European spacecraft got rare close-up of Mars' lesser-known moon
A European spacecraft on a journey to study NASA's asteroid crash site did a quick pop-in of Mars on its way, capturing unprecedented images of Mars' lesser-known moon, Deimos.
Mars has two moons, Phobos and Deimos, but scientists know relatively little about them, especially the smaller one, Deimos. Nearly all of the images they have of it were taken from the Martian surface by rovers, and because the moon is tidally locked — meaning one full spin matches the amount of time it takes to complete its orbit of Mars — only one side has been seen on the Red Planet.
The Hera mission spacecraft captured views of the moon's far side, swinging within 625 miles of Deimos in space.
While the car-sized spacecraft flew around the Mars system, flight controllers on Earth temporarily lost communication with Hera because the signal was blocked. Though the blackout was planned for the maneuver, Ian Carnelli, the European Space Agency's Hera mission manager, said it was deeply emotional.
"I was almost in tears. I mean, I know probably this is normal for a flight for spacecraft operators, but every time we lose contact with a spacecraft, I'm super nervous," he said during a webcast following the flyby. "Then I was running to the room where the scientists were [watching for images], and as soon as I opened the door, they were screaming — really screaming."
SEE ALSO: Scientists found huge beaches on Mars likely from a long gone ocean
Among those scientists was one of the co-founders of Queen. When Brian May isn't playing guitar riffs, he is an astrophysicist. As part of Hera's science team, May brings his expertise in stereoscopic imaging. That means he helps decipher complex scientific data into 3D pictures.
During a webcast on Thursday, May described some of the topographical details of the moon already brought to life through the raw data. A depression in the city-sized moon was visible, a feature May described as a "saddle" on the left side and some little craters at the bottom.
"You feel like you're there, and you see the whole scene in front of you," he said. "The science that we get from this is colossal, and I think we're all like children."
Hera launched in October 2024 and will rendezvous with Dimorphos, an asteroid previously slammed by a NASA spacecraft, in 2026. Back in 2022, NASA deliberately crashed a spacecraft into a harmless asteroid to practice thwarting a space rock, should a hazardous one ever be on a collision course with Earth. The European Space Agency is providing a follow-up to that test.
Deimos, one of Mars' two moons, is eight miles wide and orbits about 14,600 miles away from the Red Planet. Credit: ESA
The flyby of Mars and Deimos wasn't a detour but a necessary maneuver to put the spacecraft on the right trajectory toward its ultimate destination. Swinging within 3,100 miles of Mars, Hera used its gravity to adjust its course.
Scientists would like to understand where Deimos and its partner Phobos came from — whether they were once asteroids captured in orbit around Mars or are chunks of the planet itself, blown out by a giant impact.
The new data may help them figure out the moon's origin. During the flyby, three instruments were used: a black-and-white navigation camera that takes pictures in visible light; a hyperspectral imager that can help discern an object's mineral composition; and a thermal infrared imager supplied by the Japanese space agency, JAXA, which can help characterize the texture and density of the material. Overall, thousands of images were collected, and the Hera team is still processing them.
At the top of this story is an infrared photo of Deimos, backdropped by Mars. The Red Planet appears pale blue because the sun is shining on it. Its contribution to this scene would need to be removed for the colors to appear closer to how they would really look to our eyes.
A thermal camera on the Hera spacecraft took images that will help scientists characterize the texture and density of the material that makes up Deimos. Credit: ESA / JAXA
Near the top of the image is the bright Terra Sabaea region, close to the Martian equator. At the bottom right of the region is the Huygen crater, and to its left is the Schiaparelli crater. At the bottom right of the planet is Hellas Basin, one of the largest known craters in the solar system.
In a little less than two years, Hera will reach the target asteroids from NASA's DART mission to begin a crash investigation.

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National Geographic
26 minutes ago
- National Geographic
Asteroids with ‘unstable orbits' hide around Venus—do they threaten Earth?
