| dc.creator | Heymann, Dieter | |
| dc.date.accessioned | 2024-01-25T16:11:34Z | |
| dc.date.available | 2024-01-25T16:11:34Z | |
| dc.date.issued | 1964-11-28 | |
| dc.identifier.uri | https://repository.tcu.edu/handle/116099117/61650 | |
| dc.description | Article reprinted from Nature, which discusses the Canyon Diablo No. 2 and No. 3 stones in relation to those designated as Canyon Diablo No. 1, and suggests that rather than being separate masses (or even possibly distinct falls) they all originated from a singular varied parent mass. | |
| dc.relation | Oscar Monnig Papers (MS 124) | |
| dc.rights | Prior written permission from TCU Special Collections required to use any document or photograph. | |
| dc.source | Series III, Box 05, Canyon Diablo, 1905-1974 folder | |
| dc.subject | Meteorite | |
| dc.subject | Meteor Crater (Ariz.) | |
| dc.subject | Enrico Fermi Institute | |
| dc.subject | University of Chicago | |
| dc.subject | Heymann, Dieter | |
| dc.subject | Coarse octahedrite | |
| dc.subject | Kamacite | |
| dc.subject | Iron | |
| dc.subject | Palladium | |
| dc.subject | Anders, Edward | |
| dc.title | Origin of the Canyon Diablo No. 2 and No. 3 Meteorites | |
| dc.type | Document | |
| dc.description.transcription | | |
