Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Elishevah M M E Van Kooten"'
Autor:
Giulia Perotti, Henning O. Sørensen, Henning Haack, Anja C. Andersen, Dario Ferreira Sanchez, Elishevah M. M. E. van Kooten, Esther H. R. Tsai, Kim N. Dalby, Mirko Holler, Daniel Grolimund, Tue Hassenkam
Publikováno v:
Perotti, G, Sorensen, H O, Haack, H, Andersen, A C, Sanchez, D F, Van Kooten, E M M E, Tsai, E H R, Dalby, K N, Holler, M, Grolimund, D & Hassenkam, T 2021, ' Thermal History of Matrix Forsterite Grains from Murchison Based on High-resolution Tomography ', Astrophysical Journal, vol. 922, no. 2, 256 . https://doi.org/10.3847/1538-4357/ac26bc
Protoplanetary disks are dust- and gas-rich structures surrounding protostars. Depending on the distance from the protostar, this dust is thermally processed to different degrees and accreted to form bodies of varying chemical compositions. The primo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cbef14ae4a58deaec0b6af44dd87b0f
http://arxiv.org/abs/2109.06942
http://arxiv.org/abs/2109.06942
Publikováno v:
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta, Elsevier, 2019, 261, pp.248-268. ⟨10.1016/j.gca.2019.07.022⟩
Geochimica et Cosmochimica Acta, 2019, 261, pp.248-268. ⟨10.1016/j.gca.2019.07.022⟩
Geochimica et Cosmochimica Acta, Elsevier, 2019, 261, pp.248-268. ⟨10.1016/j.gca.2019.07.022⟩
Geochimica et Cosmochimica Acta, 2019, 261, pp.248-268. ⟨10.1016/j.gca.2019.07.022⟩
The potential complementarity between chondrules and matrix of chondrites, the Solar System's building blocks, is still a highly debated subject. Complementary superchrondritic compositions of chondrite matrices and subchondritic chondrules may point
Autor:
Martin Bizzarro, Elishevah M. M. E. van Kooten, Anders Johansen, Martin Schiller, Frédéric Moynier, Troels Haugbølle
Publikováno v:
The Astrophysical Journal
van Kooten, E, Schiller, M, Moynier, F, Johansen, A, Haugbolle, T & Bizzarro, M 2021, ' Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier ', Astrophysical Journal, vol. 910, no. 1, 70 . https://doi.org/10.3847/1538-4357/abd9c8
van Kooten, E, Schiller, M, Moynier, F, Johansen, A, Haugbolle, T & Bizzarro, M 2021, ' Hybrid Accretion of Carbonaceous Chondrites by Radial Transport across the Jupiter Barrier ', Astrophysical Journal, vol. 910, no. 1, 70 . https://doi.org/10.3847/1538-4357/abd9c8
Understanding the origin of chondritic components and their accretion pathways is critical to unravel the magnitude of mass transport in the protoplanetary disk, the accretionary history of the terrestrial planet region and, by extension, its prebiot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2e0d6a8a2dd7f87ff2975c173e4aaf7
http://arxiv.org/abs/2103.02393
http://arxiv.org/abs/2103.02393
Publikováno v:
Earth and Planetary Science Letters
Earth and Planetary Science Letters, Elsevier, 2020, 546, pp.116418. ⟨10.1016/j.epsl.2020.116418⟩
Earth and Planetary Science Letters, Elsevier, 2020, 546, pp.116418. ⟨10.1016/j.epsl.2020.116418⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3b24f4f59a9308f6fb7a4a86ab8815c1
https://hal-insu.archives-ouvertes.fr/insu-02916147
https://hal-insu.archives-ouvertes.fr/insu-02916147
Autor:
Jean-Alix Barrat, Frédéric Moynier, Ke Zhu, D. Wielandt, K. K. Larsen, Martin Schiller, Martin Bizzarro, Elishevah M. M. E. van Kooten
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2020, 888 (2), pp.126. ⟨10.3847/1538-4357/ab5af7⟩
The Astrophysical Journal, American Astronomical Society, 2020, 888 (2), pp.126. ⟨10.3847/1538-4357/ab5af7⟩
We report on the mass-independent Cr isotope compositions of 11 main group ureilites and an ureilitic trachyandesite (ALM-A). The 54Cr/52Cr ratios for main group ureilites vary from −1.06±0.04 to −0.78±0.05 and averaged at −0.91±0.15 (2SD, N
Publikováno v:
Meteoritics and Planetary Science
Meteoritics and Planetary Science, Wiley, 2020, 55 (3), pp.575-590. ⟨10.1111/maps.13459⟩
van Kooten, E, Cavalcante, L & Bizzarro, M 2020, ' The role of Bells in the continuous accretion between the CM and CR chondrite reservoirs ', Meteoritics and Planetary Science, vol. 55, no. 3, pp. 575-590 . https://doi.org/10.1111/maps.13459
Meteoritics & Planetary Science
Meteoritics and Planetary Science, Wiley, 2020, 55 (3), pp.575-590. ⟨10.1111/maps.13459⟩
van Kooten, E, Cavalcante, L & Bizzarro, M 2020, ' The role of Bells in the continuous accretion between the CM and CR chondrite reservoirs ', Meteoritics and Planetary Science, vol. 55, no. 3, pp. 575-590 . https://doi.org/10.1111/maps.13459
Meteoritics & Planetary Science
CM meteorites are dominant members of carbonaceous chondrites (CCs), which evidently accreted in a region separated from the terrestrial planets. These chondrites are key in determining the accretion regions of solar system materials, since in Mg and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54e7e35bf8ff1b79c1114d822e90479a
https://hal-insu.archives-ouvertes.fr/insu-02619042/document
https://hal-insu.archives-ouvertes.fr/insu-02619042/document
Publikováno v:
Earth and Planetary Science Letters
Isotopic compositions of reservoirs in the Moon can be constrained from analysis of rocks generated during lunar magmatic differentiation. Mare basalts sample the largest lunar mantle volume, from olivine- and pyroxene-rich cumulates, whereas ferroan
Publikováno v:
Geochimica et Cosmochimica Acta. 201:185-223
We report on the mineralogy, petrography, and O-isotope compositions of ∼60 Ca, Al-rich inclusions (CAIs) incompletely melted during formation of porphyritic chondrules from the CH metal-rich carbonaceous chondrites and Isheyevo (CH/CB). These incl
Publikováno v:
Geochimica et Cosmochimica Acta. 201:155-184
We describe the mineralogy, petrology and oxygen isotopic compositions of high-temperature rims around mineralogically pristine calcium–aluminum-rich inclusions (CAIs) from the CR, CB and CH carbonaceous chondrites. In CR chondrites, nearly all CAI