprietsma, a PhD student at the University of Florida who led the research, in a statement.The outer ring, which is one of the largest ever seen around a young star, is the most noticeably misaligned. It had previously been thought that an unseen gas giant planet, having carved out a gap between the middle and outer ring, was perturbing the outer ring.Now though, Galloway-Sprietsma and colleagues have discovered the hidden truth: an enormous finger of gas reaching in from the surrounding molecular cloud is disturbing the outer ring, and the exchange of angular momentum, or rotational energy, between the two is warping the ring and tipping it over.The disk around GW Orionis is composed of three rings, beginning at radii of 4.1, 17.4 and 31.6 billion miles (6.7, 28 and 51 billion kilometers/44, 187 and 340 astronomical units) from the center of the tight triple system.The streamer of gas tilting the system's outer ring was discovered through new ALMA observations. Such streamers are thought to be how stars grow, delivering mass onto nascent suns. The streamer is composed mostly of molecular hydrogen, but since molecular hydrogen is invisible at radio wavelengths, ALMA searched for molecules of carbon monoxide in the streamer instead.The length of the streamer is astounding, stretching 0.2 light years (12,600 astronomical units, 1.9 trillion kilometers or 1.2 trillion miles)."When our team modeled the infall of this streamer, we found that the angle at which it impacts the disk is closely aligned with the outer ring," said Galloway-Sprietsma. This superimposed image of of the GW Orionis star system shows images from the ALMA radio telescope (in blue) overlayed on the ESO Very Large Telescope's SPHERE instrument's view, which shows the shadow of the system's innermost ring. (Image credit: ESO/Exeter/Kraus et al., ALMA (ESO/NAOJ/NRAO))It is believed that the streamer has already done most of the work in tipping over the outer ring of the disk. Today, its angular momentum, or spin, is less than that of the disk."In the past it likely had a greater angular momentum, and that allowed the disk to become misaligned," said Bae.The discovery of the streamer might put to bed more than just the mystery of what tipped over GW Orionis' disk.In our solar system, all the planets orbit around the sun in the ecliptic plane, which is a narrow plane aligned with the sun's equator and direction of rotation. Most exoplanets orbit their star in similar fashion, but astronomers have also previously discovered some planets that have highly inclined or even retrograde orbits around their star, as though some mighty force had tipped their orbits over. With the discovery

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'This is unprecedented': Why the Pentagon's recent UFO file releases are so important
Science
Space.com·2d ago

'This is unprecedented': Why the Pentagon's recent UFO file releases are so important

Navy pilots have reported encountering a variety of unidentified aerial phenomena (UAP). (Image credit: DOD/U.S. Navy) As "The X Files" famously told us, "the truth is out there." But at the same time, inquiring minds are immersed today in finding out whether or not the proof is out there — specifically, proof that at least some unidentified anomalous phenomena (UAP) come from somewhere beyond Earth.The UAP acronym originally stood for "unidentified aerial phenomena," a term that itself was a rebranding of "unidentified flying object" (UFO). And UFO was a replacement of sorts for the long-lasting and stylish "flying saucers."Whatever the terminology, truth and proof in today's fractured and somewhat conspiratorial society could be construed as strange bedfellows.UAP study teamMike Gold is president at Redwire Space, an innovative aerospace and defense company. In 2022 and 2023, he served on the NASA Unidentified Anomalous Phenomena Independent Study Team, a council of 16 experts across diverse areas on matters relevant to potential ways to investigate UAP.Gold's past roles include NASA associate administrator for space policy and partnerships, acting associate administrator for the Office of International and Interagency Relations, and senior advisor to the administrator for international and legal affairs. While at NASA, he led the development and implementation of the Artemis Accords.That past also includes 13 years at Bigelow Aerospace, during which he established the company's Washington office and oversaw the launches of Bigelow's Genesis 1 and Genesis 2 spacecraft, which showcased the use of expandable habitat technology. A public meeting of NASA's Unidentified Anomalous Phenomena (UAP) Independent Study Team on May 31, 2023. Mike Gold is second from the right in the front row. (Image credit: NASA/Joel Kowsky)Exposing the truthGold's ongoing UAP interests were highlighted in 2024 during a hearing of the U.S. House of Representatives' Committee on Oversight and Accountability titled "Unidentified Anomalous Phenomena: Exposing the Truth.""We must be thorough in collecting information, fearless in making conclusions and open to following the data no matter how mundane or extraordinary the results may be," Gold told the lawmakers. "As the saying goes, the truth is out there. We just need to be bold enough and brave enough to face it."Space.com caught up with Gold recently to discuss his current UAP views and his work with The Disclosure Foundation as an advisory board member. A "football-shaped" UAP (unidentified anomalous phenomenon) observed by an infrared sensor on a U.S. military platform in 2024. The Pentagon released this observation on May 8, 2026. (Image credit: U.S. Deparment of War)Follow the data"I would say that I came out the same way I came in," Gold said of his past work for the NASA UAP study team, "and that was objective and wanting to follow the data."While the NASA group's final recommendations seem to be lost in the fabric of time and space, Gold said that, under the current presidential administration, NASA is taking the UAP issue quite seriously, as is the rest of the federal government."NASA is doing its best to contribute to the Department of War releases on UAP," said Gold. "I will note that what is being released by NASA is publicly available and has been. But I think it's beneficial for the White House to flag some of the most interesting aspects that we have from NASA archives."Gold said, for instance, that the 1972 Apollo 17 moon landing report included imagery showing three lights in a triangular shape that was flagged in recent Department of War (DOW)/NASA-released documents."NASA is a proactive participant in all of this," he added, noting that having imagery identified as anomalous is "very powerful in fighting the stigma."There are champions inside the space agency who want to pursue the UAP issue, according to Gold."They feel a lot more comfortable when you've got the White House putting

