Opportunity Occultations by Small Bodies - Split - CYC3HIGH

Details Opportunity Occultations by Small Bodies - Split - CYC3HIGH Opportunity Occultations by Small Bodies - Split - CYC3HIGH

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4944b&link_type=abstract

HST Proposal ID #4944

Mathematics

Logic

Hst Proposal Id #4944

Scientific paper

Although an occultation by any specific comet, asteroid, satellite, or Pluto is unlikely to be observable from the ST, the scientific return from such an event would be great because of the superior signal-to-noise ratio achievable with the ST for occultation observations. We propose to observe occultations by these bodies with the ST, as the opportunites arise, to probe their atmospheres, determine their sizes and achieve other goals. With such diverse possibilities, one must examine each opportunity as it occurs and formulate an observing strategy to fit that particular case. Revision History: Recvd on RPS 9/1/89;Added to SCCS 9/5/89; V2 prop instr - SALM; asb@MIT 5/7/90; Small logic errors fixed, BJW 7/9/90; Changed SP SCAN to SP SCAN SING-EXP, BJW 7/10/90; Target changes, ASB; Split by cycle, BJW 4/24/91; Updated targets, BJW 8/1/91; Updated targets, ASB 3/18/92; Cycle 2 changes, ASB 1/24/93 SPLIT FROM 4442 BEC. 2 TARGETS IN 4442 ALREADY EXECUTED;

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