CaltechAUTHORS
  A Caltech Library Service

The Stardust Mission: Returning Comet Samples to Earth

Brownlee, D. E. and Tsou, P. and Burnett, D. S. and Clark, B. and Hanner, M. S. and Hörz, F. and Kissel, J. and McDonnell, J. A. M. and Newburn, R. L. and Sandford, S. and Sekanina, Z. and Tuzzolino, A. J. and Zolensky, M. (1997) The Stardust Mission: Returning Comet Samples to Earth. Meteoritics and Planetary Science, 32 (S4). A22. ISSN 1086-9379. https://resolver.caltech.edu/CaltechAUTHORS:20150506-142413492

[img] PDF - Published Version
See Usage Policy.

102Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20150506-142413492

Abstract

Stardust is an approved NASA mission that will collect large numbers of cometary particles and return them to Earth for laboratory analysis. The collected samples will be processed at the Curatorial Facility at the NASA Johnson Space Center in Houston, Texas, where they will be allocated to investigators in a manner similar to the existing lunar sample, cosmic dust, and Antarctic meteorite programs. We urge all investigators interested in primitive materials to begin seriously considering what they would like to do with the samples when they are returned to Earth. Stardust is the fourth mission in the new NASA Discovery program. It is highly focused on sample return and, following Discovery guidelines, is a low-cost, rapid-development project. The mission will launch in February 1999, fly past Comet Wild 2 on January 1, 2004, and return samples to Earth on January 13, 2006. The spacecraft will collect particles by direct impact into low-density silica aerogel during a 6.1-km/s flyby approaching within 150 km of the nucleus. The particles, ranging in size up to >200 μm, will penetrate several hundred particle diameters into the aerogel, where they will remain until they are extracted in the curatorial facility. The best model of the comet dust production indicates that Stardust will collect more than 20,000particles>15 μmin diameter in its 1000 cm^2 area of collection surface.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1945-5100.1997.tb01599.xDOIArticle
http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.1997.tb01599.x/abstractPublisherArticle
ORCID:
AuthorORCID
Burnett, D. S.0000-0001-9521-8675
Clark, B.0000-0002-5546-8757
Additional Information:© 1997 The Meteoritical Society.
Issue or Number:S4
Record Number:CaltechAUTHORS:20150506-142413492
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150506-142413492
Official Citation:(1997), Abstracts. Meteoritics & Planetary Science, 32: A5–A147. doi: 10.1111/j.1945-5100.1997.tb01599.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:57289
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:06 May 2015 22:08
Last Modified:09 Mar 2020 13:18

Repository Staff Only: item control page