A Younger Age for ALH84001 and Its Geochemical Link to Shergottite Sources in Mars

Author:

Lapen T. J.1,Righter M.1,Brandon A. D.12,Debaille V.3,Beard B. L.45,Shafer J. T.16,Peslier A. H.78

Affiliation:

1. Department of Earth and Atmospheric Sciences, University of Houston, Houston, TX 77204, USA.

2. NASA Johnson Space Center, Mail Code KR, Houston, TX 77058, USA.

3. Département des Sciences de la Terre et de l’Environnement, Université Libre de Bruxelles, 1050 Brussels, Belgium.

4. Department of Geosciences, University of Wisconsin, Madison, WI 53706, USA.

5. NASA Astrobiology Institute, University of Wisconsin, Madison, WI 53706, USA.

6. Lunar and Planetary Institute, Houston, TX 77058, USA.

7. Jacobs Technology, Engineering and Science Contract Group, Houston, TX 77058, USA.

8. ARES, NASA Johnson Space Center, Houston, TX 77058, USA.

Abstract

Less Old Martian Meteorite The oldest Martian meteorite known, ALH84001, was thought to be a remnant of primordial martian crust formed during solidification of an early magma ocean. Using isotope data, Lapen et al. (p. 347 ) revised the crystallization age of this meteorite from 4.51 billion years to 4.09 billion years ago, meaning that this rock cannot be a fragment of primordial crust that escaped the period of intense bombardment that occurred between 4.25 and 4.10 billion years ago. The revised age also suggests that magmatism was ongoing in Mars for a large part of its history and that ALH84001 was actually formed during the heavy bombardment period, just before the martian core dynamo stopped and the planetary magnetic field was lost.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference37 articles.

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