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The abundance and distribution of presolar materials in cluster idps
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Messenger, Scott Keller, Lindsay Nakamura-Messenger, Keiko Ito, Motoo |
| Copyright Year | 2007 |
| Description | Presolar grains and remnants of interstellar organic compounds occur in a wide range of primitive solar system materials, including meteorites, interplanetary dust particles (IDPs), and comet Wild-2 samples. Among the most abundant presolar phases are silicate stardust grains and molecular cloud material. However, these materials have also been susceptible to destruction and alteration during parent body and nebular processing. In addition to their importance as direct samples of remote and ancient astrophysical environments, presolar materials thus provide a measure of how well different primitive bodies have preserved the original solar system starting materials. |
| File Size | 214634 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20070009863 |
| Archival Resource Key | ark:/13960/t3mw7dd81 |
| Language | English |
| Publisher Date | 2007-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Comets Meteorites Molecular Clouds Stardust Mission Silicates Solar System Interplanetary Dust Wild 2 Comet Organic Compounds Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
