Latest news with #ChrisMoeckel
Yahoo
24-05-2025
- Science
- Yahoo
Bizarre softball-sized 'mushballs' explain missing gas on Jupiter
When you buy through links on our articles, Future and its syndication partners may earn a commission. The weather forecast for Jupiter now includes softball-size hailstones, known as "mushballs," that are brewed by violent thunderstorms raging in the planet's turbulent atmosphere, a new study finds. The findings confirm these bizarre, ammonia-rich mushballs are also the source of Jupiter's missing ammonia. The absence of this gas in pockets of Jupiter's atmosphere has perplexed scientists for years. Decades ago, astronomers spotted intensely turbulent cloud tops in telescope images of the gas giant. The discovery led scientists to conclude that Jupiter's atmosphere churns and mixes constantly, like a pot of boiling water. Yet recent data from Earth-based radio telescopes and NASA's Juno spacecraft revealed deep pockets of missing ammonia — reaching 90 miles (150 kilometers) deep across all latitudes. This depletion is so significant in the planet's atmosphere that no known mechanism could explain it. Now, the new study's analysis of the aftermath of a massive 2017 storm observed by Juno offers compelling evidence that Jupiter's raging storms are the key to this atmospheric puzzle. The findings also reveal that even localized storms can strip ammonia from the planet's upper atmosphere and plunge it unexpectedly deep, indicating that the long-held vision of a thoroughly mixed atmosphere swirling around Jupiter is an illusion. "The top of the atmosphere is actually a pretty poor representation of what the whole planet looks like," study lead author Chris Moeckel, a researcher in the Space Sciences Laboratory at the University of California, Berkeley, told Live Science. "As time goes by, we have to dig deeper and deeper into the atmosphere to find the place where it appears well-mixed." Moeckel and his colleagues described their findings in a study published March 28 in the journal Science Advances. Because of the dense cloud cover blanketing Jupiter, scientists cannot directly observe what lies beneath the planet's turbulent cloud tops. The role of ammonia is like a splash of color in a flowing stream of water, Moeckel said: It acts as a tracer, revealing otherwise-invisible patterns and processes deep within Jupiter's atmosphere. To explain the missing ammonia in Jupiter's atmosphere, in 2020 scientists theorized that the planet's violent storms generate strong updrafts that rapidly lift ammonia-rich ice particles to high altitudes, where they combine with water ice into a slushy liquid. Much like Earth's hailstones, Jovian mushballs grow by accumulating ice layers as storm currents repeatedly cycle them, eventually reaching softball size and falling deep into Jupiter's atmosphere, far below their origin. This process, the theory posited, left upper regions depleted of ammonia and water that Juno and ground-based telescopes detected. A distinct signature within the radio observations beamed back by Juno confirmed that this exotic process is indeed occurring, the new study found. During its February 2017 flyby, the spacecraft passed over an active storm region, and its instruments showed a higher concentration of both ammonia and water nestled beneath the storm cloud. "I was actually sitting at the dentist's office waiting and I was playing with the code," Moeckel said. "All of a sudden I saw a signal much deeper at the same location as the storm clouds were at the top, and I remember being like 'Huh,' I didn't expect anything down here." The peculiar signal, which persisted even a month after the storm began, could only be explained by either a drop in temperature consistent with melting ice or an increase in ammonia concentration, which would occur if the ammonia within the mushballs was being released as they melted. RELATED STORIES —Powerful solar winds squish Jupiter's magnetic field 'like a giant squash ball' —NASA solves 44-year-old mystery of why Jupiter's Io is so volcanically active —Jupiter's Great Red Spot is being squeezed, Hubble Telescope finds — and nobody knows why "Both theories led me to the same conclusion — the only known mechanism was these mushballs," Moeckel said. "That's the moment I conceded." The researchers suspect Jupiter is unlikely to be unique in this regard, as gases such as ammonia are swept into forming planets and are likely circulating in the atmospheres of hydrated gas giants both within our solar system and beyond. "I won't be surprised if this is happening throughout the universe," Moeckel said.
