Was a Long-Lived, High Velocity Gas Jet Produced by the Comet Tempel 1 Deep Impact Event: Evidence from High Spectral Resolution [OI] 630 nm Interference Spectra

Authors

J. B. Corliss, University of Wisconsin-Madison
F. L. Roesler, University of Wisconsin-MadisonFollow
E. J. Mierkiewicz, Embry-Riddle Aeronautical University - Daytona BeachFollow
R. J. Oliversen, NASA Goddard Space Flight CenterFollow
W. M. Harris, University of California-Davis

Document Type

Poster

Publication/Presentation Date

7-16-2008

Abstract/Description

Results from high impact spectral resolution observations of comet P/Tempel 1.

The poster information may be viewed here.

Publication Title

Asteroids, Comets, Meteors 2008

Sponsorship/Conference/Institution

The Johns Hopkins University Applied Physics Laboratory

Location

Baltimore, Maryland, July 13-18, 2008

Additional Information

Part of Poster Session II, Comet Tempel 1 and Deep Impact; this work supported by NASA grant NAG5-12812 to the University of Washington.

Dr. Mierkiewicz was not affiliated with Embry-Riddle Aeronautical University at the time this paper was published.

Scholarly Commons Citation

Corliss, J. B., Roesler, F. L., Mierkiewicz, E. J., Oliversen, R. J., & Harris, W. M. (2008). Was a Long-Lived, High Velocity Gas Jet Produced by the Comet Tempel 1 Deep Impact Event: Evidence from High Spectral Resolution [OI] 630 nm Interference Spectra. Asteroids, Comets, Meteors 2008, (). Retrieved from https://commons.erau.edu/db-physical-sciences/40