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Not all of Jupiter's clouds are huge, swirling, otherworldly beasts.

Spectacular new images captured by NASA's Jupiter-orbiting Juno spacecraft show fluffy-looking white clouds casting their comparably tiny shadows on the giant planet's monstrous, multicolored cloud decks.

The white clouds, which get up to 50 miles (80 kilometers) wide or so, are high up in Jupiter's atmosphere — so high that they're very cold, and the material they shed is therefore almost certainly frozen, Juno team members said.

"It's snowing on Jupiter, and we're seeing how it works," Juno principal investigator Scott Bolton, of the Southwest Research Institute in San Antonio, said during a news conference Thursday (May 25). [Related: New Mysteries at Jupiter]

Zoomed-in view of a photo taken by NASA’s Juno probe on May 19, 2017, showing clouds of water ice and/or ammonia ice high up in Jupiter’s atmosphere in the south tropical zone.
Zoomed-in view of a photo taken by NASA’s Juno probe on May 19, 2017, showing clouds of water ice and/or ammonia ice high up in Jupiter’s atmosphere in the south tropical zone.
Credit: NASA/SWRI/MSSS/Gerald Eichstädt/Seán Doran

"It's probably mostly ammonia ice, but there may be water ice mixed into it, so it's not exactly like the snow that we have [on Earth]," Bolton added. "And I was using my imagination when I said it was snowing there — it could be hail."

Small bright clouds of water ice and/or ammonia ice dot Jupiter’s entire south tropical zone in this image captured by NASA’s Juno spacecraft on May 19, 2017, at an altitude of 7,990 miles (12,858 kilometers). This is the first time so many cloud towers have been visible, possibly because the late-afternoon lighting is particularly good at this geometry.
Small bright clouds of water ice and/or ammonia ice dot Jupiter’s entire south tropical zone in this image captured by NASA’s Juno spacecraft on May 19, 2017, at an altitude of 7,990 miles (12,858 kilometers). This is the first time so many cloud towers have been visible, possibly because the late-afternoon lighting is particularly good at this geometry.
Credit: NASA/SWRI/MSSS/Gerald Eichstädt/Seán Doran

The $1.1 billion Juno mission launched in August 2011 and arrived in a highly elliptical orbit around Jupiter on July 4, 2016. The spacecraft's main mission involves characterizing the structure, composition, and gravitational and magnetic fields of Jupiter, to help scientists better understand how the giant planet formed and evolved.

An even closer view of the high-altitude Jupiter clouds spotted by NASA’s Juno spacecraft on May 19, 2017.
An even closer view of the high-altitude Jupiter clouds spotted by NASA’s Juno spacecraft on May 19, 2017.
Credit: NASA/SWRI/MSSS/Gerald Eichstädt/Seán Doran

Juno makes most of its measurements during close passes over Jupiter's poles that occur once every 53.5 Earth days. The probe has conducted five such data-collecting "perijove passes" so far, with the first occurring on Aug. 27, 2016.

The new photos were taken during the most recent close approach, which Juno completed on May 19.

This photo taken by NASA’s Juno spacecraft on May 19, 2017, at 5:50 UTC from an altitude of 5,500 miles (8,900 kilometers) shows high-flying white clouds composed of water ice and/or ammonia ice. In some areas, these clouds appear to form “squall lines” — narrow bands of high winds and storms associated with a cold front.
This photo taken by NASA’s Juno spacecraft on May 19, 2017, at 5:50 UTC from an altitude of 5,500 miles (8,900 kilometers) shows high-flying white clouds composed of water ice and/or ammonia ice. In some areas, these clouds appear to form “squall lines” — narrow bands of high winds and storms associated with a cold front.
Credit: NASA/SWRI/MSSS/Gerald Eichstädt/Seán Doran

Thursday's news conference focused mainly on the science results that the Juno team has been able to glean from the first few perijove passes. For example, Bolton and his colleagues discussed the surprising cyclones that Juno spotted near Jupiter's poles, the mysterious processes driving Jovian auroras and hints that the gas giant may have a large and "fuzzy," or partially dissolved, core, among other topics.

Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.