Zobrazeno 1 - 10
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pro vyhledávání: '"formation, planets and satellites"'
Akademický článek
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Akademický článek
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Publikováno v:
Zhu, K, Becker, H, Li, S J, Fan, Y, Liu, X N & Elliott, T 2022, ' Radiogenic chromium isotope evidence for the earliest planetary volcanism and crust formation in the Solar system ', Monthly Notices of the Royal Astronomical Society: Letters, vol. 515, no. 1, pp. L39-L44 . https://doi.org/10.1093/mnrasl/slac061
Erg Chech (EC) 002 is a meteorite with andesitic composition, potentially recording the lava crystallization and crust formation of its parent body. Nucleosynthetic Cr isotope composition (ε54Cr = −0.35 ± 0.06) for EC 002 suggests a non-carbonace
Autor:
E. Fernández-Valenzuela, N. Morales, M. Vara-Lubiano, J. L. Ortiz, G. Benedetti-Rossi, B. Sicardy, M. Kretlow, P. Santos-Sanz, B. Morgado, D. Souami, F. Organero, L. Ana, F. Fonseca, A. Román, S. Alonso, R. Gonçalves, M. Ferreira, R. Iglesias-Marzoa, J. L. Lamadrid, A. Alvarez-Candal, M. Assafin, F. Braga-Ribas, J. I. B. Camargo, F. Colas, J. Desmars, R. Duffard, J. Lecacheux, A. R. Gomes-Júnior, F. L. Rommel, R. Vieira-Martins, C. L. Pereira, V. Casanova, A. Selva, C. Perelló, S. Mottola, S. Hellmich, J. L. Maestre, A. J. Castro-Tirado, A. Pal, J. M. Trigo-Rodriguez, W. Beisker, A. Laporta, M. Garcés, L. Escaned, M. Bretton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2023, 669, pp.A112. ⟨10.1051/0004-6361/202243214⟩
Astronomy and Astrophysics-A&A, 2023, 669, pp.A112. ⟨10.1051/0004-6361/202243214⟩
Within our program of physical characterization of trans-Neptunian objects and centaurs, we predicted a stellar occultation by the centaur (54598) Bienor to occur on January 11, 2019, with good observability potential. We obtained high accuracy astro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f04abb1eb2175631ceb9b5b637aab6bc
http://hdl.handle.net/10261/308511
http://hdl.handle.net/10261/308511
Publikováno v:
Johansen, A, Ronnet, T, Schiller, M, Deng, Z & Bizzarro, M 2023, ' Anatomy of rocky planets formed by rapid pebble accretion : II. Differentiation by accretion energy and thermal blanketing ', Astronomy and Astrophysics, vol. 671, A75 . https://doi.org/10.1051/0004-6361/202142142
We explore the heating and differentiation of rocky planets that grow by rapid pebble accretion. Our terrestrial planets grow outside of the ice line and initially accrete 28\% water ice by mass. The accretion of water stops after the protoplanet rea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ac7c3caf28a17e9b516a0fb266d7d1d5
https://curis.ku.dk/portal/da/publications/anatomy-of-rocky-planets-formed-by-rapid-pebble-accretion(436f25ad-dd05-41bc-9d06-4c4f2e5d67b9).html
https://curis.ku.dk/portal/da/publications/anatomy-of-rocky-planets-formed-by-rapid-pebble-accretion(436f25ad-dd05-41bc-9d06-4c4f2e5d67b9).html
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2023, 674, ⟨10.1051/0004-6361/202245763⟩
Astronomy & Astrophysics, 674
Astronomy and Astrophysics-A&A, 2023, 674, ⟨10.1051/0004-6361/202245763⟩
Astronomy & Astrophysics, 674
Context. Ultrahot (>1500 K) rocky exoplanets may be covered by a magma ocean, resulting in the formation of a vapor rich in rocky components (e.g., Mg, Si, Fe) with a low total pressure and high molecular mass. However, exoplanets may have also captu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd841645c6d5eff70ac760dfe4597104
https://insu.hal.science/insu-04155710/document
https://insu.hal.science/insu-04155710/document
Publikováno v:
Appelgren, J, Lambrechts, M & van der Marel, N 2023, ' Disc population synthesis : Decrease in the solid mass reservoir through pebble drift ', Astronomy & Astrophysics, vol. 673, A139 . https://doi.org/10.1051/0004-6361/202245252
Surveys of star-forming regions reveal that the dust mass of protoplanetary discs decreases by several orders of magnitude on a timescale of a few million years. This decrease in the mass budget of solids is likely due to the gas-drag-induced radial
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9aebff0d1855bb4af9573b71c117726a
https://curis.ku.dk/portal/da/publications/disc-population-synthesis(76571cf3-8c67-4d62-9011-caac0d1b723c).html
https://curis.ku.dk/portal/da/publications/disc-population-synthesis(76571cf3-8c67-4d62-9011-caac0d1b723c).html
Autor:
Iglesias Álvarez, Santiago, Díez Alonso, Enrique, Sánchez, María Luisa, Castro - González, Amadeo, Rodríguez Rodríguez, Javier, Pereira, César Rodríguez
In this work we search and characterize exoplanets orbiting members of stellar streams, which are structures in the Galaxy composed of stars with similar dynamic and chemical properties, and with galactic or extragalactic origin. With current facilit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::716783709fec82d2b13bcff8d6f1e13c