| BCC9601 photomicrographs |
|
| BCC9602 |
|
| BCC9603 | |
| BCC9604 |
|
| BCC9607 This sample appears to match BCC9805 below and is placed on hold under the same conditions as BCC9805 and requires much more analytical work. |
|
| BCC9701 photomicrographs | |
| BCC9702 |
|
| BCC9703 |
|
| BCC9704 |
|
| BCC9705 | |
|
|
BCC9706 |
|
|
BCC9707 |
|
|
BCC9801 |
|
|
BCC9802 |
|
|
BCC9803 |
|
|
BCC9804
photomicrographs |
|
|
BCC9805
photomicrographs This sample is on hold and being classified as a pseudo-meteorite. Even though it contains abundant Ni particles much more work needs to be done on this one. |
|
|
BCC9807 photomicrographs |
|
|
BCC9809 |
|
|
BCC9912 |
|
|
BCC9901 |
|
|
BCC9902 |
|
|
BCC9903 photomicrographs |
|
|
BCC9907 |
|
|
BCC9908 photomicrographs |
|
|
BCC9909 |
|
|
BCC9910 |
|
|
BCC9911 |
|
|
BCC9912 |
|
|
BCC9913 |
| BCC0001 photomicrographs
Remote sensing vs lab analysis of
stellar grains |
|
| 2000 (additional pending) | |
| 2001, 2002 (pending) | |