Origin of Isotopic Diversity among Carbonaceous Chondrites
Carbonaceous chondrites are some of the most primitive meteorites and derive from planetesimals that formed a few million years after the beginning of the solar system. Here, using new and previously published Cr, Ti, and Te isotopic data, we show that carbonaceous chondrites exhibit correlated isot...
Main Authors: | Jan L. Hellmann, Jonas M. Schneider, Elias Wölfer, Joanna Drążkowska, Christian A. Jansen, Timo Hopp, Christoph Burkhardt, Thorsten Kleine |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/acc102 |
Similar Items
-
Oxygen Isotopic Variations in the Calcium, Aluminum-rich Inclusion–forming Region Recorded by a Single Refractory Inclusion from the CO3.1 Carbonaceous Chondrite Dar al Gani 083
by: Samuel Ebert, et al.
Published: (2024-01-01) -
The origin of chondrules and chondrites /
by: Sears, Derek W. G., 1948-
Published: (2004) -
Large Carbonaceous Chondrite Parent Bodies Favored by Abundance–Volatility Modeling: A Possible Chemical Signature of Pebble Accretion
by: Jeremy W. Boyce, et al.
Published: (2024-01-01) -
Reproduction Experiments of Radial Pyroxene Chondrules Using a Gas-jet Levitation System under Reduced Conditions
by: Kana Watanabe, et al.
Published: (2024-01-01) -
Bubbles to Chondrites-II. Chemical fractionations in chondrites
by: Akihiko Hashimoto, et al.
Published: (2021-01-01)