! $Id: 5662,v 8.1 1994/07/27 20:11:31 pepsa Exp $ coverpage: title_1: CYCLE 4 DD HST OBSERVATIONS OF COMET SHOEMAKER-LEVY (1993E) title_2: FOR JULY 1994 sci_cat: SOLAR SYSTEM sci_subcat: COMETS proposal_for: GO/DD pi_fname: HAROLD pi_mi: A. pi_lname: WEAVER pi_inst: STSCI pi_country: USA hours_pri: 13 num_pri: 1 wf_pc: Y fos: Y realtime: N time_crit: Y funds_length: 12 off_fname: HERVEY off_mi: S. off_lname: STOCKMAN off_title: DEPUTY DIRECTOR off_inst: 3470 off_addr_1: SPACE TELESCOPE SCIENCE INSTITUTE off_addr_2: 3700 SAN MARTIN DRIVE off_city: BALTIMORE off_state: MD off_zip: 21218 off_country: USA abstract: LINE_1: Comet Shoemaker-Levy (1993e) is a comet that has recently broken LINE_2: up into many fragments, apparently somewhere in the vicinity LINE_3: of Jupiter. Ground-based observations reveal a string of sub-nuclei LINE_4: spaced over a distance of about one arcminute. HST observations LINE_5: of this object with the WFPC-2 should reveal a fascinating spatial LINE_6: morphology that is more detailed than any images obtained from LINE_7: ground-based telescopes. Most importantly, WFPC-2 images of 1993e LINE_8: should allow us to refine the nuclear size estimates that were LINE_9: originally estimated from WFPC-1 HST observations in July 1993. LINE_10: This proposal is for the July 1994 observations. general_form_proposers: lname: WEAVER fname: HAROLD title: PI mi: A. inst: STSCI country: USA general_form_address: lname: Weaver fname: Harold Title: Dr. MI: A Category: PI Inst: 3470 addr_1: 3700 San Martin Drive city: Baltimore state: MD zip: 21218 country: USA phone: 410-338-5004 GENERAL_FORM_TEXT: QUESTION:3 SECTION: 1 line_1: The program consists of ten separate visits to the comet with line_2: all but one being devoted to imaging with the WFPC-2. One visit line_3: is devoted to FOS spectroscopy near fragment 15 (G). line_4: For the observations during the impact week, we have used line_5: AT special requirements with UTC times for the orbits that line_6: we hope to use. These latter choices were made AFTER consultation line_7: with the latest version of the timeline for the 199 sms. These line_8: ATs can be RELAXED by one or two orbits if necessary. Please line_9: consult with me before making any larger changes. QUESTION:3 SECTION: 2 QUESTION: 4 SECTION: 1 line_1: HST observations of Comet Shoemaker-Levy (1993e) should provide line_2: better detail on the break-up of this object than is available line_3: from any other source. QUESTION: 4 SECTION: 2 QUESTION: 4 SECTION: 3 QUESTION: 5 SECTION: 1 QUESTION: 8 SECTION: 1 QUESTION: 9 SECTION: 1 line_1:ID no. 3064: HST Observations of Comet Levy (1990c) line_2:(A'Hearn, Arpigny, and Feldman are Co-Is), an imaging-only line_3:program that is only peripherally related to the line_4:current program. line_5: line_6:ID no. 2481: HST Observations of Periodic Comets (A'Hearn, Arpigny, line_7:and Feldman are Co-Is), only peripherally related to this program. line_8: line_9:ID no. 2483: The Volatile Composition of New Comets (A'Hearn, Arpigny, line_10:and Feldman are Co-Is), only peripherally related to this program. line_11: line_12:ID no. 2442: Cometary Parent Molecules, P.D. Feldman, PI (A'Hearn line_13:and Weaver are Co-Is), only peripherally related to this program. line_14: line_15:Cycle 2 program: line_16:ID no. 3707: HST Observations of Periodic Comets (A'Hearn, Arpigny, line_17:and Feldman are Co-Is), only peripherally related to this program. QUESTION: 9 SECTION: 2 line_1:ID no. 3064: Two sets of WFC images of comet Levy were obtained 6.5 line_2:hours apart on 27 September 1990 in order to investigate its temporal line_3:variability. An arc of large grains was observed propagating line_4:sunward with a projected velocity of 0.16 km/sec. line_5: line_6:ID no. 2481: P/Hartley 2 was successfully observed in late 9/91 line_7:These observations produced the first detection of CO Cameron bands in line_8:comets. This emission is essentially a unique tracer of the CO2 line_9:abundance in comets. Additionally we obtained a beautiful spectrum line_10:of the comet covering the entire spectral range 1200-6800 A, from line_11:which we are compiling (still in progress) an inventory of volatiles line_12:in that comet. line_13: line_14:ID no. 2483: Comet Shoemaker-Levy (1991a1) was successfully observed line_15:in July 1992. Unfortunately, the comet was not as bright as we had line_16:hoped, but