The subsurface structure of comet 9P/Tempel 1 projected into the dust plume

T. Kadono; S. Sugita; S. Sako; Takafumi Ootsubo; H. Kawakita; M. Honda; T. Miyata; R. Furusho; J. Watanabe

doi:10.1007/978-3-540-76959-0_18

The subsurface structure of comet 9P/Tempel 1 projected into the dust plume

T. Kadono, S. Sugita, S. Sako, Takafumi Ootsubo, H. Kawakita, M. Honda, T. Miyata, R. Furusho, J. Watanabe

SCI - Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Cometary nuclei are believed to contain important information on the condition of the solar nebula, but little observational data is available on their interior structure. Our ground-based observations of NASA's Deep Impact event and the cratering mechanism show that comet 9P/ Tempel 1 has a surface layer consisting of small (submicron to micron-sized) carbonaceous grains whose thickness is a few tens of cm.

Original language	English
Title of host publication	Deep Impact as a World Observatory Event
Subtitle of host publication	Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference
Editors	Hans Ulrich Kaufl, Christiaan Sterken
Pages	143-146
Number of pages	4
DOIs	https://doi.org/10.1007/978-3-540-76959-0_18
Publication status	Published - 2009 Jan 1

Publication series

Name	ESO Astrophysics Symposia
Volume	2009
ISSN (Print)	1431-2433
ISSN (Electronic)	1611-6143

ASJC Scopus subject areas

Astronomy and Astrophysics
Physics and Astronomy (miscellaneous)

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10.1007/978-3-540-76959-0_18

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Kadono, T., Sugita, S., Sako, S., Ootsubo, T., Kawakita, H., Honda, M., Miyata, T., Furusho, R., & Watanabe, J. (2009). The subsurface structure of comet 9P/Tempel 1 projected into the dust plume. In H. U. Kaufl, & C. Sterken (Eds.), Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference (pp. 143-146). (ESO Astrophysics Symposia; Vol. 2009). https://doi.org/10.1007/978-3-540-76959-0_18

The subsurface structure of comet 9P/Tempel 1 projected into the dust plume. / Kadono, T.; Sugita, S.; Sako, S.; Ootsubo, Takafumi; Kawakita, H.; Honda, M.; Miyata, T.; Furusho, R.; Watanabe, J.

Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference. ed. / Hans Ulrich Kaufl; Christiaan Sterken. 2009. p. 143-146 (ESO Astrophysics Symposia; Vol. 2009).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Kadono, T, Sugita, S, Sako, S, Ootsubo, T, Kawakita, H, Honda, M, Miyata, T, Furusho, R & Watanabe, J 2009, The subsurface structure of comet 9P/Tempel 1 projected into the dust plume. in HU Kaufl & C Sterken (eds), Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference. ESO Astrophysics Symposia, vol. 2009, pp. 143-146. https://doi.org/10.1007/978-3-540-76959-0_18

Kadono T, Sugita S, Sako S, Ootsubo T, Kawakita H, Honda M et al. The subsurface structure of comet 9P/Tempel 1 projected into the dust plume. In Kaufl HU, Sterken C, editors, Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference. 2009. p. 143-146. (ESO Astrophysics Symposia). https://doi.org/10.1007/978-3-540-76959-0_18

Kadono, T. ; Sugita, S. ; Sako, S. ; Ootsubo, Takafumi ; Kawakita, H. ; Honda, M. ; Miyata, T. ; Furusho, R. ; Watanabe, J. / The subsurface structure of comet 9P/Tempel 1 projected into the dust plume. Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength: Proceedings of the ESO/VUB Conference. editor / Hans Ulrich Kaufl ; Christiaan Sterken. 2009. pp. 143-146 (ESO Astrophysics Symposia).

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The subsurface structure of comet 9P/Tempel 1 projected into the dust plume

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