Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.
Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact
Michael J. Mumma,1*Michael A. DiSanti,1Karen Magee-Sauer,2Boncho P. Bonev,1,3Geronimo L. Villanueva,1Hideyo Kawakita,4Neil Dello Russo,5Erika L. Gibb,6Geoffrey A. Blake,7James E. Lyke,8Randall D. Campbell,8Joel Aycock,8Al Conrad,8Grant M. Hill8
We quantified eight parent volatiles (H2O, C2H6, HCN, CO, CH3OH,H2CO, C2H2, and CH4) in the Jupiter-family comet Tempel 1 usinghigh-dispersion infrared spectroscopy in the wavelength range2.8 to 5.0 micrometers. The abundance ratio for ethane was significantlyhigher after impact, whereas those for methanol and hydrogencyanide were unchanged. The abundance ratios in the ejecta aresimilar to those for most Oort cloud comets, but methanol andacetylene are lower in Tempel 1 by a factor of about 2. Theseresults suggest that the volatile ices in Tempel 1 and in mostOort cloud comets originated in a common region of the protoplanetarydisk.
1 Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. 2 Department of Physics and Astronomy, Rowan University, Glassboro, NJ 08028–1701, USA. 3 Ritter Astrophysical Research Center, Department of Physics and Astronomy, University of Toledo, Toledo, OH 43606, USA. 4 Department of Physics, Kyoto Sangyo University, Motoyama, Kamigamo, Kita-ku, Kyoto 603-8555, Japan. 5 Space Department, Planetary Exploration Group, Applied Physics Laboratory/Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723–6099, USA. 6 Department of Physics and Astronomy, University of Missouri, St. Louis, MO 63121–4499, USA. 7 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA. 8 W. M. Keck Observatory, 65-1120 Mamalahoa Highway, Kameula, HI 96743, USA.
* To whom correspondence should be addressed. E-mail: michael.j.mumma{at}nasa.gov
The editors suggest the following Related Resources on Science sites:
In Science Magazine
RESEARCH ARTICLES
M. F. A'Hearn, M. J. S. Belton, W. A. Delamere, J. Kissel, K. P. Klaasen, L. A. McFadden, K. J. Meech, H. J. Melosh, P. H. Schultz, J. M. Sunshine, P. C. Thomas, J. Veverka, D. K. Yeomans, M. W. Baca, I. Busko, C. J. Crockett, S. M. Collins, M. Desnoyer, C. A. Eberhardy, C. M. Ernst, T. L. Farnham, L. Feaga, O. Groussin, D. Hampton, S. I. Ipatov, J.-Y. Li, D. Lindler, C. M. Lisse, N. Mastrodemos, W. M. Owen, Jr., J. E. Richardson, D. D. Wellnitz, and R. L. White (14 October 2005) Science310 (5746), 258.
[DOI: 10.1126/science.1118923] |Abstract »|Full Text »|PDF »|Supporting Online Material »
RESEARCH ARTICLES
K. J. Meech, N. Ageorges, M. F. A'Hearn, C. Arpigny, A. Ates, J. Aycock, S. Bagnulo, J. Bailey, R. Barber, L. Barrera, R. Barrena, J. M. Bauer, M. J. S. Belton, F. Bensch, B. Bhattacharya, N. Biver, G. Blake, D. Bockelée-Morvan, H. Boehnhardt, B. P. Bonev, T. Bonev, M. W. Buie, M. G. Burton, H. M. Butner, R. Cabanac, R. Campbell, H. Campins, M. T. Capria, T. Carroll, F. Chaffee, S. B. Charnley, R. Cleis, A. Coates, A. Cochran, P. Colom, A. Conrad, I. M. Coulson, J. Crovisier, J. deBuizer, R. Dekany, J. de Léon, N. Dello Russo, A. Delsanti, M. DiSanti, J. Drummond, L. Dundon, P. B. Etzel, T. L. Farnham, P. Feldman, Y. R. Fernández, M. D. Filipovic, S. Fisher, A. Fitzsimmons, D. Fong, R. Fugate, H. Fujiwara, T. Fujiyoshi, R. Furusho, T. Fuse, E. Gibb, O. Groussin, S. Gulkis, M. Gurwell, E. Hadamcik, O. Hainaut, D. Harker, D. Harrington, M. Harwit, S. Hasegawa, C. W. Hergenrother, P. Hirst, K. Hodapp, M. Honda, E. S. Howell, D. Hutsemékers, D. Iono, W.