Here, we 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.
Schrader, Devin L., et al. "Tarda and Tagish Lake: Samples from the same outer Solar System asteroid and implications for D- and P-type asteroids." Geochimica et Cosmochimica Acta, vol. 380, Sep. 2024. https://doi.org/10.1016/j.gca.2024.07.007
Schrader, Devin L., Cloutis, Edward A., Applin, Daniel M., Davidson, Jemma, Torrano, Zachary A., Foustoukos, Dionysis, Alexander, Conel O'D., Domanik, Kenneth J., Matsuoka, Moe, Nakamura, Tomoki, Zega, Thomas J., Brennecka, Gregory A., & Render, Jan (2024). Tarda and Tagish Lake: Samples from the same outer Solar System asteroid and implications for D- and P-type asteroids. Geochimica et Cosmochimica Acta, 380. https://doi.org/10.1016/j.gca.2024.07.007
Schrader, Devin L., Cloutis, Edward A., Applin, Daniel M., et al., "Tarda and Tagish Lake: Samples from the same outer Solar System asteroid and implications for D- and P-type asteroids," Geochimica et Cosmochimica Acta 380 (2024), https://doi.org/10.1016/j.gca.2024.07.007
@article{osti_2406137,
author = {Schrader, Devin L. and Cloutis, Edward A. and Applin, Daniel M. and Davidson, Jemma and Torrano, Zachary A. and Foustoukos, Dionysis and Alexander, Conel O'D. and Domanik, Kenneth J. and Matsuoka, Moe and Nakamura, Tomoki and others},
title = {Tarda and Tagish Lake: Samples from the same outer Solar System asteroid and implications for D- and P-type asteroids},
annote = {Here, we 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.},
doi = {10.1016/j.gca.2024.07.007},
url = {https://www.osti.gov/biblio/2406137},
journal = {Geochimica et Cosmochimica Acta},
issn = {ISSN 0016-7037},
volume = {380},
place = {United States},
publisher = {Elsevier; The Geochemical Society; The Meteoritical Society},
year = {2024},
month = {09}}