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Tarda and Tagish Lake: Samples From The Same Outer Solar System Asteroid and Implications for D- and P-Type AsteroidsWe report a comprehensive study of the ungrouped type 2 carbonaceous chondrite, Tarda, which fell in Morocco in 2020. This meteorite exhibits substantial similarities to Tagish Lake, Wisconsin Range 91600, and Meteorite Hills 00432, which are generally considered to have originated from a D-type asteroid(s). We constrain the compositions and petrologies of the materials present in a potential sample of a D-type asteroid by reporting the petrography, bulk chemical compositions, bulk H, C, N, Cr, and Ti isotopic compositions, reflectance spectra, and in situ chemical compositions of metals, sulfides, carbonates, and FeO-poor and FeO-rich chondrule silicates of Tarda. We also present new data for Tagish Lake. We then compare Tarda with the other Tagish Lake-like meteorites.

Tarda and Tagish Lake appear to be from the same parent body, as demonstrated by their similar petrologies (modal abundances, chondrule sizes), mineral compositions, bulk chemical and isotopic compositions, and reflectance spectra. While the two other Tagish Lake-like meteorites, Wisconsin Range 91600 and Meteorite Hills 00432, show some affinities to Tagish Lake and Tarda, they also share similar characteristics to the Mighei-like carbonaceous (CM) chondrites, warranting further study. Similarities in reflectance spectra suggest that P-type asteroids 65 Cybele and 76 Freia are potential parent bodies of Tarda and the Tagish Lake-like meteorites, or at least have similar surface materials. Since upcoming spacecraft missions will spectrally survey D-type, P-type, and C-type Trojan asteroids (NASA's Lucy) and spectrally study and return samples from Mars' moon Phobos (JAXA's Martian Moons eXploration mission), which is spectrally similar to D-type asteroids, these meteorites are of substantial scientific interest. Furthermore, since Tarda closely spectrally matches P-type asteroids (but compositionally matches the D-type asteroid like Tagish Lake meteorite), P-type and D-type asteroids may represent fragments of the same or similar parent bodies.
Document ID
20240008763
Acquisition Source
Johnson Space Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Devin L. Schrader
(Arizona State University Tempe, United States)
Edward A. Cloutis
(University of Winnipeg Winnipeg, Manitoba, Canada)
Daniel M. Applin
(University of Winnipeg)
Jemma Davidson
(Johnson Space Center Houston, United States)
Zachary A. Torrano
(Carnegie Institution for Science Washington, United States)
Dionysis Foustoukos
(Carnegie Institution for Science Washington, United States)
Conel M. O'D. Alexander ORCID
(Carnegie Institution for Science Washington, United States)
Kenneth J. Domanik
(University of Arizona)
Moe Matsuoka ORCID
(Geological Survey of Japan Tsukuba, Japan)
Tomoki Nakamura ORCID
(Tohoku University Sendai, Japan)
Thomas J. Zega
(University of Arizona Tucson, United States)
Gregory A. Brennecka
(Lawrence Livermore National Laboratory Livermore, United States)
Jan Render
(Lawrence Livermore National Laboratory Livermore, United States)
Date Acquired
July 10, 2024
Publication Date
August 30, 2024
Publication Information
Publication: Geochimica et Cosmochimica Acta
Publisher: Elsevier
Volume: 380
Subject Category
Lunar and Planetary Science and Exploration
Funding Number(s)
WBS: 048290.02.01.01.05
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
Tarda
ungrouped chondrite
D-type asteroid
P-type asteroid
Tagish Lake
carbonaceous chondrites
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