Three Red Spots Mix It Up on Jupiter
This sequence of Hubble Space Telescope images offers an unprecedented view of a planetary game of Pac-Man among three red spots clustered together in Jupiter's atmosphere.
The time series shows the passage of the "Red Spot Jr." in a band of clouds below (south) of the Great Red Spot (GRS). "Red Spot Jr." first appeared on Jupiter in early 2006 when a previously white storm turned red. This is the second time, since turning red, it has skirted past its big brother apparently unscathed.
But this is not the fate of "baby red spot," which is in the same latitudinal band as the GRS. This new red spot first appeared earlier this year. The baby red spot gets ever closer to the GRS in this picture sequence until it is caught up in the anticyclonic spin of the GRS. In the final image the baby spot is deformed and pale in colour and has been spun to the right (east) of the GRS. (Amateur astronomers' observations confirm that this is the baby spot that migrated around the GRS.) The prediction is that the baby spot will now get pulled back into the GRS "Cuisinart" and disappear for good. This is one possible mechanism that has powered and sustained the GRS for at least 150 years.
These three natural-colour Jupiter images were made from data acquired on May 15, June 28, and July 8, 2008, by the Wide Field Planetary Camera 2 (WFPC2). Each one covers 58 degrees of Jovian latitude and 70 degrees of longitude (centred on 5 degrees South latitude and 110, 121, and 121 degrees West longitude, respectively).
Credit:NASA, ESA, A. Simon-Miller (Goddard Space Flight Center), N. Chanover (New Mexico State University), and G. Orton (Jet Propulsion Laboratory)
About the Image
About the Object
Name: | Jupiter, Red Spot |
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Type: | Solar System : Planet : Type : Gas Giant |
Category: | Solar System |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical B | 410 nm |
Hubble Space Telescope
WFPC2 |
Optical V | 502 nm |
Hubble Space Telescope
WFPC2 |
Optical R | 673 nm |
Hubble Space Telescope
WFPC2 |