visit 13 change G230LB to G230L (NUV MAMA), Time Tag, Buffer Time =5000s,
52x0.5 aperture
changed buffer time to 200s
----- Attempting Submission 9 (Tue Aug 24 19:35:40 GMT 2010) -----
----- Attempting Submission 10 (Thu Sep 09 13:39:41 GMT 2010) -----
----- Attempting Submission 11 (Fri Sep 24 15:00:56 GMT 2010) -----
----- Attempting Submission 12 (Mon Oct 11 15:50:34 GMT 2010) -----
----- Attempting Submission 13 (Mon Oct 18 01:39:20 GMT 2010) -----
----- Attempting Submission 14 (Fri Oct 29 13:48:24 GMT 2010) -----
----- Attempting Submission 15 (Fri Nov 05 17:27:58 GMT 2010) -----
HST Phase II Proposal 12312 (12312.apt) successfully submitted.
----- Attempting Submission 16 (Fri Nov 05 18:06:56 GMT 2010) -----
HST Phase II Proposal 12312 (12312.apt) successfully submitted.
----- Attempting Submission 17 (Fri Nov 05 18:32:41 GMT 2010) -----
----- Attempting Submission 18 (Thu Nov 11 16:23:17 GMT 2010) -----
----- Attempting Submission 19 (Tue Nov 16 16:15:00 GMT 2010) -----
Alison: Please verify that the new target (#3=103P-Hartley-2-C) is used for visits 11-15,
which will be executed during the last week in November.
Hubble Investigation of 103P/Hartley 2 in Support of NASA's DIXI Mission
Comet 103P/Hartley 2 is a small but highly active comet that will pass
unusually close to the Earth (0.12 AU) during the fall of 2010, when it
will also be visited by NASA's DIXI spacecraft. We propose a 15-orbit
spectroscopic observing campaign with Hubble, comprised of three 5-orbit
visits spanning a 2-month period, to measure the abundances of several
key volatiles (CO, CO2, S2) and their possible seasonal variations. CO
has not yet been detected in 103P, and Hubble may be the only facility
capable of doing it. Hubble is also uniquely capable of providing
confirmation of DIXI's measurements of the CO2 abundance. The DIXI flyby
is an exceptional opportunity to study the nature of comets, and Hubble
will contribute important and unique data to the international campaign
supporting this mission.
We plan to observe 103P/Hartley 2 during three different epochs: on the same day as the NASA
DIXI mission's closest approach (CA) to the comet (on 4-Nov-2010), roughly 1 month before CA, and roughly 1 month after CA.
During each epoch, we will execute exactly the same 5-orbit sequence of observations:
Orbit #1 --> COS/FUV G160M
Orbit #2 --> COS/NUV G185M
Orbit #3 --> STIS/CCD G230LB + STIS/CCD image with F28x50LP
Orbit #4 --> COS/FUV G160M
Orbit #5 --> COS/NUV G185M
Finding adequate guide star coverage for this fast-moving target is going to be a major challenge for this program,
and GS selection may end up dictating where these observations are scheduled.
SOLAR SYSTEM
12
false
0.0
0.0
false
false
false
false
false
false
SUPPORTED
SOLAR SYSTEM
Currently using JPL #50 reference ephemeris. This should be accurate enough for planning the Hubble observations this fall.
COMET
103P-HARTLEY2-DIXI
TYPE=COMET,Q=1.0586833307917800,E=0.6951398461582717,I=13.61732081969205,O=219.76129504028940,W=181.19735624925000,T=28-OCT-2010:06:10:23,EQUINOX=J2000,EPOCH=25-SEP-2010:00:00:00,A1=1.80911924294E-09,A2=-3.1418447208E-11,A3=4.8989105707E-10
EARTH
SOLAR SYSTEM
This is the JPL #122 reference ephemeris and should be accurate enough for planning the Hubble observations on Nov4, 2010
COMET
103P-HARTLEY2-DIXI-NOV4
TYPE=COMET,Q=1.058676120124298,E=0.6949802846326966,I=13.61928878420733,O=219.7596943092058,W=181.2071038939688,T=28-OCT-2010:06:20:57,EQUINOX=J2000,EPOCH=04-NOV-2010:00:00:00,A1=6.028426008179833E-10,A2=-5.704220041383923E-11,A3=2.354554128002155E-09
EARTH
SOLAR SYSTEM
This is the JPL #214 reference ephemeris and should be accurate enough for planning the Hubble observations on Nov28, 2010
COMET
103P-HARTLEY2-DIXI-NOV28
TYPE=COMET,Q=1.058676120124298,E=0.6948944852399084,I=13.61937718211394,O=219.7584073592891,W=181.2099419064577,T=28-OCT-2010:06:22:11,EQUINOX=J2000,EPOCH=28-NOV-2010:00:00:00
EARTH
COS/FUV
Spectroscopic
No
No
G160M
1589
COS/NUV
Spectroscopic
No
No
G185M
1986
STIS/CCD
Spectroscopic
No
No
G230LB
2375
COS/FUV
Spectroscopic
No
No
G160M
1589
COS/NUV
Spectroscopic
No
No
G185M
1986
STIS/CCD
Spectroscopic
No
No
G230LB
2375
COS/FUV
Spectroscopic
No
No
G160M
1589
COS/NUV
Spectroscopic
No
No
G185M
1986
STIS/CCD
Spectroscopic
No
No
G230LB
2375
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Using ephemeris for target 12312-02-103P-HARTLEY-2
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