Photometric seismology of Jupiter

Details Photometric seismology of Jupiter Photometric seismology of Jupiter

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..155g&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The recipe for a successful study of the Jovian interior structure is given by the association of seismology and precise visible photometry. In this framework, the micro-satellite project Jovis, presented to the French space agency (Mosser et al. 2004), is for Jupiter a copy of what the European space mission COROT is for the stars. The Jovian visible flux being dominated by the albedo map, an accurate analysis of the cloud response to a seismic wave has been done by Gaulme & Mosser (2005). When submitted to a plane wave of 0.5 m/s the cloud albedo fluctuates up to 70 ppm. We extend these results to the whole Jovian map and we estimate the visibility of the modes with the JOVIS micro-satellite.

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