Abstract
Studies related to the origin of life on Earth arehampered by the fact that suitable rocks dating from the first billion years arelacking due to metamorphism and plate tectonics. Thus the oldest traces oflife occur in rocks formed ~3.5 billion years ago [1, 2], a billion years afterthe formation of the Earth. As a consequence, the investigations now focus onMars where the ancient terrains have not been destroyed by plate tectonicactivity.One means of studying hypothetical Martian traces of life would be toanalyze sedimentary meteorites. However, only 49 meteorites of presumedMartian origin have been so far been found and all have a basalticcomposition. The aim of this study was to determine if sedimentary rocks andtheir embedded microfossils could survive the shock of entry into the Earth’satmosphere
| Original language | English |
|---|---|
| Article number | 5055 |
| Pages (from-to) | A207 |
| Number of pages | 1 |
| Journal | Meteoritics & Planetary Sciences |
| Volume | 44 |
| Issue number | Suppl. S7 |
| DOIs | |
| Publication status | Published - Jul 2009 |
| Event | 72nd Annual Meteoritical Society Meeting (2009) - Nancy, France Duration: 13 Jul 2009 → 18 Jul 2009 |
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