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Herschel
Space Observatory

An ESA Mission
with Participation from NASA

Nhsc2013-014a

Distribution of Water in Jupiter's Stratosphere

This map shows the distribution of water in the stratosphere of Jupiter as measured with the Herschel space observatory. White and cyan indicate highest concentration of water, and blue indicates lesser amounts. The map has been superimposed over an image of Jupiter taken at visible wavelengths with the NASA/ESA Hubble Space Telescope.

The distribution of water clearly shows an asymmetric distribution across the planet: water is more abundant in the southern hemisphere. Based on this and other clues collected with Herschel, astronomers have established that at least 95 percent of the water currently present in Jupiter's stratosphere was supplied by comet Shoemaker-Levy 9, which famously impacted the planet at intermediate southern latitudes in 1994.

The map is based on spectrometric data collected with the Photodetecting Array Camera and Spectrometer (PACS) instrument on board Herschel around 66.4 microns, a wavelength that corresponds to one of water's many spectral signatures.

Herschel is a European Space Agency mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, Calif. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA.

Image Details
Date
April 23, 2013
ID
nhsc2013-014a
Type
Observation
Credit
Water map: ESA/Herschel/T. Cavali et al.; Jupiter image: NASA/ESA/Reta Beebe (New Mexico State University)
Object Details
Name
Jupiter
Subject | Solar System
Planet Type Gas Giant
Color Mapping
Telescope Spectral Band Color Assigment Wavelength
Herschel (PACS) Infrared Blue 70.0 µm
Hubble Optical Grayscale 550.0 nm