Title Mapping the surfaces of large icy bodies Pi B. Butler Time 104 hrs Title: Mapping the surfaces of large icy bodies Authors: B. Butler Abstract: ALMA will be able to map with unprecedented accuracy and fidelity the millimeter wavelength emission from the solid surfaces of the larger icy bodies in the solar system, including jovian, saturnian, uranian and neptunian satellites, Pluto & Charon, and the larger of the TNOs. Such maps will provide us with information on the thermal and electrical properties of the surface and near-surface, as well as the surface texture - which may hold clues to composition - see, e.g., Muhleman & Berge 1991; Jewitt 1994; Lellouch et al. 2000. contin line poln name RA&DEC m T SD CA sub resn size freq line dfreq BW fd rms fd rms fd rms time ------------ -------- - - -- -- --- ---- ---- ---- ------ -------- ----- ------------ ----------- --------- ------ icy sat/TNO ecliptic Y Y N N N .1 .1-1 345 N/A N/A 8 GHz 50-100 K 1 K N/A 1 K .1 K 40x2 h Pluto/Charon ecliptic Y Y N N N .01 .1 345 N/A N/A 8 GHz 40 K 1 K N/A 1 K .1 K 4x6 h total 104 h ************************************************************************** See program 4.1.1 for general comments Butler and Gurwell Review Mark Gurwell: OK. -------------------------------------------------- Review v2.0: Review of 4.2.1-4.2.8 (no DRSP 2.0 updates received) These projects still remain scientifically valid. Do the additional ALMA bands offer something new (e.g., for projects 4.2.4, 4.2.5)? The integration times are probably still ok eventhough the number of antennas has gone from 64 to 50 - or at least close enough. Several of these projects focus on objects larger than the ALMA primary beam, and mosaicing is needed. Here the ACA and also the ACA in crosscorrelation with the ALMA-12m antennas may be beneficial.