IRS Moons and Planets, Cycle 4 extension

Details IRS Moons and Planets, Cycle 4 extension IRS Moons and Planets, Cycle 4 extension

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40842v&link_type=abstract

Spitzer Proposal ID #40842

Computer Science

Scientific paper

We are continuing our observations of the principal satellites of outer Solar System planets, using all SIRTF instruments. We use IRAC photometry to measure poorly known albedos of these cold objects at wavelengths between 3.5 and 8 microns, IRS will do reflectance spectrosopy at wavelengths between 5.3 and 15 µm, and thermal emission spectroscopy between 10 and 40 µm. Combined with MIPS photometry and SED measurements, these data willl provide compositional information, albedo, and thermal properties of these objects. When the observations in this proposal are combined with those already executed in Program 71, we will have observed synchronous satellites at both leading and trailing hemispheres. We also observe eclipse of Ganymede and Callisto.

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