Iapetus's SED from 3-11 mm

Details Iapetus's SED from 3-11 mm Iapetus's SED from 3-11 mm

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..654r&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.654

Physics

Scientific paper

Several observations were made of Saturn's moon Iapetus using the NRAO Green Bank Telescope (GBT) using the MUSTANGW-band (3.3mm) bolomoter and the Ka-band (7.5-11mm) CCB instrument in order to constrain its spectral energy distribution (SED). Observations show a severe decrement in brightness temperature at some wavelengths, but the location of the decrement shifts depending on the sub-observer longitude.

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