Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 13 October 2000:
Vol. 290. no. 5490, pp. 320 - 325
DOI: 10.1126/science.290.5490.320

Reports

The Fall, Recovery, Orbit, and Composition of the Tagish Lake Meteorite: A New Type of Carbonaceous Chondrite

Peter G. Brown,1 Alan R. Hildebrand,3 Michael E. Zolensky,4 Monica Grady,5 Robert N. Clayton,6 Toshiko K. Mayeda,6 Edward Tagliaferri,7 Richard Spalding,8 Neil D. MacRae,9 Eric L. Hoffman,10 David W. Mittlefehldt,11 John F. Wacker,12 J. Andrew Bird,3 Margaret D. Campbell,1 Robert Carpenter,9 Heather Gingerich,9 Michael Glatiotis,3 Erika Greiner,9 Michael J. Mazur,3 Phil JA. McCausland,9 Howard Plotkin,2 Tina Rubak Mazur3

The preatmospheric mass of the Tagish Lake meteoroid was about 200,000 kilograms. Its calculated orbit indicates affinity to the Apollo asteroids with a semimajor axis in the middle of the asteroid belt, consistent with a linkage to low-albedo C, D, and P type asteroids. The mineralogy, oxygen isotope, and bulk chemical composition of recovered samples of the Tagish Lake meteorite are intermediate between CM and CI meteorites. These data suggest that the Tagish Lake meteorite may be one of the most primitive solar system materials yet studied.

1 Department of Physics and Astronomy,
2 Department of Philosophy, University of Western Ontario, London, Ontario N6A 3K7, Canada.
3 Department of Geology and Geophysics, University of Calgary, Calgary, Alberta T2N 1N4, Canada.
4 SN2, NASA Johnson Space Center, Houston, TX 77058, USA.
5 Department of Mineralogy, Natural History Museum, Cromwell Road, London SW7 5BD, UK.
6 Enrico Fermi Institute, Department of Chemistry, and Department of Geophysical Sciences, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA.
7 ET Space Systems, 5990 Worth Way, Camarillo, CA 93012, USA.
8 Sandia National Laboratories, Organization 5909, Mail Stop 0978, Post Office Box 5800, Albuquerque, NM 87185, USA.
9 Department of Earth Sciences, University of Western Ontario, London, Ontario N6A 5B7, Canada.
10 Activation Laboratories Ltd., 1336 Sandhill Drive, Ancaster, Ontario L9G 4V5, Canada.
11 Lockheed Martin SO, Houston, TX 77058, USA.
12 Pacific Northwest National Laboratory, Post Office Box 999, Richland, WA 99352, USA.


Read the Full Text



THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Collisional erosion and the non-chondritic composition of the terrestrial planets.
H. St.C O'Neill and H. Palme (2008)
Phil Trans R Soc A 366, 4205-4238
   Abstract »    Full Text »    PDF »
Oxygen Isotopes in Asteroidal Materials.
I. A. Franchi (2008)
Reviews in Mineralogy and Geochemistry 68, 345-397
   Abstract »    Full Text »    PDF »
Record of Low-Temperature Alteration in Asteroids.
M. E. Zolensky, A. N. Krot, and G. Benedix (2008)
Reviews in Mineralogy and Geochemistry 68, 429-462
   Abstract »    Full Text »    PDF »
Special Feature: Extraterrestrial amino acids in Orgueil and Ivuna: Tracing the parent body of CI type carbonaceous chondrites.
P. Ehrenfreund, D. P. Glavin, O. Botta, G. Cooper, and J. L. Bada (2001)
PNAS 98, 2138-2141
   Abstract »    Full Text »    PDF »
Stable Isotope Variations in Extraterrestrial Materials.
K. D. McKeegan, K. D. McKeegan, and L. A. Leshin (2001)
Reviews in Mineralogy and Geochemistry 43, 279-318
   Full Text »    PDF »
The Organic Content of the Tagish Lake Meteorite.
S. Pizzarello, Y. Huang, L. Becker, R. J. Poreda, R. A. Nieman, G. Cooper, and M. Williams (2001)
Science 293, 2236-2239
   Abstract »    Full Text »    PDF »
The Tagish Lake Meteorite: A Possible Sample from a D-Type Asteroid.
T. Hiroi, M. E. Zolensky, and C. M. Pieters (2001)
Science 293, 2234-2236
   Abstract »    Full Text »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)