we obtained data of comparable (slightly higher) quality line_17:to that already in hand from P/Hartley 2. We definitely detected line_18:the CO Cameron bands again, but it is much too early to say anything line_19:more at this time. line_20: line_21:ID no. 2442: Comet Shoemaker-Levy (1991a1) was successfully observed line_22:in July 1992, but it is too early to say anything more at this time. QUESTION: 9 SECTION: 3 line_1:ID no. 3064: Inner Coma Imaging of Comet Levy (1990c) with the Hubble line_2:Space Telescope, H. A. Weaver, M. F. A'Hearn, P. D. Feldman, line_3:C. Arpigny, W. A. Baum, J. C. Brandt, R. M. Light and line_4:J. A. Westphal,Icarus}, v. 97, p. 85, 1992. line_5: line_6:ID no. 2481: Probing the Nature of Comets with HST, H. A. Weaver line_7:and P. D. Feldman, in "Science with the Hubble Space Telescope", line_8:ESA-NASA CP, in press. line_9: line_10:Presentations on both the above programs have been made at several line_11:scientific meetings, including the annual DPS meetings in 1990 line_12:(for 3064), 1991 (for 2481), and 1992 (2481 and 2483). A paper line_13:on our detection of CO Cameron band emission in P/Hartley 2 line_14:will be submitted to a refereed journal shortly. QUESTION: 10 SECTION: 1 line_1:The STScI has excellent data-analysis capabilities and also maintains line_2:a pool of Science Data Analysts (SDAs) that are available to its staff. line_3:However, SDA support for our program can only be assured if we are line_4:allocated money to cover the SDA's salary. line_5: line_6:The other institutions co-sponsoring this program also have excellent line_7:data analysis facilities and access to graduate students and research line_8:assistants. However, funds must be provided by this program in order line_9:for the Co-Is to utilize these resources. GENERAL_FORM_ADDRESS: LNAME: Weaver FNAME: Harold TITLE: Dr. MI: A. CATEGORY: PI INST: STScI ADDR_1: 3700 San Martin Drive ADDR_2: Baltimore, MD 21218 ADDR_3: USA CITY: Baltimore STATE: MD ZIP: 21218 COUNTRY: USA PHONE: 410-338-5004 SOLAR_SYSTEM_TARGETS: TARGNUM: 1 NAME_1: SL-7 DESCR_1: COMET SHOEMAKER-LEVY 1993E-7 LEV1_1: FILE = SL-7, LEV1_2: ACQ = 3 fluxnum_1: 1 fluxval_1: SURF(V) = 24 +/- 1 fluxnum_2: 2 fluxval_2: SIZE = 0.1 comment_1: THIS TARGET IS THE GANG OF comment_2: FOUR OF COMET SL 1993E. comment_3: THE LETTER DESIGNATION IS Q. TARGNUM: 2 NAME_1: SL-15 DESCR_1: COMET SHOEMAKER-LEVY 1993E-15 LEV1_1: FILE = SL-15, LEV1_2: ACQ = 3 fluxnum_1: 1 fluxval_1: SURF(V) = 24 +/- 1 fluxnum_2: 2 fluxval_2: SIZE = 0.1 comment_1: THIS TARGET IS THE BRIGHTEST comment_2: NUCLEUS OF COMET SL 1993E. comment_3: THE LETTER DESIGNATION IS G. TARGNUM: 3 NAME_1: SL-5 DESCR_1: COMET SHOEMAKER-LEVY 1993E-5 LEV1_1: FILE = SL-5, LEV1_2: ACQ = 3 fluxnum_1: 1 fluxval_1: SURF(V) = 24 +/- 1 fluxnum_2: 2 fluxval_2: SIZE = 0.1 comment_1: THIS TARGET IS A BRIGHT comment_2: NUCLEUS OF COMET SL 1993E comment_3: THAT MAY BE FRAGMENTING. comment_4: THE LETTER DESIGNATION IS S. TARGNUM: 4 NAME_1: SL-12 DESCR_1: COMET SHOEMAKER-LEVY 1993E-12 LEV1_1: FILE = SL-12, LEV1_2: ACQ = 3 fluxnum_1: 1 fluxval_1: SURF(V) = 24 +/- 1 fluxnum_2: 2 fluxval_2: SIZE = 0.1 comment_1: THIS TARGET IS A BRIGHT comment_2: NUCLEUS OF COMET SL 1993E. comment_3: THE LETTER DESIGNATION IS K. ! TARGNUM: 5 NAME_1: SL-11 DESCR_1: COMET SHOEMAKER-LEVY 1993E-11 LEV1_1: FILE = SL-11, LEV1_2: ACQ = 3 fluxnum_1: 1 fluxval_1: SURF(V) = 24 +/- 1 fluxnum_2: 2 fluxval_2: SIZE = 0.1 comment_1: THIS TARGET IS A BRIGHT comment_2: NUCLEUS OF COMET SL 1993E. comment_3: THE LETTER DESIGNATION IS L. ! exposure_logsheet: linenum: 1.100 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: CYCLE 4 / 1.1-5.2; req_2: SEQ 1.1-1.4 NO GAP; req_3: AT 12-JUL-94 +/- 1D; comment_1: 1st orbit, 1st image for SL-7. comment_2: Take this during 7/11-13/94. ! linenum: 1.200 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-7 comment_2: during the 7/11-13/94 period. ! linenum: 1.300 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 1st image for SL-7 comment_2: during the 7/11-13/94 period. ! linenum: 1.400 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 2nd image for SL-7 comment_2: during the 7/11-13/94 period. ! linenum: 1.500 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 1.5-1.8 NO GAP; req_2: AT 20-JUL-94:08:30 +/- 3H; comment_1: 1st orbit, 1st image for SL-7 comment_2: during day 201 (7/20). comment_3: I really want the two consecutive