Mars Orbiter Captures Rare View of Ancient Volcano Poking Above the Clouds
Floating in orbit above Mars, NASA's 2001 Mars Odyssey orbiter captured a panorama of the Red Planet's biggest volcanoes, Arsia Mons, peeking over a sea of clouds. The picturesque moment offers an exceptionally rare view of a Martian volcano, showing the landform at an angle in space that captures the planet's horizon.
'We picked Arsia Mons hoping we would see the summit poke above the early morning clouds. And it didn't disappoint,' Jonathon Hill, the operations lead for Odyssey's camera and a mission planner at Arizona State University's Mars Space Flight Facility, called the Thermal Emission Imaging System, or THEMIS, said in a statement. THEMIS can view Mars in both visible and infrared light.
Launched in 2001, Odyssey has been circling around Mars for over two decades, studying the Martian surface. But in 2023, the orbiter began taking breathtaking panoramic views of the Martian horizon. Because THEMIS can't pivot to get these stunning views, the orbiter flips on its side, rotating a full 90 degrees. That way, it captured Mars' 'limb,' the edge of the planet's horizon. This is THEMIS' fourth limb observation since 2023.
Odyssey captured the image on May 2, just before dawn. In it, Arsia Mons stands 12 miles (20 kilometers) high and measures 70 miles (450 km) in diameter. For comparison, Earth's tallest volcano, Mauna Loa, stands 6 miles (9 km) above the seafloor and measures 75 miles (121 km) in diameter.
Arsia Mons is also one of Mars' cloudiest volcanoes and the southernmost of the three Tharsis volcanoes that form Tharsis Montes, or Tharsis Mountains. These mountains are often surrounded by water ice clouds, particularly early in the morning. The clouds form when air expands as it blows up the sides of the mountain and then rapidly cools.
This view also allows scientists to study Martian weather and phenomena like dust clouds and how they change over the course of the seasons. Odyssey might be able to capture a few more of these panoramas before its eventual retirement, likely at the end of this year.
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'I should know my data better, after years of working with it.' The existence of the Oort Cloud was first proposed in 1950 by Dutch astronomer Jan Oort, who imagined it as a shell of icy bodies swirling around the sun from up to 1.5 light-years away. The cloud is the most distant region in our solar system, stretching as much as halfway to the next star, according to NASA. It's composed of leftovers from the making of our solar system, which were scattered in every direction by the planets after they formed. That means many of the icy bodies in the Oort Cloud don't share the same orbital plane as the solar system itself but travel at various inclinations, which is why the Oort Cloud is pictured as a sphere. If one of those icy bodies gets flung inward toward the sun, the heat starts vaporizing some of the material in the body, creating a tail — and what we call a comet. 'Every now and again, some of these icy bodies come into the inner solar system, and we can see the orbit that they're on,' Faherty said. 'And they're on these really crazy, long orbits. It can take them millions of years to go around the sun. And when they come in, they help us understand how far away they may have come from.' The problem with trying to imagine what the Oort Cloud looks like is that scientists have never seen it, even though we are technically surrounded by it. That's because the bodies that make it up are small — fewer than 60 miles (97 kilometers) in diameter — and even though they potentially number in the trillions, they are far away, making observations with telescopes difficult. The spiral was hiding in Nesvorny's data because he had never thought of visualizing it three-dimensionally. 'I never looked at it in Cartesian coordinates — I didn't have a good reason to do so,' he said. 'But once you do that, it's obvious. It's there.' To confirm the findings, Nesvorny used one of the most powerful computers in the world, NASA's Pleiades Supercomputer, to run simulations that took weeks to complete. 'I thought, maybe just this particular simulation (I gave the planetarium) is showing it, and all the other simulations with other stellar encounters, other parameters, will not show it, in which case it wouldn't be so interesting,' he said. 'But all the simulations, all the models I have, show the spiral.' The reason it's there, he said, is that objects in the Oort Cloud are far away enough from the sun's gravity that they also start being affected by the galactic tide — the gravitational field of our galaxy, exerted by the stars and the dark matter in it. This field is acting on the small bodies and comets in the Oort Cloud by twisting their orbital planes to create a spiral. The spiral, Nesvorny added, is in the inner part of the Oort Cloud, the closest to us, and he still believes that the outer portion is spherical or shell-shaped. The problem of observing the Oort Cloud remains, even though the Vera C. Rubin Observatory, a powerful telescope that recently came online in Chile, could offer a hand by discovering and observing individual icy bodies in the cloud. However, according to Nesvorny, the telescope will likely discover dozens of these bodies — not the hundreds that would be required to produce a meaningful visualization of the spiral. The spiral theory helps to illuminate the dynamics of our solar system, according to Faherty. 'If you're going to come up with a theory of how solar systems evolve, you should take into account the kind of shapes you might have in their structure,' she said. 'Maybe comets helped deliver water to Earth. Maybe the building blocks of life could be out there in the Oort Cloud, so if you want to talk about the potential building blocks of life that surround our solar system, you need to understand its shape.' It's a 'dream,' she added, to be able to present science so recent in a show aimed at the general public. 'I truly believe that the planetarium, the dome itself, is a research tool,' Faherty said. 'I like to say that this is science that hasn't had time to reach your textbook yet.' The spiral finding is a wonderful example of just how much we can learn through visualizing the universe in new ways, said Malena Rice, an assistant professor of astronomy at Yale University who did not participate in the study. 'This result reshapes our mental image of our home solar system, while also providing a new sense for what extrasolar systems' Oort clouds may look like,' Rice added. 'It unites our models of the solar system with what we know about the broader galaxy, placing it into context as a dynamic system. We are not static, and we are not isolated — our solar system is shaped by its broader ecosystem, and the Oort spiral exemplifies that.' While the paper is interesting, it is almost entirely theoretical, as it is based on numerical simulations of the interactions between the sun's gravity and the gravitational pull of the rest of the Milky Way galaxy's motion, said Edward Gomez, an astrophysicist and honorary lecturer at Cardiff University in the UK. He also was not involved with the study. 'Long period comets enter the inner solar system at a range of angles, which the authors try to model using their spiral arm idea,' Gomez said in an email. 'What they are proposing could be true, but it could also be modelled by other shapes of the Oort cloud or physical processes. How to test this is their major issue, because only a handful of potential Oort cloud objects are known about.' Confirming the findings will be a challenge, noted Simon Portegies Zwart, a professor of numerical star dynamics at Leiden University in the Netherlands who was not part of the team behind the research. 'It is interesting that they found the spiral, (but) it seems unlikely that we are going to witness (it) in the foreseeable future,' he said. With luck, he added, the Vera Rubin observatory will detect a few hundred inner Oort Cloud objects, but the spiral would only be visible if many more are found: 'It therefore seems unlikely to be a clearly detectable structure.'
