Subaru telescope observations of Deep Impact

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; M. F. A'Hearn

doi:10.1126/science.1119091

Subaru telescope observations of Deep Impact

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. MeechD. H. Wooden, W. H. Ip, M. F. A'Hearn

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摘要

The impact cratering process on a comet is controversial but holds the key for interpreting observations of the Deep Impact collision with comet 9P/Tempel 1. Mid-infrared data from the Cooled Mid-Infrared Camera and Spectrometer (COMICS) of the Subaru Telescope indicate that the large-scale dust plume ejected by the impact contained a large mass (∼10⁶ kilograms) of dust and formed two wings approximately ±45° from the symmetric center, both consistent with gravity as the primary control on the impact and its immediate aftermath. The dust distribution in the inner part of the plume, however, is inconsistent with a pure gravity control and implies that evaporation and expansion of volatiles accelerated dust.

原文	???core.languages.en_GB???
頁（從 - 到）	274-278
頁數	5
期刊	Science
卷	310
發行號	5746
DOIs	https://doi.org/10.1126/science.1119091
出版狀態	已出版 - 14 10月 2005

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10.1126/science.1119091

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Sugita, S., Ootsubo, T., Kadono, T., Honda, M., Sako, S., Miyata, T., Sakon, I., Yamashita, T., Kawakita, H., Fujiwara, H., Fujiyoshi, T., Takato, N., Fuse, T., Watanabe, J., Furusho, R., Hasegawa, S., Kasuga, T., Sekiguchi, T., Kinoshita, D., ... A'Hearn, M. F. (2005). Subaru telescope observations of Deep Impact. Science, 310(5746), 274-278. https://doi.org/10.1126/science.1119091

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title = "Subaru telescope observations of Deep Impact",

abstract = "The impact cratering process on a comet is controversial but holds the key for interpreting observations of the Deep Impact collision with comet 9P/Tempel 1. Mid-infrared data from the Cooled Mid-Infrared Camera and Spectrometer (COMICS) of the Subaru Telescope indicate that the large-scale dust plume ejected by the impact contained a large mass (∼106 kilograms) of dust and formed two wings approximately ±45° from the symmetric center, both consistent with gravity as the primary control on the impact and its immediate aftermath. The dust distribution in the inner part of the plume, however, is inconsistent with a pure gravity control and implies that evaporation and expansion of volatiles accelerated dust.",

author = "S. Sugita and T. Ootsubo and T. Kadono and M. Honda and S. Sako and T. Miyata and I. Sakon and T. Yamashita and H. Kawakita and H. Fujiwara and T. Fujiyoshi and N. Takato and T. Fuse and J. Watanabe and R. Furusho and S. Hasegawa and T. Kasuga and T. Sekiguchi and D. Kinoshita and Meech, {K. J.} and Wooden, {D. H.} and Ip, {W. H.} and A'Hearn, {M. F.}",

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Sugita, S, Ootsubo, T, Kadono, T, Honda, M, Sako, S, Miyata, T, Sakon, I, Yamashita, T, Kawakita, H, Fujiwara, H, Fujiyoshi, T, Takato, N, Fuse, T, Watanabe, J, Furusho, R, Hasegawa, S, Kasuga, T, Sekiguchi, T, Kinoshita, D, Meech, KJ, Wooden, DH, Ip, WH & A'Hearn, MF 2005, 'Subaru telescope observations of Deep Impact', Science, 卷 310, 編號 5746, 頁 274-278. https://doi.org/10.1126/science.1119091

TY - JOUR

T1 - Subaru telescope observations of Deep Impact

AU - Sugita, S.

AU - Ootsubo, T.

AU - Kadono, T.

AU - Honda, M.

AU - Sako, S.

AU - Miyata, T.

AU - Sakon, I.

AU - Yamashita, T.

AU - Kawakita, H.

AU - Fujiwara, H.

AU - Fujiyoshi, T.

AU - Takato, N.

AU - Fuse, T.

AU - Watanabe, J.

AU - Furusho, R.

AU - Hasegawa, S.

AU - Kasuga, T.

AU - Sekiguchi, T.

AU - Kinoshita, D.

AU - Meech, K. J.

AU - Wooden, D. H.

AU - Ip, W. H.

AU - A'Hearn, M. F.

PY - 2005/10/14

Y1 - 2005/10/14

N2 - The impact cratering process on a comet is controversial but holds the key for interpreting observations of the Deep Impact collision with comet 9P/Tempel 1. Mid-infrared data from the Cooled Mid-Infrared Camera and Spectrometer (COMICS) of the Subaru Telescope indicate that the large-scale dust plume ejected by the impact contained a large mass (∼106 kilograms) of dust and formed two wings approximately ±45° from the symmetric center, both consistent with gravity as the primary control on the impact and its immediate aftermath. The dust distribution in the inner part of the plume, however, is inconsistent with a pure gravity control and implies that evaporation and expansion of volatiles accelerated dust.

AB - The impact cratering process on a comet is controversial but holds the key for interpreting observations of the Deep Impact collision with comet 9P/Tempel 1. Mid-infrared data from the Cooled Mid-Infrared Camera and Spectrometer (COMICS) of the Subaru Telescope indicate that the large-scale dust plume ejected by the impact contained a large mass (∼106 kilograms) of dust and formed two wings approximately ±45° from the symmetric center, both consistent with gravity as the primary control on the impact and its immediate aftermath. The dust distribution in the inner part of the plume, however, is inconsistent with a pure gravity control and implies that evaporation and expansion of volatiles accelerated dust.

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DO - 10.1126/science.1119091

M3 - 期刊論文

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SN - 0036-8075

VL - 310

SP - 274

EP - 278

JO - Science

JF - Science

IS - 5746

ER -

Subaru telescope observations of Deep Impact

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