See other posts from December 2009
Planetary Society Advent Calendar for December 7: Jupiter
Posted By Emily Lakdawalla
2009/12/07 03:11 CST
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Jupiter has been high overhead at sunset for several months, a brilliant light that's easy to spot even when the sky is still bright at dusk; but it's now moving quickly to the west as Earth speeds ahead of Jupiter's more stately march around the Sun. Although Jupiter's moons were discovered by Galileo, the banded and spotted appearance of the planet wasn't observed until Cassini pointed his more powerful telescope at the planet in the 1660s. Since then, it's been a fascinating target for professional and amateur observers; every night it appears different, since each of its dark belts and bright zones, and the bright and dark spots that twist on the boundaries between belts and zones, move with winds of slightly different speeds.

NASA / JPL / color mosaic by Björn Jónsson
Voyager 2 view of Jupiter
Here is a Voyager 2 view of Jupiter that hasn't been seen before. The original data consists of eighteen images, nine each captured through orange and violet filters by Voyager 2 as it approached the greatest planet on June 30, 1979. The white oval below and to the left of the Red Spot is Oval DE, one of three white spots at that latitude that later merged to become Oval BA, also known as "Red Junior."Jupiter mosaics are notoriously difficult to assemble because of the complicated motions of cloud features and the fast rotation of the planet. To produce this view, Jonsson reprojected each image in 3D space to align them, and had to do additional processing near the terminator to account for the way features rotated into daylight through the nearly half an hour that it took for Voyager 2 to acquire all 18 frames. To create a three-color composite from only two filters' worth of images, he calculated weighted averages of orange and violet images to create synthetic red, green, and blue channels. (Specifically: G=(0.71*O + 0.29*V) * 1.11285; color balance of O, G, V channels adjusted to make bright zones white; then R=1.1*O-0.1*V and B=0.25*G+0.75*V.)
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