Astronomers have finally found direct proof that almost all water present in Jupiter’s stratosphere, an intermediate atmospheric layer, was delivered by comet Shoemaker-Levy 9, which famously struck the planet in 1994.
The findings, based on new data from the Herschel Space Observatory, reveal more water in Jupiter’s southern hemisphere, where the impacts occurred, than in the north. Herschel is a European Space Agency mission with important NASA participation.
The origin of water in the upper atmospheres of the solar system’s giant planets has been debated for almost two decades. Astronomers were quite surprised at the discovery of water in the stratospheres of Jupiter, Saturn, Uranus, and Neptune, which dates to observations performed with ESA’s Infrared Space Observatory in 1997.
While the source of water in the lower layers of their atmospheres can be explained as internal, the presence of this molecule in their upper atmospheric layers is puzzling due to the scarcity of oxygen there. Its supply must have an external origin. Since then, astronomers have investigated several possible candidates that may have delivered water to these planets, from icy rings and satellites to interplanetary dust particles and cometary impacts.
Data from Herschel’s Photodetecting Array Camera and Spectrometer (PACS), with the help of NASA’s Infrared Telescope Facility, helped solve the mystery at Jupiter by showing an asymmetry in the distribution of water in its stratosphere, caused by the comet impact. Additional proof for a cometary source for the water came from Hershel’s Heterodyne Instrument for the Far-Infrared (HIFI), which probed the vertical profile of water in the stratosphere. NASA’s Jet Propulsion Laboratory in Pasadena, Calif., helped build the HIFI instrument.
“The asymmetry between the two hemispheres suggests that water was delivered during a single event and rules out icy rings or moons as candidate sources,” says Thibault Cavalié from the Laboratoire d’Astrophysique de Bordeaux, France, who led the study. “Local sources would provide a steady supply of water, which over time would lead to a hemispherically symmetric distribution in the stratosphere. Depending on whether the chemical species are transported in neutral or ionized form, local sources of water would result in higher concentrations either at the poles or along the equator, but not in a north-south asymmetry.”
Read the full ESA news release here: http://www.esa.int/Our_Activities/Space_Science/Herschel/Herschel_links_Jupiter_s_water_to_comet_impact .
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 JPL. 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.
This article was written by NASA’s Whitney Clavin and originally appeared on NASA’s website, which can be viewed by clicking here: Jupiter
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