NASA's Parker Solar Probe captured this image showing the nightside surface of Venus. A family of asteroids share the planet's orbit, and two new studies suggest that one day the space rocks could theoretically pose a danger to Earth. Photograph by NASA/APL/NRL Venus has groupies—a family of asteroids that share its orbit, either trailing it or leading it as the planet revolves around the sun. Researchers have known that such stealthy space rocks might exist for years, but now, a pair of papers (one published in a journal, and one a pre-print undergoing peer-review) conclude that some might develop unstable orbits and, over a very long period of time, arch toward Earth. But despite what several histrionic headlines have claimed, Earth is not at risk of one of these asteroids suddenly sneaking up on us and vaporizing a city. While some of these asteroids could be large enough to cause this sort of damage, there is no evidence whatsoever suggesting any of these Venus-pursuing asteroids are currently heading our way. 'I wouldn't say that these objects are not dangerous,' says Valerio Carruba, an asteroid dynamicist at the São Paulo State University in Brazil and a co-author of both studies. 'But I don't think there is any reason to panic.' These studies simply highlight that asteroids near Venus have the potential to fly our way on sometime in the next few thousand years or so. 'The likelihood of one colliding with Earth any time soon is extremely low,' says Scott Sheppard, an astronomer at the Carnegie Institution for Science in Washington, D.C. who was not involved with the new research. 'There isn't too much to be worried about here.' Asteroids around Venus, shown in the background above during a 2012 transit, are difficult to track because they fall inside Earth's orbit and are obscured by the sun's glare. Research suggests that some of the asteroids that share Venus' orbit are large enough to take out a city on Earth. Illustration by David A. Hardy, Futures: 50 Years In Space/Science Photo Library The real problem, though, is that asteroids like this are remarkably difficult to find, and you can't protect yourself against a danger you cannot see. Fortunately, in the next few years, two of the most advanced observatories ever built are coming online. And together, they will find more asteroids—including those hiding near Venus—than the sum total already identified by the world's telescopes. Concealed by sunlight While the Japanese and European space agencies mostly request time on busy telescopes to search for these space rocks, NASA leads the pack: It funds a network of observatories solely dedicated to finding sketchy-looking asteroids. Planetary defenders are chiefly concerned about near-Earth asteroids. As the name suggests, these have orbits that hew close to Earth's own. Many of these asteroids were removed from the largely stable belt between Mars and Jupiter, either through the chaotic gravitational pull of the planets (often Jupiter, as it's the most massive) or through asteroid-on-asteroid collisions. If one gets within 4.6 million miles of Earth's orbit, there's a chance that, over time, both orbits cross and a collision becomes possible. And if that asteroid is 460 feet long, it's big enough to plunge through the atmosphere and (with a direct hit) destroy a city. Combined, these characteristics describe 'potentially hazardous asteroids'—and finding them is of paramount importance. Venus appears above giant sandstone cliffs amid the sand dunes of Tassili National Park in Algeria. Photograph by Babak Tafreshi, Nat Geo Image Collection Asteroids are first found because of the sunlight they reflect. That works well for most, but there are known to be asteroids hiding interior to Earth's orbit, toward the direction of the sun. And that's a problem. Astronomers seeking out these asteroids cannot just point their telescopes directly at the sun: It would be like trying to see a lit match in front of a nuclear explosion. Instead, they look in the vicinity of the sun in the few minutes just after sunset, or just before sunrise. Not only are these surveys severely time-limited, but by aiming close to the horizon, they are peering through more of the Earth's atmosphere, which distorts what they are looking at. 'All of these factors make it hard to search for and discover asteroids near Venus' orbit,' says Sheppard. (Here's how researchers track asteroids that might hit Earth.) The invisible Venusian fleet Asteroids have occasionally been spotted in this sun-bleached corner of space. And twenty of them have been found scooting along the same orbital highway Venus uses to orbit the sun. These are known as co-orbital asteroids; similar rocks can be found either following or trailing other planets, most notably Jupiter. Co-orbiting asteroids tend to cluster around several gravitationally stable sections, known as Lagrange points, along the planet's orbital path. But over a timescale of about 12,000 years or so, it's thought that the Venus co-orbital asteroids can dramatically alter their orbits. They remain on the same orbital path as Venus, but instead of maintaining a circular orbit, they get creative: Some migrate to a different Lagrange point, while others zip about in a horseshoe pattern around several Lagrange points. Some of these new, exotic orbits become quite stretched-out and elliptical—and, in some cases, these orbits can eventually bring these asteroids closer to Earth. When they do, 'there is a higher chance of a collision,' says Carruba. In their first study, published in the journal Icarus earlier this year, Carruba and his team looked at the 20 known co-orbital asteroids of Venus. Their simulations forecast how their orbits would evolve over time and show that three of the space rocks—each between 1,000 and 1,300 feet or so—could approach within 46,500 miles of Earth's orbit. (For reference, the moon is an average of 240,000 miles from our planet.) That proximity may make them potentially hazardous asteroids. But there's no need to worry—it can take as long as 12,000 years for an asteroid to end up on an elliptical, near-Earth orbit. Perhaps they will be a problem for our very, very distant descendants. The asteroids that hang out in the orbit of Venus (shown above in simulated color) are largely unknown. This illustration shows the orbits of the binary near-Earth asteroid Didymos (labelled) and another 2,200 potentially hazardous asteroids (fainter lines) around the sun. Illustration