Zobrazeno 1 - 10
of 141
pro vyhledávání: '"Marc M. Hirschmann"'
Autor:
Avishek Rudra, Marc M. Hirschmann
Publikováno v:
Geochimica et Cosmochimica Acta. 328:258-279
Autor:
Marc M. Hirschmann
Publikováno v:
Geochimica et Cosmochimica Acta. 313:74-84
We present thermodynamic and empirical calculations for the iron-wustite (IW) buffer applicable from 100 kPa to 100 GPa and from 1000 to 3000 K. The thermodynamic calculation self-consistently accounts for changing stoichiometry of iron-saturated wus
Publikováno v:
Geochimica et Cosmochimica Acta. 265:32-47
To better understand the solution of volatile species in a reduced magma ocean, we identify via Raman spectroscopy the nature of C-O-H-N volatile species dissolved in a series of reduced basaltic glasses. The oxygen fugacity (ƒO2) during synthesis v
Publikováno v:
Earth and Planetary Science Letters. 520:164-174
To better understand the role of sulfide in C storage in the upper mantle, we construct a thermodynamic model for Fe-Ni-S-C sulfide melts and consider equilibrium between sulfide melts, mantle silicates, Fe-Ni alloy, and diamond. The sulfide melt mod
Publikováno v:
Eos, Transactions American Geophysical Union
Eos, Transactions American Geophysical Union, American Geophysical Union (AGU), 2021, 102, ⟨10.1029/2021EO159473⟩
Eos, Transactions American Geophysical Union, 2021, 102, ⟨10.1029/2021EO159473⟩
Eos, Transactions American Geophysical Union, American Geophysical Union (AGU), 2021, 102, ⟨10.1029/2021EO159473⟩
Eos, Transactions American Geophysical Union, 2021, 102, ⟨10.1029/2021EO159473⟩
International audience; “Cousin” worlds—slightly bigger or slightly hotter than Earth—can help us understand planetary habitability, but we need more lab and numerical experiments to make the most of this opportunity.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebf7e13be5414bca443fd2a0cc4846fd
https://hal.archives-ouvertes.fr/hal-03408627
https://hal.archives-ouvertes.fr/hal-03408627
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America
During the formation of terrestrial planets, volatile loss may occur through nebular processing, planetesimal differentiation, and planetary accretion. We investigate iron meteorites as an archive of volatile loss during planetesimal processing. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::15694bf056458da79c1ec8e34d62a316
http://arxiv.org/abs/2104.02706
http://arxiv.org/abs/2104.02706
Autor:
Timothy W. Lyons, Hilairy E. Hartnett, Laura Kreidberg, Giada Arney, Stephen R. Kane, Michael J. Way, Martha S. Gilmore, Bradford J. Foley, Noam R. Izenberg, Christopher T. Reinhard, Joe P. Renaud, Paul K. Byrne, Kanani K. M. Lee, Ariel D. Anbar, Edward W. Schwieterman, Edwin S. Kite, W. G. Henning, Wendy R. Panero, David Brain, S. J. Desch, Cayman T. Unterborn, Marc M. Hirschmann, L. E. Sohl, Laura Schaefer, Elizabeth J. Tasker, Noah J. Planavsky
Publikováno v:
Bulletin of the AAS, vol 53, iss 4
Publikováno v:
Goldschmidt2021 abstracts.
Autor:
Marc M. Hirschmann
Publikováno v:
Goldschmidt2021 abstracts.
Publikováno v:
Science advances. 7(14)
Carbon is an essential element for life but its behavior during Earth's accretion is not well understood. Carbonaceous grains in meteoritic and cometary materials suggest that irreversible sublimation, and not condensation, governs carbon acquisition