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File:PIA01598 Hubble Views Ancient Storm in the Atmosphere of Jupiter.jpg

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PIA01598_Hubble_Views_Ancient_Storm_in_the_Atmosphere_of_Jupiter.jpg (321 × 321 pixels, file size: 70 KB, MIME type: image/jpeg)

Summary

Description
English: When 17th-century astronomers first turned their telescopes to Jupiter, they noted a conspicuous reddish spot on the giant planet. This Great Red Spot is still present in Jupiter's atmosphere, more than 300 years later. It is now known that it is a vast storm, spinning like a cyclone. Unlike a low-pressure hurricane in the Caribbean Sea, however, the Red Spot rotates in a counterclockwise direction in the southern hemisphere, showing that it is a high-pressure system. Winds inside this Jovian storm reach speeds of about 270 mph.

The Red Spot is the largest known storm in the Solar System. With a diameter of 15,400 miles, it is almost twice the size of the entire Earth and one-sixth the diameter of Jupiter itself.

The long lifetime of the Red Spot may be due to the fact that Jupiter is mainly a gaseous planet. It possibly has liquid layers, but lacks a solid surface, which would dissipate the storm's energy, much as happens when a hurricane makes landfall on the Earth. However, the Red Spot does change its shape, size, and color, sometimes dramatically. Such changes are demonstrated in high-resolution Wide Field and Planetary Cameras 1 & 2 images of Jupiter obtained by NASA's Hubble Space Telescope between 1992 and 1999 (PIA01594 thru PIA01599 and PIA02400 thru PIA02402). This image was obtained in February 1995.

A montage representing the entire series of images was prepared by the Hubble Heritage Project team and is available at PIA01593.

Astronomers study weather phenomena on other planets in order to gain a greater understanding of our own Earth's climate. Lacking a solid surface, Jupiter provides us with a laboratory experiment for observing weather phenomena under very different conditions than those prevailing on Earth. This knowledge can also be applied to places in the Earth's atmosphere that are over deep oceans, making them more similar to Jupiter's deep atmosphere.
Date
Source http://photojournal.jpl.nasa.gov/catalog/PIA01598 (direct link)
Author Amy Simon (Cornell U.), Reta Beebe (NMSU), Heidi Hammel (Space Science Institute, MIT)

Licensing

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:
Public domain
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.


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24 August 1999

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Date/TimeThumbnailDimensionsUserComment
current07:00, 1 January 2016Thumbnail for version as of 07:00, 1 January 2016321 × 321 (70 KB)PlanetUsercompressed
09:20, 17 April 2015Thumbnail for version as of 09:20, 17 April 2015321 × 321 (10 KB)Jcpag2012exactly the same as existing file (10 KB)
23:49, 12 May 2008Thumbnail for version as of 23:49, 12 May 2008321 × 321 (10 KB)File Upload Bot (Magnus Manske) {{BotMoveToCommons|nl.wikipedia}} {{Information |Description={{nl|Ancient Storm in the Atmosphere of Jupiter}} |Source=Transferred from [http://nl.wikipedia.org nl.wikipedia]<br/> (Original text : ''[http://photojournal.jpl.nasa.gov/catalog/PIA01598 NASA
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