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NASA funds spherical 'Aerobots' that could explore the caves of Saturn's moon Titan
Science
Space.com·3d ago

NASA funds spherical 'Aerobots' that could explore the caves of Saturn's moon Titan

A composite image of an infrared view of Saturn's moon Titan from NASA's Cassini spacecraft; renderings of several "SPARK" Aerobots being developed by Daniel Drew of the University of Hawaii. (Image credit: NASA/JPL/University of Arizona/University of Idaho/Daniel Drew/University of Hawaii) Spherical "Aerobots" may one day swarm the caves of Titan — a moon of Saturn that NASA says is one of the most Earthlike in our solar system.Titan is covered in rivers, lakes and seas of hydrocarbons, like methane and ethane, as well as a strange "karst" terrain including underground sinkholes and caves. No rover could easily traverse this surface, but flying vehicles may have more success.So a new grant, under the early-stage NASA Innovative Advanced Concepts (NIAC) program, aims to create small, flying vehicles that could explore those caves. It's unclear if the aerobots — called SPARK, or Solid-state Propulsion for Autonomous Reconnaissance of Karst — would be ready in time for NASA's Dragonfly mission to Titan, project lead Daniel Drew, an assistant professor at the University of Hawaii at Mānoa, told Space.com.That's because SPARK is beginning a nine-month Phase 1 grant and would need to at least get through the up-to-two-year Phase 2 before things look "more realistic" for a liftoff, he noted. Dragonfly, meanwhile, is targeted for a 2028 launch but if the mission is delayed, that provides more possibilities for late-mission additions."Where does that line up with the current Titan mission timeline, assuming we've missed the window for Dragonfly? I don't know," Drew said of SPARK. But whenever the mission lifts off, Drew said SPARK has a good chance of doing well on Titan with its novel ion (electric) thrusters.Drew said his design could "provide persistence, maneuverability, robustness to the challenging near-cryogenic [icy] conditions, and minimize downwash disturbance of scientifically-important hydrocarbon layering." He hopes that SPARK, he added, could be a cave-exploration forerunner at Titan similar to the Ingenuity helicopter on Mars that made 72 flights — more than tenfold what the Red Planet demo mission was supposed to do.Drew has been working on a particular type of ion thrusters, called electrohydrodynamic (EHD) propulsion, since he did graduate school at the University of California, Berkeley. Thanks in part to a National Science Foundation (NSF) fellowship, Drew explored several designs for flying and became interested in creating robots that flap their wings in a way similar to real-life creatures.While exploring, he stumbled on the hobbyist "lifter" community "pretty much by chance," he said. "These [prototypes] are triangular balsa wood, magnet wire, and aluminum foil prototypes. You connect them to 40,000 volts from a flyback transformer that you rip out of a microwave or CRT monitor or whatever, and they can float above the table. There are plenty of examples of people making these on YouTube," he said.More plumbing the archives revealed early experiments and studies at NASA and the Air Force similar to what the hobbyists were using. And by coincidence, NIAC awarded funding to another research group, led by the Massachusetts Institute of Technology, that was interested in using EHD propulsion for Earthborne aircraft. As such, Drew sensed a fruitful direction for research."Long story short, I ran with that idea," Drew said, "and wrote a bunch of papers where I created microfabricated centimeter-scale flying robots propelled by atmospheric ion thrusters." His accomplishments prior to the NIAC grant included what he says is the first demonstration of microfabricated EHD actuators (mechanical devices), and other firsts such as a centimeter-scale "ionocraft" taking off and subsequently, carrying a payload."We recently published the design and takeoff of the first ion-propelled micro-hovercraft," he added, referring to a paper on preprint server arXiv. "That may seem like a pretty decent list of significant milestones,

