The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk

Author:

Connelly James N.1,Bizzarro Martin1,Krot Alexander N.12,Nordlund Åke3,Wielandt Daniel1,Ivanova Marina A.4

Affiliation:

1. Centre for Star and Planet Formation and Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark.

2. Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i at Manoa, HI 96822, USA.

3. Centre for Star and Planet Formation and Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark.

4. Vernadsky Institute of Geochemistry and Analytical Chemistry, Moscow 119991, Russia.

Abstract

Dating the First Solids The solar system's first solids: calcium-aluminum–rich inclusions and chondrules are found in meteorites and provide a direct record of the dynamics of the solar protoplanetary disk that led to the formation of the solar system. Previous results indicate that chondrules formed 1 to 2 million years after the inclusions—an age difference that has been used in constructing models of chondrule formation. Based on uranium- and lead-isotope measurements of a collection of these primitive materials, Connelly et al. (p. 651 ) show that chondrules in fact started to form at the same time as the inclusions, 4.567 billion years ago, and that their formation took about 3 million years.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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