-H. Ip, W. Jackson, E. Jehin, Z. J. Jiang, G. H. Jones, P. A. Jones, T. Kadono, U. W. Kamath, H. U. Käufl, T. Kasuga, H. Kawakita, M. S. Kelley, F. Kerber, M. Kidger, D. Kinoshita, M. Knight, L. Lara, S. M. Larson, S. Lederer, C.-F. Lee, A. C. Levasseur-Regourd, J. Y. Li, Q.-S. Li, J. Licandro, Z.-Y. Lin, C. M. Lisse, G. LoCurto, A. J. Lovell, S. C. Lowry, J. Lyke, D. Lynch, J. Ma, K. Magee-Sauer, G. Maheswar, J. Manfroid, O. Marco, P. Martin, G. Melnick, S. Miller, T. Miyata, G. H. Moriarty-Schieven, N. Moskovitz, B. E. A. Mueller, M. J. Mumma, S. Muneer, D. A. Neufeld, T. Ootsubo, D. Osip, S. K. Pandea, E. Pantin, R. Paterno-Mahler, B. Patten, B. E. Penprase, A. Peck, G. Petitas, N. Pinilla-Alonso, J. Pittichova, E. Pompei, T. P. Prabhu, C. Qi, R. Rao, H. Rauer, H. Reitsema, S. D. Rodgers, P. Rodriguez, R. Ruane, G. Ruch, W. Rujopakarn, D. K. Sahu, S. Sako, I. Sakon, N. Samarasinha, J. M. Sarkissian, I. Saviane, M. Schirmer, P. Schultz, R. Schulz, P. Seitzer, T. Sekiguchi, F. Selman, M. Serra-Ricart, R. Sharp, R. L. Snell, C. Snodgrass, T. Stallard, G. Stecklein, C. Sterken, J. A. Stüwe, S. Sugita, M. Sumner, N. Suntzeff, R. Swaters, S. Takakuwa, N. Takato, J. Thomas-Osip, E. Thompson, A. T. Tokunaga, G. P. Tozzi, H. Tran, M. Troy, C. Trujillo, J. Van Cleve, R. Vasundhara, R. Vazquez, F. Vilas, G. Villanueva, K. von Braun, P. Vora, R. J. Wainscoat, K. Walsh, J. Watanabe, H. A. Weaver, W. Weaver, M. Weiler, P. R. Weissman, W. F. Welsh, D. Wilner, S. Wolk, M. Womack, D. Wooden, L. M. Woodney, C. Woodward, Z.-Y. Wu, J.-H. Wu, T. Yamashita, B. Yang, Y.-B. Yang, S. Yokogawa, A. C. Zook, A. Zauderer, X. Zhao, X. Zhou, and J.-M. Zucconi (14 October 2005) Science310 (5746), 265.
[DOI: 10.1126/science.1118978] |Abstract »|Full Text »|PDF »
REPORTS
Horst Uwe Keller, Laurent Jorda, Michael Küppers, Pedro J. Gutierrez, Stubbe F. Hviid, Jörg Knollenberg, Luisa-Maria Lara, Holger Sierks, Cesare Barbieri, Philippe Lamy, Hans Rickman, and Rafael Rodrigo (14 October 2005) Science310 (5746), 281.
[DOI: 10.1126/science.1119020] |Abstract »|Full Text »|PDF »
REPORTS
S. Sugita, T. Ootsubo, T. Kadono, M. Honda, S. Sako, T. Miyata, I. Sakon, T. Yamashita, H. Kawakita, H. Fujiwara, T. Fujiyoshi, N. Takato, T. Fuse, J. Watanabe, R. Furusho, S. Hasegawa, T. Kasuga, T. Sekiguchi, D. Kinoshita, K. J. Meech, D. H. Wooden, W. H. Ip, and M. F. A'Hearn (14 October 2005) Science310 (5746), 274.
[DOI: 10.1126/science.1119091] |Abstract »|Full Text »|PDF »|Supporting Online Material »
Deep Impact: Observations from a Worldwide Earth-Based Campaign.
K. J. Meech, N. Ageorges, M. F. A'Hearn, C. Arpigny, A. Ates, J. Aycock, S. Bagnulo, J. Bailey, R. Barber, L. Barrera, et al. (2005)
Science
310, 265-269
|Abstract »|Full Text »|PDF »
