This new image from the largest planet in the Solar System, Jupiter, was made during the Outer Planet Atmospheres Legacy (OPAL) programme. The images from this programme make it possible to determine the speeds of Jupiter’s winds, to identify different phenomena in its atmosphere and to track changes in its most famous features.

The map shown was observed on 19 January 2015, from 2:00 UT to 12:30 UT.

NASA, ESA, A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech)

Hubble Sees Changes in Jupiter’s Red Spot, a Weird Wisp and Rare Waves

Article Updated: 23 Dec , 2015

Jupiter global map created from still images from the Hubble Space Telescope

It’s been widely reported,  including at Universe Today, that the apple of Jupiter’s eye, the iconic Great Red Spot (GRS), has been shrinking for decades. Even the rate of shrinkage has been steadily increasing.

Back in the late 1800s you could squeeze three Earths inside the GRS. Those were the days. Last May it measured just 10,250 miles (16,496 km) across, big enough for only 1.3 of us. 

And while new photos from the Hubble Space Telescope show that Jupiter’s swollen red eye has shrunk an additional 150 miles (240 km) since 2014, the good news is that the rate of shrinkage appears to be well, shrinking. The contraction of the GRS has been studied closely since the 1930s; even as recently as 1979, the Voyager spacecraft measured it at 14,500 miles (23,335 km) across. But the alarm sounded in 2012, when amateur astronomers discovered sudden increase in the rate of 580 miles (933 km) a year along with a shift in shape from oval to roughly circular.

For the moment, it appears that the GRS is holding steady, making for an even more interesting Jupiter observing season than usual. Already, the big planet dominates the eastern sky along with Venus on October mornings. Consider looking for changes in the Spot yourself in the coming months. A 6-inch or larger scope and determination are all you need.

Hubble photos of the Great Red Spot taken at on a first rotation (left frames) and 10 hours later (right frames) show the counterclockwise rotation of the newly-discovered filament or wisp inside the GRS. Credit:

Hubble photos of the Great Red Spot taken on a first rotation (left frames) and 10 hours later (right frames) show the counterclockwise rotation of the newly-discovered filament or wisp inside the GRS. Credit: NASA, ESA, A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech)

New imagery from the Hubble OPAL program also shows a curious wisp at the center of the Great Red Spot spanning almost the entire width of the hurricane-like vortex. This filamentary streamer rotates and twists throughout the 10-hour span of the Great Red Spot image sequence, drawn out by winds that are blowing at 335 mph (540 km/hr). Color-wise, the GRS remains orange, not red. Currently, the reddest features on the planet are the North Equatorial Belt and the occasional dark, oval “barges” (cyclonic storms) in the northern hemisphere.

The newly-found waves in Jupiter's atmosphere are located in regions where cyclones are common. They look like dark eyelashes. Credit:

The newly-found waves in Jupiter’s atmosphere are located in regions where cyclones and anticyclones are common. They look like dark eyelashes. A cyclone is a storm or system of winds that rotates around an area of low pressure. Anticyclones spin around areas of high pressure. Credit: NASA, ESA, A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech)

That’s not all. The photos uncovered a rare wave structure just north of Jupiter’s equator that’s only been seen once before and with difficulty by the Voyager 2 spacecraft in 1979. The scientists, whose findings are described in this just-published Astrophysical Journal paper, say it resembles an earthly atmospheric feature called a baroclinic wave, a large-scale meandering of the jet stream associated with developing storms.

Hubble view of Jupiter's barocyclonic clouds and those recorded earlier by Voyager 2. Credit:

Hubble view of Jupiter’s baroclinic waves on January 19, 2015 (top) and our only other view of them photographed by Voyager 2 in 1979. Credit: NASA, ESA, A. Simon (GSFC), M. Wong (UC Berkeley), and G. Orton (JPL-Caltech)

Jupiter’s “current wave” riffles across a region rich with cyclonic and anticyclonic storms. The wave may originate in a clear layer beneath Jupiter’s clouds, only becoming visible when it propagates up into the cloud deck, according to the researchers. While it’s thought to be connected to storm formation in the Jovian atmosphere, it’s a mystery why the wave hasn’t been observed more often.

The OPAL program focuses on long-term observation of the atmospheres of Jupiter, Uranus and Neptune until the end of the Saturn Cassini Mission and all four planets afterwords. We have to keep watch from Earth as no missions to Saturn and beyond are expected for quite some time. To date, Neptune and Uranus have already been observed with photos to appear (hopefully) soon in a public archive.

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7 Responses

  1. N70SAK says:

    Will we ever learn to accept the reality of climate change? 😉

    • BlackWolfStanding says:

      Climate is changing all the time. Everybody agrees with that. What is in dispute is man’s involvement as the climate has drastically changed even before humans ever entered the industrial age. The climate change people can’t even determine what chemicals human produce to change the climate with.

  2. RUF says:

    Climate change comments should be removed from the comment section on an article that has nothing to do with climate change. This is an astronomy site, not a political site.

    • Bob King says:

      I agree, but am leaving the comment to stand. I would ask that other replies stick to the subject at hand — thanks everyone.

    • Bo Zo says:

      I’m sure you meant to say, it’s an astronomy site, not a climate science site. What’s political about climate change?

      But I agree that the comment was off topic and, whatever the poster’s intention may have been, it’s effectively grade A troll bait.

    • UFOsMOTHER says:

      RUF what has Climate Change got to do with politics Dah!

  3. Aqua4U says:

    I read in your link to baroclinic waves that they are mostly due to Coriolis forces and that here on Earth jet streams exhibit similar properties. I’ve oft wondered just how big a role the solar wind might play in the way upper tippy top of the atmosphere? Cloud waveforms or gravity waves, generated in the alto cirrus region seem to be effected by periods of high solar proton flux and speed? Also, when the sun flips it’s magnetic field the eq. jet stream(s) on Earth can change direction 180 degrees. (Depends on Sol’s field strength) I wonder how Sol effects Jupiter’s upper atmosphere? Go JUNO!

    Listen to the audio and then watch the video?

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