comment_4: orbits between 7:00-10:30 UTC. ! linenum: 1.600 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-7 comment_2: during day 201 (7/20). ! linenum: 1.700 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 1st image for SL-7 comment_2: during day 201 (7/20). ! linenum: 1.800 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 2nd image for SL-7 comment_2: during day 201 (7/20). linenum: 1.900 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 1.900-1.910 NO GAP; req_2: AT 4-JUL-94 +/- 1D; comment_1: 1st orbit, 1st image for SL-7 comment_2: during day 201 (7/20). comment_3: I really want as close to comment_4: July 4th as possible. linenum: 1.910 targname: SL-7 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-7 comment_2: during 7/4. linenum: 2.100 targname: SL-15 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 2.1-2.4 NO GAP; req_2: AT 14-JUL-94 +/- 3D; comment_1: I want two consecutive orbits comment_2: ANYTIME during sms 192. comment_3: 1st orbit, 1st image for SL-15 comment_4: during the 192 sms. linenum: 2.200 targname: SL-15 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-15 comment_2: during the 192 sms. linenum: 2.300 targname: SL-15 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 1st image for SL-15 comment_2: during the 192 sms. linenum: 2.400 targname: SL-15 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 2nd image for SL-15 comment_2: during the 192 sms. linenum: 2.500 targname: SL-15 config: FOS/RD opmode: ACCUM aperture: 4.3 sp_element: G270H num_exp: 1 time_per_exp: 25 M req_1: SEQ 2.5-2.6 NO GAP; req_2: AT 14-JUL-94 +/- 3D; comment_1: I want two consecutive orbits comment_2: ANYTIME during sms 192. comment_3: It would be NICE to put the comment_4: exps as close as possible to comment_5: the WFPC2 exps. comment_6: 1st orbit FOS exp for SL-15. ! linenum: 2.600 targname: SL-15 config: FOS/RD opmode: ACCUM aperture: 4.3 sp_element: G270H num_exp: 1 time_per_exp: 35 M comment_1: 2nd orbit FOS exp for SL-15. comment_2: Please change exp time to optimally comment_3: match the time available in the orbit. ! linenum: 3.100 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 3.1-3.22 NO GAP; req_2: AT 14-JUL-94 +/- 3D; comment_1: I want one orbit ANYTIME comment_2: during the 192 sms. comment_3: 1st orbit, 1st image for SL-5 comment_4: during the 192 sms. ! linenum: 3.200 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL5 comment_2: during the 192 sms. ! linenum: 3.210 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 1st image for SL5 comment_2: during the 192 sms. ! linenum: 3.220 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 1000 S comment_1: 2nd orbit, 2nd image for SL5 comment_2: during the 192 sms. ! linenum: 3.300 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 3.3-3.4 NO GAP; req_2: AT 20-JUL-94:17:45 +/- 3H; comment_1: I really want one orbit comment_2: during the 17:20-18:10 window comment_3: in the 199 sms. comment_4: 1st orbit, 1st image for SL-5 comment_5: during the 199 sms. ! linenum: 3.400 targname: SL-5 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL5 comment_2: during the 199 sms. ! linenum: 4.100 targname: SL-12 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 4.1-4.2 NO GAP; req_2: AT 18-JUL-94:17:00 +/- 3H; comment_1: 1st orbit, 1st image for SL-12 comment_2: during day 199 (7/18). comment_3: I really want one comment_4: orbit between 15:20-18:00 UTC. linenum: 4.200 targname: SL-12 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-7 comment_2: during day 199 (7/18). ! linenum: 4.300 targname: SL-12 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 4.3-4.4 NO GAP; req_3: AT 30-JUN-94 +/- 3D; comment_1: 1st orbit, 1st image for SL-12 comment_2: Take this as close to 6/27 comment_3: as possible. linenum: 4.400 targname: SL-12 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-12 comment_2: near 6/27. ! linenum: 5.100 targname: SL-11 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S req_1: SEQ 5.1-5.2 NO GAP; req_2: AT 19-JUL-94:13:30 +/- 3H; comment_1: 1st orbit, 1st image for SL-11 comment_2: I really want the orbit comment_3: between 12:20 and 14:50. ! linenum: 5.200 targname: SL-11 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F702W param_1: CR-SPLIT=NO num_exp: 1 time_per_exp: 800 S comment_1: 1st orbit, 2nd image for SL-11 comment_2: during 7/19. !~~~RPSS~~~,P4349,psl1993e-dd-july94v2.prop,23-MAY-1994 17:55