Loading...
Please wait, while we are loading the content...
Similar Documents
Physical properties of interplanetary grains
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Tomandl, D. A. Hodge, P. W. Brownlee, D. E. Horz, F. |
| Copyright Year | 1976 |
| Description | Morphological analyses of micrometeorite craters found on lunar rocks and laboratory simulation experiments are used to formulate a meteoritic interplanetary dust particle for optical scattering calculations that is roughly spherical and has a density of 2g cm/3. The model particle has chondritic elemental abundances and also contains a high content of finely dispersed carbon. |
| File Size | 5636603 |
| Page Count | 21 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19760014004 |
| Archival Resource Key | ark:/13960/t5v746z0w |
| Language | English |
| Publisher Date | 1976-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Astronomical Models Meteoroid Dust Clouds Chondrites Chemical Composition Carbon Interplanetary Dust Physical Properties Particles Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
