Subaru/COMICS Mid-Infrared Spectroscopic Observations of the Dust Plume from Comet 9P/Tempel

被引:0
作者
Ootsubo, T. [1 ]
Sugita, S. [2 ]
Watanabe, J. [3 ]
Honda, M. [4 ]
Kawakita, H. [5 ]
Kadono, T. [6 ]
Furusho, R. [7 ]
机构
[1] Nagoya Univ, Grad Sch Sci, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
[2] Univ Tokyo, Dept Complex Sci & Engn, Kashiwa, Chiba 2778561, Japan
[3] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[4] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[5] Kyoto Sangyo Univ, Dept Phys, Kita Ku, Kyoto 6038555, Japan
[6] Japan Agcy Marine Earth Sci & Technol, Ctr Deep Earth Explorat, Yokohama, Kanagawa 2360001, Japan
[7] Waseda Univ, Tokyo 1698050, Japan
来源
DEEP IMPACT AS A WORLD OBSERVATORY EVENT: SYNERGIES IN SPACE, TIME, AND WAVELENGTH | 2009年
关键词
DEEP IMPACT; SUBARU-TELESCOPE; KUIPER-BELT; COMICS; SPECTROMETER; CAMERA;
D O I
10.1007/978-3-540-76959-0_16
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We carried out; mid-infrared observations of the Deep Impact (DI) collision with a Jupiter-family (JF) comet, 9P/Tempel, using the Cooled Mid-Infrared Camera and Spectrometer (COMICS) on the 8.2 m Subaru Telescope. The N-band spectrum (8-13 mu m; R similar to 250) of the dust ejecta from the comet nucleus 3.5 hours after the DI event shows a strong crystalline silicate feature. The Subaru/COMICS observation also reveals that small (< 1 mu m) amorphous pyroxene and carbon-rich grains flew away in the forefront of the ejecta, plume before our spectroscopic observation, leaving behind relatively large submicron (0.8-1 mu m) crystalline particles that we subsequently observed. The submicron grains within the subsurface layer of comet 9P/Tempel's nucleus have a higher crystalline-to-amorphous silicate ratio than that in the comae of other JF comets, and even that of Oort cloud comets. Near the comet nucleus 3.5 hours after the impact the crystalline-to-amorphous ratio is similar to that of Hale-Bopp coma, dust at 0,97 AU.
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页码:131 / +
页数:2
相关论文
共 20 条
[1]   Deep Impact: Excavating comet Tempel 1 [J].
A'Hearn, MF ;
Belton, MJS ;
Delamere, WA ;
Kissel, J ;
Klaasen, KP ;
McFadden, LA ;
Meech, KJ ;
Melosh, HJ ;
Schultz, PH ;
Sunshine, JM ;
Thomas, PC ;
Veverka, J ;
Yeomans, DK ;
Baca, MW ;
Busko, I ;
Crockett, CJ ;
Collins, SM ;
Desnoyer, M ;
Eberhardy, CA ;
Ernst, CM ;
Farnham, TL ;
Feaga, L ;
Groussin, O ;
Hampton, D ;
Ipatov, SI ;
Li, JY ;
Lindler, D ;
Lisse, CM ;
Mastrodemos, N ;
Owen, WM ;
Richardson, JE ;
Wellnitz, DD ;
White, RL .
SCIENCE, 2005, 310 (5746) :258-264
[2]   Spectral irradiance calibration in the infrared. X. A self-consistent radiometric all-sky network of absolutely calibrated stellar spectra [J].
Cohen, M ;
Walker, RG ;
Carter, B ;
Hammersley, P ;
Kidger, M ;
Noguchi, K .
ASTRONOMICAL JOURNAL, 1999, 117 (04) :1864-1889
[3]  
Furusho R, 2007, ICARUS, V190, P454, DOI 10.1016/j.icarus.2007.03.040
[4]   The Kuiper belt and the solar system's comet disk [J].
Gladman, B .
SCIENCE, 2005, 307 (5706) :71-75
[5]   Grain properties of comet C/1995 O1 (Hale-Bopp) [J].
Harker, DE ;
Wooden, DH ;
Woodward, CE ;
Lisse, CM .
ASTROPHYSICAL JOURNAL, 2002, 580 (01) :579-597
[6]   Grain properties of comet C/1995 O1 (Hale-Bopp) (vol 580, pg 579, 2002) [J].
Harker, DE ;
Wooden, DH ;
Woodward, CE ;
Lisse, CM .
ASTROPHYSICAL JOURNAL, 2004, 615 (02) :1081-1081
[7]   The dust grains from 9P/Tempel 1 before and after the encounter with deep impact [J].
Harker, DE ;
Woodward, CE ;
Wooden, DH .
SCIENCE, 2005, 310 (5746) :278-280
[8]   COMICS: The cooled mid-infrared camera and spectrometer for the Subaru Telescope [J].
Kataza, H ;
Okamoto, Y ;
Takubo, S ;
Onaka, T ;
Sako, S ;
Nakamura, K ;
Miyata, T ;
Yamashita, T .
OPTICAL AND IR TELESCOPE INSTRUMENTATION AND DETECTORS, PTS 1 AND 2, 2000, 4008 :1144-1152
[9]   The formation of the Kuiper belt by the outward transport of bodies during Neptune's migration [J].
Levison, HF ;
Morbidelli, A .
NATURE, 2003, 426 (6965) :419-421
[10]   Spitzer spectral observations of the Deep Impact ejecta [J].
Lisse, C. M. ;
VanCleve, J. ;
Adams, A. C. ;
A'Hearn, M. F. ;
Fernandez, Y. R. ;
Farnham, T. L. ;
Armus, L. ;
Grillmair, C. J. ;
Ingalls, J. ;
Belton, M. J. S. ;
Groussin, O. ;
McFadden, L. A. ;
Meech, K. J. ;
Schultz, P. H. ;
Clark, B. C. ;
Feaga, L. M. ;
Sunshine, J. M. .
SCIENCE, 2006, 313 (5787) :635-640