Yahoo
04-04-2025
- Science
- Yahoo
Major storms on Jupiter can leave a fingerprint in the planet's atmosphere
When you buy through links on our articles, Future and its syndication partners may earn a commission. It would appear that a really big storm on Jupiter can leave a noticeable mark in the planet's atmosphere. A recent study tapped into data collected by the Jupiter-orbiting spacecraft Juno and the Hubble Space Telescope to start piecing together how this gas giant's storms churn up the world's atmosphere — even surprisingly far below the clouds. This churning involves the storms dredging up ammonia in some places and hurling it far into the Jovian depths as slushy hailstones in others. The result, it appears, is that patches of ammonia gas end up buried deep in some parts of Jupiter's lower atmosphere, while other areas have far less ammonia than they normally would. In other words, some storms on Jupiter can leave behind a fingerprint, reworking the whole chemical makeup of the planet's atmosphere. A huge storm on Jupiter broke out in December of 2016, just south of the planet's equator and about 60 degrees east of the famous Great Red Spot. Amateur astronomer Phil Miles was the first to spot this storm in February of 2017 — and the timing couldn't have been better. Juno was about to make its fourth close flyby of Jupiter, and the Atacama Large Millimeter/submillimeter Array here on Earth, along with the Hubble Space Telescope in orbit, were also pointed at the gas giant. This meant astronomers could see Jupiter in different wavelengths of light at the same time. Armed with data from three observatories, University of California, Berkeley, planetary scientist Chris Moeckel and his colleagues just needed to figure out what kinds of updrafts, downdrafts and heat transfer could best explain what Juno, Hubble and ALMA saw during and after the storm. The team simulated the inner workings of Jupiter's atmosphere, which revealed that the massive storm had stirred up the planet's atmosphere dozens of miles below even the lowest-hanging cloud decks. To understand exactly what that means, we first need to understand one of the quirks of describing the weather on Jupiter. It's hard to measure altitudes in Jupiter's atmosphere, because the planet doesn't have a surface in the usual sense (there's liquid somewhere below all those deep layers of gas, but it's never been directly measured), so scientists rely on pressure instead. There's a level in Jupiter's middle stratosphere at which the atmospheric pressure is about the same as it is at sea level here on Earth, and that makes a useful baseline for saying how deep things are in Jupiter's atmosphere. The dense, heavy water vapor clouds where huge Jovian storms begin are about 82 miles (132 kilometers) below that level, where the air pressure is about 10 times higher than it is at sea level on Earth. Furthermore, Juno's data suggests the lowest-hanging clouds present during the early 2017 storm loomed several miles lower than even that level — thus, in the storm's wake, the atmosphere had been stirred up deep, deep below the clouds. Juno and Hubble images from 2017 showed a powerful updraft near the heart of the storm, pumping ammonia from deep within Jupiter's atmosphere and rushing it upward to the peaks of the towering storm clouds. Below that plume, Juno and Hubble saw that the updraft had "dried out" most of the ammonia from a patch of Jupiter's atmosphere stretching down at least tens of miles below the base of the storm clouds. Wrapped around the bright spot of the updraft, darker patches shown in Juno's data mark where downdrafts carried a slushy mix of ammonia and water back down to the Jovian depths. And surprisingly, the ammonia was plunging much deeper into the atmosphere than Moeckel and his colleagues expected. If the clouds in the early 2017 storm had just been raining big liquid droplets of ammonia, they shouldn't have been able to fall very deep into the atmosphere before the higher temperature and pressure evaporated the droplets — and the resulting gas wouldn't keep falling. It would just hang out, forming a new ammonia gas layer. But instead, the ammonia fell deeper — according to Moeckel and his colleagues' simulations, down to a depth where the pressure in Jupiter's atmosphere is about 30 times higher than that at sea level on Earth. That means the storm was most likely dropping down big, slushy mush balls of mixed water and ammonia. Mush balls are a weird weather phenomenon on Jupiter that astronomers first pieced together (also from Juno data) a few years ago. Related Stories: — NASA's Juno probe sees active volcanic eruptions on Jupiter's volcanic moon Io (images) — NASA's Juno probe spots massive new volcano on Jupiter moon Io — Jupiter's volcanic moon Io may spew sulfur to icy neighbor Europa's surface Ammonia stays liquid at much lower temperatures than water can, which means droplets of liquid ammonia can mingle with icy crystals of water in Jupiter's storm clouds. The resulting mix is a ball of slush just solid enough to stay together, but definitely mushier than, say, a hailstone; picture a wet snowball. And mush balls raining out of a storm could fall much faster than raindrops, so they'd make it much farther before succumbing to evaporation. The result is that deep within Jupiter's atmosphere, there are patches of ammonia that fell as mush balls from storms raging dozens of miles above – and that ammonia will stay buried down there until the next big storm dredges it up. The scientists published their work on March 28 in the journal Science Advances.
