nh 3 in comets
DESCRIPTION
NH 3 in comets. Jennifer Hatchell (Exeter, ex-MPIfR). with. Mike Bird (RAIUB) William Sherwood (MPIfR) Wilhelm Altenhoff (MPIfR) Floris van der Tak (MPIfR) Karl Menten (MPIfR). Motivation. - NH 3 along with CO 2 and H 2 O is a constituent of cometary ices. - PowerPoint PPT PresentationTRANSCRIPT
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
NH3 in comets
with
Mike Bird (RAIUB)William Sherwood (MPIfR)Wilhelm Altenhoff (MPIfR)Floris van der Tak (MPIfR)Karl Menten (MPIfR)
Jennifer Hatchell (Exeter, ex-MPIfR)
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Motivation
- NH3 along with CO2 and H2O is a constituent of cometary ices.-Nitrogen chemistry in early solar nebula poorly understood (N2, NH3 and N balance)- Spin temperature (from ortho/para ratio) implies formation temperature of ices
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Radio observations
Photo: William Sherwood
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Previous radio detectionsC/1983 D IRAS-Araki-Alcock (Altenhoff et al. 1983)C/1996 B2 Hyakutake (Palmer et al. 1996, Green Bank)C/1995 O1 Hale-Bopp (Butler et al. 2002, Green Bank)C/1995 O1 Hale-Bopp (Hirota et al. 1999, Nobeyama)C/1995 O1 Hale-Bopp (Bird et al. 1997, Effelsberg)
Direct detectionHalley (Allen et al. 1987; Meier et al. 1994, Giotto)
6%
0.3%
1.8%
1.0-1.8%
NH3 /H2O
0.1-2%
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Optical detections of NH2 (daughter)
C/2002 T7 NH3 near 3 microns(Magee-Sauer et al. 2002)
C/1999 S4 LINEAR(Kawakita et al. 2001)C/1995 O1 Hale-Bopp &153P/Ikeya-Zhang(Kawakita et al. 2004)
Kawakita et al. 2002 reanalysisof earlier NH2 data
OPR 3.33Spin temp. 28K
Spin temp. 30K
NH3 /H2O = 0.5%
Infrared detections of NH3(lines often overlap with atmospheric absorptions)
NH3 /H2O = ???
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Targets 2001,2002,2004
Images:
T.V
sosk
e, T.L
ovejo
y, S.K
im, and
M.Jäger/
G.R
hem
an
C/2001 A2 (NEAT) C/2002 C1 (Ikeya-Zhang) (153P)
C/2001 Q4 (NEAT) C/2002 T7 (LINEAR)
2001 2002
2004
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
OH 1665/1667 MHz
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
NH
3 2
4 G
Hz
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
NH
3 2
4 G
Hz
NH3 /H2O <=
0.5%
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Conclusions
NH3 / H2O variable, 0.3-1.5% NH3 / H2O <= 0.5% in many comets: Halley and Hale-Bopp may have been exceptionalConsistency between radio / optically derived ratios
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JENNIFER HATCHELL – UNIVERSITY OF EXETER Cardiff Astrochemistry Jan 2004
Upcoming comet missions
Deep Impact (NASA)9P/Tempel 1launch date Jan 12 2005Impactor + cameras July 4 2005
Rosetta (ESA)67 P/Churyumov-
Gerasimenko launched 2 March 2004
Lander 2014Rosetta
Philae (lander)