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Jupiter's Great Red Spot is smaller than ever seen before

Date:
May 15, 2014
Source:
Space Telescope Science Institute (STScI)
Summary:
Recent Hubble observations confirm that Jupiter's Great Red Spot, a swirling storm feature larger than Earth, has shrunken to the smallest size astronomers have ever measured. Jupiter's Great Red Spot is a churning anticyclonic storm.

Jupiter's monster storm, the Great Red Spot, was once so large that three Earths would fit inside it. But new measurements by NASA's Hubble Space Telescope reveal that the largest storm in our solar system has downsized significantly. The Great Red Spot, which has been raging for at least a hundred years, is only the width of one Earth. What is happening? One possibility is that some unknown activity in the planet's atmosphere may be draining energy and weakening the storm, causing it to shrink. The Hubble images were taken in 1995, 2009, and 2014.
Credit: mage: NASA, ESA, and A. Simon (GSFC);Science: A. Simon (GSFC), G. Orton (JPL), J. Rogers (Univ. of Cambridge, UK), and M. Wong and I. de Pater (Univ. of California, Berkeley);Acknowledgment: C. Go, H. Hammel (SSI, Boulder, and AURA), and R. Beebe (NMSU)

Jupiter's trademark Great Red Spot -- a swirling anticyclonic storm feature larger than Earth -- has shrunken to the smallest size ever measured. Astronomers have followed this downsizing since the 1930s. Jupiter's Great Red Spot is a churning anticyclonic storm.

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"Recent Hubble Space Telescope observations confirm that the Great Red Spot (GRS) is now approximately 10,250 miles across, the smallest diameter we've ever measured," said Amy Simon of NASA's Goddard Space Flight Center in Greenbelt, Maryland. Historic observations as far back as the late 1800s gauged the GRS to be as big as 25,500 miles on its long axis. The NASA Voyager 1 and Voyager 2 flybys of Jupiter in 1979 measured the GRS to be 14,500 miles across.

Starting in 2012, amateur observations revealed a noticeable increase in the spot's shrinkage rate. The GRS's "waistline" is getting smaller by 580 miles per year. The shape of the GRS has changed from an oval to a circle. The cause behind the shrinking has yet to be explained.

"In our new observations it is apparent that very small eddies are feeding into the storm," said Simon. "We hypothesized that these may be responsible for the sudden change by altering the internal dynamics and energy of the Great Red Spot."

Simon's team plans to study the motions of the small eddies and also the internal dynamics of the GRS to determine if these eddies can feed or sap momentum entering the upwelling vortex.

In the comparison images on the right, the Hubble photo at top was taken in 1995, when the long axis of the GRS was estimated to be 13,020 miles across. In the 2009 photo the GRS was measured at 11,130 miles across.

The full disk image of Jupiter on the left was taken on April 21, 2014, with Hubble's Wide Field Camera 3.


Story Source:

The above story is based on materials provided by Space Telescope Science Institute (STScI). Note: Materials may be edited for content and length.


Cite This Page:

Space Telescope Science Institute (STScI). "Jupiter's Great Red Spot is smaller than ever seen before." ScienceDaily. ScienceDaily, 15 May 2014. <www.sciencedaily.com/releases/2014/05/140515103658.htm>.
Space Telescope Science Institute (STScI). (2014, May 15). Jupiter's Great Red Spot is smaller than ever seen before. ScienceDaily. Retrieved January 27, 2015 from www.sciencedaily.com/releases/2014/05/140515103658.htm
Space Telescope Science Institute (STScI). "Jupiter's Great Red Spot is smaller than ever seen before." ScienceDaily. www.sciencedaily.com/releases/2014/05/140515103658.htm (accessed January 27, 2015).

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