Quantcast
Channel: Space station – Astro Bob
Viewing all articles
Browse latest Browse all 59

Jupiter’s Clouds Never Cease To Amaze

$
0
0
I loved playing with marbles as a kid but never imagined I’d see Jupiter as one. This global image was taken last September during orbit 22 and features numerous storm cells (called vortices) whirling about the planet’s northern hemisphere each about as wide as the continental U.S. NASA/JPL-Caltech/SwRI/MSSS with processing by Prateek Sarpal, © CC NC SA and the author

Seeing Jupiter and its cloud belts the other morning got me curious about what NASA’s Juno spacecraft has been up to. Juno swings around Jupiter every 53 days on a highly elongated orbit that reaches as far as 5 million miles (8.1 million km) from the planet to only 2,600 miles (4,200 km) above its cloud tops. The detailed images it captures during those close shaves will make your eyes pop.

Juno (white dot) spends only a brief time close to the planet because Jupiter’s radiation field is intense. The electronics are also heavily protected inside a titanium “vault” to further minimize risk. NASA

The spacecraft completed its 24th close flyby on Feb. 17 and will perform the next on April 10. My favorite way to track down recent and archival images taken by NASA space missions is through their photojournal sites. These come from the Juno Photojournal. I’m convinced if the painter Van Gogh were alive today he’d be captivated by Jupiter, a planet with a style similar to his own. The artist’s bright swirls of color imprinted with the strokes of his paintbrush mimic the wild vortices that crowd the planet’s polar regions.

Soft pastels enhance the rich colors of the swirls and storms in Jupiter’s clouds. This image of a vortex on Jupiter captures the amazing internal structure of the giant storm. NASA/JPL-Caltech/SwRI/MSSS / Image processing by Gerald Eichstädt/Seán Doran, © BY NC ND

Instead of using cadmium yellow and Prussian blue Jupiter mixes ammonia, methane, hydrogen, helium and dashes of sulfur and phosphorous to make its color palette. There are hundreds of vortices but they come in just two varieties: cyclones or low pressure centers and anticyclones or high pressure centers. And they’re whopping huge! Those near the planet’s north pole span 2,500 miles to 2,900 miles (4,000 to 4,600 kilometers) across with winds up to 220 miles an hour (350 kph). The biggest — from 3,500 to 4,300 miles (5,600 – 6,900 km) wide — jostle cheek to jowl around the south pole.

The two white ovals seen within the orange-colored band left of center are anticyclonic storms in the process of merging. The merger may be the result of the duo interacting with the larger oval (called OVAL BA) just to the north. Oval BA is the second largest anticyclonic vortex in Jupiter’s atmosphere, second only to the famous Great Red Spot. NASA/JPL-Caltech/SwRI/MSSS / Image processing by Tanya Oleksuik, © CC BY

The massive storms are caused by convection when warm, moist air rises up from deeper down in Jupiter’s atmosphere and condenses into clouds in the cold upper atmosphere, similar to how thunderstorms form on Earth. The planet’s rapid spin combined with powerful jet-stream-like winds coil the condensing gases into whirlpools. Jupiter’s spin also torques the mammoth cells and nudges them toward the poles where they accumulate in abundance.

This will give you an idea of the scale of the polar storms compared to the United States. NASA/JPL-Caltech/SwRI/MSSS

We’ve observed a variety of vortices practically since the invention of telescope but had no idea of their number and longevity (lifetimes range from several days to hundreds of years) until Juno was able to look over the top and bottom of the planet at its storm-rich polar regions. Juno also discovered water within the clouds along Jupiter’s equator, a finding that will help scientists better understand its meteorology.

The tiny bright white clouds are the highest, casting shadows on the next layer of clouds. Splashes of orange may be the color of the deepest clouds in this image, viewed through openings in the pastel layer. NASA/JPL-Caltech/SwRI/MSSS / Image processing by Kevin M. Gill, © CC BY

You can see Jupiter any morning at dawn now through a small telescope and marvel for yourself at its colorful and dynamic clouds. We share that with the solar system’s biggest planet. Althought the scale may be grander the underlying causes — heat, condensation, wind and rotation — are familiar to every earthling.


Viewing all articles
Browse latest Browse all 59

Trending Articles