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William T. Reach
Researcher at Universities Space Research Association
Publications - 545
Citations - 95523
William T. Reach is an academic researcher from Universities Space Research Association. The author has contributed to research in topics: Galaxy & Interstellar medium. The author has an hindex of 131, co-authored 535 publications receiving 90496 citations. Previous affiliations of William T. Reach include California Institute of Technology & Space Telescope Science Institute.
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On the origin of interplanetary dust within recorded history
TL;DR: In this paper, the possibility of an abrupt origin of interplanetary dust as a result of a collision between asteroids or an extraordinary comet is considered, and the rate, surface area, and brightness of asteroid collision remnants are derived.
Journal ArticleDOI
Discovery of Broad Molecular lines and of Shocked Molecular Hydrogen from the Supernova Remnant G357.7+0.3: HHSMT, APEX, Spitzer and SOFIA Observations
TL;DR: In this paper, the authors reported a discovery of shocked gas from the supernova remnant (SNR) G357.7+0.3 using both millimeter and submillimeter observations.
Spectroscopy and Photometry of the Earth Grazer 2002 NY40
Andrew S. Rivkin,Ellen S. Howell,S. J. Bus,Michael D. Hicks,William T. Reach,Thomas H. Jarrett,R. P. Binzel +6 more
TL;DR: The near Earth asteroid 2002 NY40 was discovered on July 14, 2002 by the LINEAR survey and was predicted to make a close pass by the Earth on August 18, which led to observations at a large range of wavelengths, including radar as mentioned in this paper.
Posted Content
Spitzer's Solar System studies of asteroids, planets and the zodiacal cloud
David E. Trilling,Carey M. Lisse,Dale P. Cruikshank,Joshua P. Emery,Yanga R. Fernandez,Leigh N. Fletcher,Douglas P. Hamilton,Heidi B. Hammel,Alan W. Harris,Michael Mueller,Michael Mueller,Glenn S. Orton,Yvonne Pendleton,William T. Reach,Naomi Rowe-Gurney,Michael F. Skrutskie,Anne J. Verbiscer +16 more
TL;DR: In this paper, the authors describe results from Spitzer observations of asteroids, dust rings, and planets that provide new insight into the formation and evolution of our Solar System, including a large survey of Near Earth Objects, detection and characterization of several dust/debris disks in the Solar System; and comprehensive characterization of ice giant (Uranus, Neptune) atmospheres.