Skip to main content

Citizen scientist shares stunning image of Jupiter’s atmosphere

We’re used to thinking of Jupiter as an orangey-brown sort of color, with its distinctive colored features like the Great Red Spot. But a recent image of Jupiter shared by NASA shows the planet in quite a different color palette, showing the planet’s clouds in two different formats. Firstly, there’s the planet as the human eye would see it, in Earthy, browny beige shades tinged with green. And secondly, there’s a saturated version that shows off the details of the cloud formations in vivid teals and greens.

The images were made from data taken by NASA’s Juno spacecraft, and they were processed by citizen scientist Björn Jónsson, an amateur image processor who shares his work with the public.

NASA’s Juno spacecraft observed the complex colors and structure of Jupiter’s clouds as it completed its 43rd close flyby of the giant planet on July 5, 2022. Citizen scientist Björn Jónsson created these two images using raw data from the JunoCam instrument aboard the spacecraft. At the time the raw image was taken, Juno was about 3,300 miles (5,300 kilometers) above Jupiter’s cloud tops, at a latitude of about 50 degrees. North is up. At that moment, the spacecraft was traveling at about 130,000 mph (209,000 kilometers per hour) relative to the planet.
NASA’s Juno spacecraft observed the complex colors and structure of Jupiter’s clouds as it completed its 43rd close flyby of the giant planet on July 5, 2022. Citizen scientist Björn Jónsson created these two images using raw data from the JunoCam instrument aboard the spacecraft. At the time the raw image was taken, Juno was about 3,300 miles (5,300 kilometers) above Jupiter’s cloud tops, at a latitude of about 50 degrees. North is up. At that moment, the spacecraft was traveling at about 130,000 mph (209,000 kilometers per hour) relative to the planet. Image data: NASA/JPL-Caltech/SwRI/MSSS Image processing by Björn Jónsson © CC NC SA

Turning observations from spacecraft or telescopes into an image is a detailed process requiring many particular decisions about color, contrast, and balance, which affect how the final image turns out and which features it emphasizes. It is possible to process an image to make it as close to what we would observe personally if we were to travel to the object, like the image of Jupiter on the left. But it’s also useful to make adjustments like turning up the saturation and contrast to help see features like cloud shapes in sharper detail, as you can see in the image of Jupiter on the right.

Recommended Videos

In the more saturated image, you can see features of Jupiter’s atmosphere like its deep swirling vortices, and the different colors can help to pick out different chemicals making up the atmosphere.

Please enable Javascript to view this content

The reason Jónsson was able to process these images is that all Juno data is made publicly available in its raw form on the mission’s website, and members of the public are encouraged to try their hands at processing the data for themselves. While you’re there, you can also see more of Jónsson’s stunning images, plus many other images processed by other citizen scientists.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
SpaceX shares stunning night shot of its Super Heavy booster
SpaceX's Super Heavy booster on the launchpad in Boca Chica, Texas.

SpaceX has released a breathtaking image (below left) of its Super Heavy booster, which has been moved to the launchpad ahead of the Starship’s fourth test flight. It shows the world’s most powerful launch vehicle on the pad at night, with a dramatic star-filled sky as the backdrop.

https://twitter.com/SpaceX/status/1775956032021495886

Read more
Stunning image shows the magnetic fields of our galaxy’s supermassive black hole
The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of our Milky Way black hole released in 2022, has captured a new view of the massive object at the center of our Galaxy: how it looks in polarized light. This is the first time astronomers have been able to measure polarization, a signature of magnetic fields, this close to the edge of Sagittarius A*. This image shows the polarized view of the Milky Way black hole. The lines mark the orientation of polarization, which is related to the magnetic field around the shadow of the black hole.

The Event Horizon Telescope collaboration, the group that took the historic first-ever image of a black hole, is back with a new stunning black hole image. This one shows the magnetic fields twirling around the supermassive black hole at the heart of our galaxy, Sagittarius A*.

Black holes are hard to image because they swallow anything that comes close to them, even light, due to their immensely powerful gravity. However, that doesn't mean they are invisible. The black hole itself can't be seen, but the swirling matter around the event horizon's edges glows brightly enough to be imaged. This new image takes advantage of a feature of light called polarization, revealing the powerful magnetic fields that twirl around the enormous black hole.

Read more
See the stunning Vela supernova remnant in exquisite detail in expansive image
This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the US National Science Foundation's Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, a Program of NSF’s NOIRLab. The striking reds, yellows, and blues in this image were achieved through the use of three DECam filters that each collect a specific color of light. Separate images were taken in each filter and then stacked on top of each other to produce this high-resolution image that contains 1.3 gigapixels and showcases the intricate web-like filaments snaking throughout the expanding cloud of gas.

A new image of the ghostly Vela supernova remnant shows off the fascinating and elaborate structure of this striking cosmic object. Taken using the Dark Energy Camera (DECam), this enormous image is 1.3 gigapixels, making it DECam's largest image to date.

This colorful web of wispy gas filaments is the Vela Supernova Remnant, an expanding nebula of cosmic debris left over from a massive star that exploded about 11,000 years ago. This image was taken with the Department of Energy-fabricated Dark Energy Camera (DECam), mounted on the U.S. National Science Foundation's Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile. CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab)

Read more