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Should we trust AI in the search for alien life? Scientists aren't so sure
Science
Space.com·4d ago

Should we trust AI in the search for alien life? Scientists aren't so sure

On Aug. 15, 1977, astronomers using Ohio State University's Big Ear radio telescope detected the famous "Wow!" signal, which to this day is one of the strongest pieces of evidence that we are not alone in the universe.Astronomer Jerry Ehman was using the telescope to scan a region in the constellation Sagittarius when it detected a weird, 72-second-long radio burst. The signal was too strong to be explained by background noise, and researchers determined that it was very unlikely that this signal came from anything on Earth.Despite their best efforts, astronomers have not been able to detect any other signals like it. The now-famous "Wow!" signal. (Image credit: Public domain)Why it matteredFor as long as humans have existed, we have looked up and wondered, "Are we alone?" This question remains one of the biggest mysteries across not just science but for humanity as a whole. The "Wow" signal remains an iconic and important finding in the search for life out in the cosmos.Nearly 50 years since the "Wow!" signal, scientists have made incredible progress in the search for alien life. We have landed rovers on Mars that have found possible signs of life on the Red Planet, for example, and discovered thousands of exoplanets, or planets outside of our solar system.The "Wow!" signal was detected nearly two decades before scientists first confirmed the existence of exoplanets. Today, we have found more than 6,000 of them and are using cutting-edge technologies to explore further and see if any of these far-off planets might contain signs of life.

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The moon shines with a swarm of stars on May 21 as Jupiter, Venus and Mercury line-up nearby
Science
Space.com·5d ago

The moon shines with a swarm of stars on May 21 as Jupiter, Venus and Mercury line-up nearby

As Venus wanes to a crescent, its disk gets bigger, and it reaches its brightest. (Image credit: Jamie Cooper/SSPL/Getty Images via Getty Images) Can Venus cast a shadow? With Aug. 12's total solar eclipse — where the moon's dark silhouette is everything — now behind us, it's a good time to test another kind of celestial shadow.Astronomical folklore has it that the second rock from the sun, Venus, is, after the sun and moon, the third object able to cast a shadow when it's near peak brightness, albeit extremely faint, according to EarthSky.Is it true? Not in a city, where skylights glow and porch lights blaze, where shadows are mostly thrown by passing cars that appear to become the brightest object in the solar system briefly. Venus does cast a shadow, but the sky must be very dark, transparent and free of any light — apparently.Timing is everything. Having reached dichotomy — its half-lit phase — on Aug. 12, Venus is currently 49%-lit and waning as it moves closer to Earth, increasing in angular size as it becomes a slim crescent. Cue a surge in brightness, thanks to its reflective clouds and its closeness. Shouldn't it be brightest when it's "full?" No, because it's an inferior planet — i.e., it orbits closer to the sun — so it's fully lit only when it's on the other side of the sun from Earth, when its disk appears at its smallest.What’s happening and when to lookVenus is beautifully placed this week because it reaches greatest eastern elongation, its widest apparent separation from the sun in the evening sky. Look low in the west after sunset — Venus will be the bright white "star" that appears before the fainter stars even have a chance.On Aug. 14-15, it sits about 46 degrees from the sun and shines at a magnitude of -4.3 to -4.4, bright enough to dominate twilight but not quite at its most impressive stage of the apparition. The real test comes around Sept. 18, when Venus reaches its greatest brilliancy at magnitude -4.6. Sadly, by then it's going to be rather low in the sky from mid-northern latitudes, making observation from the U.K. difficult, but possible from most of the U.S. Venus shines over the Mitsuke Iwa Rock in Ishikawa, Japan. (Image credit: Yuga Kurita via Getty Images)How and when I’m watching itAccording to Sky & Telescope, to catch a faint but well-defined shadow of Venus — a point source of light — you'll need to be somewhere free from artificial lighting and wait until twilight is over. Face Venus and place a white surface (a white card or sheet works well) also facing Venus. You'll also need to position something in front of the card to cast a shadow. Although it is possible to see the faint shadow of Venus, photographing the card is the best way to capture it, using a technique similar to that for any night sky photograph — a high ISO, a wide aperture and a long exposure of up to 30 seconds. It may be wise to test the location, find the best line of sight, and work out where the card needs to go while Venus is still high enough above the western horizon.If you're not in a good location to catch the shadow of Venus, instead try to see and photograph the light from Venus reflecting on water. Any pond, lake or ocean you can get between you and Venus ought to catch its shine in a long exposure image. That identical technique — high ISO, a wide aperture and a long exposure — will also apply, but this time you can actually aim your camera at Venus!Stargazer’s Corner: August 14-20, 2026This is an excellent week for darkness and faint objects. With new moon on Aug. 12, this week is all about a crescent moon. On Aug. 15 you may catch a 12%-lit waxing crescent close to Venus, but more likely you'll see it on Aug, 16, when it will be 19%-lit. The latter occasion is one to aim for — a beautiful sight. On both occasions, look for "earthshine" on the darkened limb of the moon — sunlight reflected by Earth, and something else you can try to capture with a long exposure. The waxing crescent moon will be low in the

