Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact

Michael J. Mumma; Michael A. DiSanti; Karen Magee-Sauer; Boncho P. Bonev; Geronimo L. Villanueva; Hideyo Kawakita; Neil Dello Russo; Erika L. Gibb; Geoffrey A. Blake; James E. Lyke; Randall D. Campbell; Joel Aycock; Al Conrad; Grant M. Hill

doi:10.1126/science.1119337

Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact

Michael J. Mumma, Michael A. DiSanti, Karen Magee-Sauer, Boncho P. Bonev, Geronimo L. Villanueva, Hideyo Kawakita, Neil Dello Russo, Erika L. Gibb, Geoffrey A. Blake, James E. Lyke, Randall D. Campbell, Joel Aycock, Al Conrad, Grant M. Hill

University of Missouri-St. Louis

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	Science
Volume	310
DOIs	https://doi.org/10.1126/science.1119337
State	Published - Oct 14 2005

Disciplines

Chemistry
Biology

Access to Document

10.1126/science.1119337License: Unspecified

Cite this

@article{77693076c12f4c789f558ce733b92675,

title = "Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact",

author = "Mumma, {Michael J.} and DiSanti, {Michael A.} and Karen Magee-Sauer and Bonev, {Boncho P.} and Villanueva, {Geronimo L.} and Hideyo Kawakita and Russo, {Neil Dello} and Gibb, {Erika L.} and Blake, {Geoffrey A.} and Lyke, {James E.} and Campbell, {Randall D.} and Joel Aycock and Al Conrad and Hill, {Grant M.}",

note = "We quantified eight parent volatiles (H2O, C2H6, HCN, CO, CH3OH, H2CO, C2H2, and CH4) in the Jupiter-family comet Tempel 1 using high-dispersion infrared spectroscopy in the wavelength range 2.8 to 5.0 micrometers. The abundance ratio for ethane was significantly higher after impact, whereas those for methanol and hydrogen cyanide were unchanged.",

year = "2005",

month = oct,

day = "14",

doi = "10.1126/science.1119337",

language = "American English",

volume = "310",

journal = "Science",

}

TY - JOUR

T1 - Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact

AU - Mumma, Michael J.

AU - DiSanti, Michael A.

AU - Magee-Sauer, Karen

AU - Bonev, Boncho P.

AU - Villanueva, Geronimo L.

AU - Kawakita, Hideyo

AU - Russo, Neil Dello

AU - Gibb, Erika L.

AU - Blake, Geoffrey A.

AU - Lyke, James E.

AU - Campbell, Randall D.

AU - Aycock, Joel

AU - Conrad, Al

AU - Hill, Grant M.

N1 - We quantified eight parent volatiles (H2O, C2H6, HCN, CO, CH3OH, H2CO, C2H2, and CH4) in the Jupiter-family comet Tempel 1 using high-dispersion infrared spectroscopy in the wavelength range 2.8 to 5.0 micrometers. The abundance ratio for ethane was significantly higher after impact, whereas those for methanol and hydrogen cyanide were unchanged.

PY - 2005/10/14

Y1 - 2005/10/14

UR - http://science.sciencemag.org/content/sci/310/5746/270.full.pdf

U2 - 10.1126/science.1119337

DO - 10.1126/science.1119337

M3 - Article

VL - 310

JO - Science

JF - Science

ER -

Parent Volatiles in Comet 9P/Tempel 1: Before and After Impact

Disciplines

Access to Document

Other files and links

Cite this