by NASA/JPL-Caltech/Science Photo Library The team's latest study, uploaded to the pre-print server arXiv last month, delves into how easy it might be for any of Venus' co-orbital asteroids—including those astronomers have yet to find—to end up on these precarious orbits. To find out, they created virtual asteroids and simulated their many potential orbital voyages 36,000 years into the future. Many things could perturb the orbits of asteroids over that many years, so any truly accurate predictions are impossible. But the simulations came to some broad conclusions. The first is that a Venus co-orbital asteroid is more likely to approach Earth if it switches from a circular to a considerably elongated orbit—it's zooming over a larger patch of the inner solar system, including our own planet's neighborhood. The second, more surprising thing, is that some asteroids still manage to reach near-Earth space even they start out with only a mildly stretched-out orbit. It seems that their chaotic journeys through space, filled with gravitational disturbances, can still end up throwing them our way. But to be clear, these potentially worrisome orbits develop over the course of many millennia. 'This is not something to be alarmed about, as these asteroids are still relatively dynamically stable on human timescales,' says Sheppard. (These five asteroids pose the highest risk to Earth.) A new asteroid-hunting dawn For Marco Fenucci, a near-Earth object dynamicist at the European Space Agency, the paper raises awareness about these relatively mysterious asteroids in Venus' orbit. And that is a good point to make, he adds: We don't know much about these asteroids, including their population size, their dimensions, and their orbits, because we struggle to find them with today's telescopes. Two upcoming facilities are about to make this task considerably easier. The first, the U.S.-owned Vera C. Rubin Observatory in Chile is set to officially come online in the next few weeks. With a huge field-of-view, it can see huge swathes of the night sky at once, and its giant nest of mirrors can gather so much starlight than even the smallest, faintest objects can be seen. In just three to six months, the observatory could find as many as a million new asteroids, effectively doubling the current total. Meg Schwamb, a planetary scientist at Queen's University Belfast who was not involved with the new research, explains that Rubin will also conduct its own twilight surveys, the very sort used today to search for near-Venus asteroids. If these surveys are conducted over the next decade, 'Rubin could find as many as 40 to 50 percent of all objects larger than about [1,150 feet] in the interior-to-Venus-orbit population,' says Mario Jurić, an astronomer at the University of Washington and who was not involved with the new research. But, as with all ground-based optical telescopes, Rubin will still have the sun's glare, and Earth's atmosphere, to contend with. As long as the federal government decides to continue to fund the mission—something that is not guaranteed—NASA will also launch a dedicated asteroid-hunting space observatory, the Near-Earth Object (NEO) Surveyor, in the next few years. Unobstructed by Earth's atmosphere, it will seek out space rocks by viewing them through a highly-sensitive infrared scope, meaning it can see those hidden by the luminous sun. Even those asteroids sneaking around near Venus won't be able to hide from NEO Surveyor. And, finally, says Carruba, 'we can see if the impact threat is real, or not.'
Yahoo
an hour ago
- Yahoo
Bug-eyed telescope ready to find Earth-smashing asteroids
It's only a matter of time before a catastrophically sized asteroid barrels towards Earth again. Until very recently in human history, there was no way of knowing if one was hurtling towards us, much less do anything to alter its path. Now, international space agencies and disaster preparedness experts have powerful tools to keep watch over the skies—and the newest aide just opened its bug-inspired compound 'eye.' According to the European Space Agency, the Flyeye-1 telescope recently completed its 'first light' test at the Italian Space Agency's Space Geodesy Center, located about 160 miles east of Naples. Soon, it and as many as three other similar installations around the world will work in tandem to provide comprehensive, automated surveys of space every night to scan for cosmic threats. 'The earlier we spot potentially hazardous asteroids, the more time we have to assess them and, if necessary, prepare a response,' explains Richard Moissl, Head of ESA's Planetary Defence Office. 'ESA's Flyeye telescopes will be an early-warning system, and their discoveries will be shared with the global planetary defence community.' Similar to an insect's vision (hence its name), Flyeye captures incoming light through its 3.3-foot-wide primary mirror. That light is divided into 16 independent channels, all equipped with their own secondary lens and detector cameras designed to flag extremely faint objects. Flyeye's automated observation schedule is designed to factor in variables such as lunar brightness along with other survey telescopes like NASA's ATLAS, the Zwicky Transient Facility, and the forthcoming Vera Rubin Telescope. So what happens if Flyeye spies a suspicious space rock out there in deep space? The plan is for experts at ESA's Near-Earth Object Coordination Center (NEOCC) to review and verify any potential concerns. If the situation warrants further investigation, the NEOCC will then forward their report to the Minor Planet Center, a global hub for asteroid data. Subsequent research will lead to international contingency planning, which could involve any number of solutions, such as smacking the asteroid off course with a targeted spacecraft launch. Before that can happen, Flyeye needed to demonstrate its up to the task. For its first light test, Flyeye focused on multiple known asteroids, including 2025 KQ. Astronomers discovered the space rock only two days earlier, offering direct proof that the telescope is already capable of rapid follow-up observations. 'These images of the sky above the ancient stone hills of Matera, Italy, are more than just a test—they are proof that Flyeye is ready to begin its mission,' ESA said in its announcement. Flyeye-1 is now on its way for installation on Monte Mulfara in Sicily. If all goes according to plan, the telescope's first sibling will be up and running sometime in 2028.