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'Thor' hammered down 15 years ago, and it's still the only Marvel movie to do the God of Thunder justice
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Space.com·6d ago

'Thor' hammered down 15 years ago, and it's still the only Marvel movie to do the God of Thunder justice

(Image credit: Mattel / The Cannon Group) For the generation that grew up in the 1980s, the release of the recent big-budget "Masters of the Universe" movie would undoubtedly have conjured up a sense of déjà-vu.Picture the scene. The year is 1987. You've got the action figures and the Castle Grayskull playset, you've watched every episode of the cartoon again and again, and you can recite He-Man's opening credits voiceover by heart. He has the power!Then someone tells you there's a live-action film adaptation coming out.You persuade your parents to take you to the theater, pick up a great big bucket of popcorn, and get ready to be transported to the familiar surroundings of Eternia. And then…Well, it's fair to say this is not the "Masters of the Universe" you know and love. Sure, leading man Dolph Lundgren is big, but why does he look and dress nothing like He-Man? Who's that Gwildor guy, and what the hell happened to Orko, BattleCat and Prince Adam? Why do He-Man and Skeletor spend so much of the movie on planet Earth? And when are we going to hear that famous theme tune? (Spoiler: you won't.) (Image credit: Mattel / The Cannon Group)By the power of Grayskull, this was not the film '80s kids expected, or indeed wanted. But disappointing a pre-teen fanbase was the least of "Masters of the Universe"'s worries. Sales of Mattel's previously all-conquering toyline were way past their peak, while the appetite for films trying to capture "Star Wars"' unique blend of sci-fi and fantasy had all but disappeared. Perhaps more importantly, "MOTU" 1987 had been bankrolled by an ambitious but eccentric studio, whose efforts to break into the mainstream had left it in a financial state so perilous that not even the most powerful man in the universe could save it."Masters of the Universe" was one of the undoubted pop culture success stories of the 1980s. Although Mattel had made the mistake of turning down the licence to make "Star Wars" toys, the toy giant responded in spectacular style by launching a fantasy behemoth of its own in 1982. He-Man, Skeletor and their Eternian colleagues would soon become household names, largely thanks to the advertising power of an immensely popular cartoon series.Decades before "Transformers", "The Lego Movie" and "Barbie" made big money at the box office, producer Edward Pressman had seen the potential in taking a toy franchise to the big screen. There had been early interest in "He-Man" from major studios (including Warner Bros), but — largely thanks to delays caused by management changes at Mattel — interest had waned by the time Cannon Films stepped in to foot the bill. Masters of the Universe (1987) ORIGINAL TRAILER [HD 1080p] - YouTube Watch On Throughout the '80s, Cannon had become more renowned for the quantity of its output than the quality, as a pair of ambitious Israeli cousins, Menahem Golan and Yoram Globus, invested in unashamed B-movies like "Enter the Ninja", Charles Bronson's "Death Wish" sequels, and Chuck Norris vehicle "The Delta Force". The studio had around 40 movies in production at the time "Masters of the Universe" got the green light, but was keen to make a move on tentpole blockbuster territory. As well as financing the disastrous "Superman IV: The Quest for Peace", Cannon had also paid Sylvester Stallone a record-breaking fee to headline arm-wrestling drama "Over the Top". Both flopped at the box office.Despite being "a little bit reluctant because it was [based on] a toy line", Stallone's "Rocky IV" co-star Dolph Lundgren signed up to play the mighty He-Man. The Swedish actor looked more like the lead singer of a hair metal band than the sword-wielding hero of the cartoons, though his impressive physique (coupled with He-Man's scanty wardrobe) ensured it was hard to find a convincing stunt double.Director Gary Goddard also became concerned that his leading man (topping the bill for the first time) wasn't delivering dialogue as he wanted, and subtly chopped some of Lundgren's