Newsweek
an hour ago
- Newsweek
NASA Tracking Three Asteroids Approaching Earth
Based on facts, either observed and verified firsthand by the reporter, or reported and verified from knowledgeable sources. Newsweek AI is in beta. Translations may contain inaccuracies—please refer to the original content. NASA is monitoring three asteroids soaring past the Earth at about 8,000 to 15,000 miles per hour, the biggest of which measures around 1,300 feet in diameter. The largest space rock, known as "424482 (2008 DG5)," is due to zip past our planet at over 13,800 miles per hour later today. It is expected to come as close as 2.17 million miles from the Earth, according to NASA's Jet Propulsion Laboratory (JPL), A smaller asteroid known as "2025 LD," which is around 73 feet in diameter, zoomed past the Earth earlier today at over 15,000 miles per hour, according to the JPL's Center for Near-Earth Object Studies (CNEOS). The space rock came as close as 696,000 miles from the Earth. A third asteroid, known as "2025 KY4," measuring around 42 feet in diameter, also zipped past the Earth earlier today, reaching within 1.72 million miles of our planet. The asteroid soared past at over 8,000 miles per hour. Stock image: An illustration of asteroids floating around in space. Stock image: An illustration of asteroids floating around in space. Getty Asteroids—small, rocky masses left over from the formation of the solar system nearly 4.6 billion years ago—are found in the main asteroid belt, orbiting around the sun between the paths of Mars and Jupiter. In February, data from the CNEOS showed the impact probability of an asteroid known as "2024 YR4" in 2032 was at 3.1 percent. This was "the highest impact probability NASA has ever recorded for an object of this size or larger," the national space agency noted at the time. Further studies that month brought 2024 YR4's chance of Earth impact on December 22 in 2032 down to 0.004 percent. The data showed there is "no significant potential" for 2024 YR4 to "impact our planet for the next century" and "the range of possible locations the asteroid could be on Dec. 22, 2032, has moved farther away from the Earth," NASA said in a blog post on February 24. 2024 YR4 was measured to be about 200 feet across by NASA's James Webb Space Telescope, Andy Rivkin, an astronomer at the Johns Hopkins University Applied Physics Laboratory, noted in a NASA blog post on April 2. There is still a "very small chance," however, for 2024 YR4 to impact the moon on that date, and that probability is currently 1.7 percent, the space agency noted. The orbits of asteroids bring them within 120 million miles of the sun. Most near-Earth objects (NEOs) are asteroids that range in size from about 10 feet to nearly 25 miles across. "The majority of near-Earth objects have orbits that don't bring them very close to Earth, and therefore pose no risk of impact," NASA says. A small portion of NEOs—known as potentially hazardous asteroids—do merit closer attention. PHAs, which are around 460 feet in diameter, have orbits that bring them as close as 4.6 million miles of the Earth's orbit around the sun, NASA notes. Despite the number of PHAs in our solar system, none is likely to hit our planet any time soon. "The 'potentially hazardous' designation simply means over many centuries and millennia the asteroid's orbit may evolve into one that has a chance of impacting Earth. We do not assess these long-term, many-century possibilities of impact," Paul Chodas, manager of the CNEOS, previously told Newsweek. Do you have a tip on a science story that Newsweek should be covering? Do you have a question about asteroids? Let us know via science@