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ScienceSpace.com·Aug 12

Perseid meteor shower peaks under perfect skies tonight — here's what to expect

Don't miss the Perseid meteor shower 2026 peak tonight. (Image credit: Background: Kevin Key / Slworking via Getty Images, Text and notification symbol added in Canva Pro.) The Perseid meteor shower, one of the most prolific and impressive meteor showers of the year, peaks tonight!Widely regarded as one of the best meteor showers of the year, the Perseids can produce up to 100 meteors per hour under ideal viewing conditions and weather permitting.This year's display is particularly favorable because the shower peaks on the night of the new moon, leaving skies free from bright moonlight that can wash out fainter meteors.What time should I look?The Perseids can produce meteors throughout the night, but the best viewing begins around 11 p.m. local time, with activity increasing after midnight and continuing until the predawn hours. Under dark, clear skies, patient observers could see dozens of meteors every hour with the highest rates expected just before dawn.Where do they come from?The annual show occurs as Earth passes through a trail of comet dust and rocky debris left behind by Comet 109P/Swift-Tuttle. Every year, our planet plows through this stream of cometary material, causing tiny fragments — many no larger than a grain of sand — to slam into Earth's atmosphere at around 133,000 mph (214,000 km/h).As these particles compress and heat the air in front of them, they burn up high above Earth's surface, creating the brilliant streaks of light we know as meteors or shooting stars. Every year, Earth passes through the path of Comet Swift-Tuttle. With the Perseid meteor shower's peak occurring when Earth passes through the densest, dustiest area. (Image credit: Future)How can I see the Perseids? The Perseids appear to radiate from the constellation Perseus, but you don't need to look directly at the constellation to enjoy the show. In fact, the longest and brightest meteors appear about 45 degrees away from the radiant, when you're not viewing them head-on.To give yourself the best chance of seeing as many meteors as possible, head somewhere with dark skies, away from city lights and give your eyes around 30 minutes to adjust to the darkness. Avoid checking bright phone screens (easier said than done!) and leave the telescope or binoculars at home — meteors are best enjoyed with the naked eye. The Perseid meteor shower will appear to radiate from the Perseus constellation. (Image credit: Future)The highest number of meteors occurs in the predawn hours because it's when the side of Earth you're situated on has rotated into the stream of comet debris. You can think of it a bit like driving through rain — the windshield catches more raindrops than the rear window because it's facing the direction of travel. Likewise, before dawn, your location on Earth is facing into the stream of comet debris, meaning more meteoroids collide with Earth's atmosphere overhead.A rare double sky showBest cameras for astrophotography (Image credit: Nikon)If you're looking for a good camera for meteor showers and astrophotography, our top pick is the Nikon D850.Why have one remarkable sky event when you can have two? This year's Perseid peak arrives on the heels of today's total solar eclipse that crosses parts of Greenland, Iceland and Spain, making it possible to witness two of the year's most spectacular celestial events within just a few hours of each other.If you're unable to catch the Perseids tonight, don't worry! While meteor numbers will gradually decline after the peak, the Perseids remain active through Aug. 24, meaning there are still opportunities to catch plenty of shooting stars under clear, dark skies.If you're looking to snap photos of the meteor shower or the night sky in general, check out our guide on how to photograph meteor showers, as well as our best cameras for astrophotography and best lenses for astrophotography. Daisy Dobrijevic joined Space.com in February 2022, having previously worked as a staff writer for All About

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