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Radiogenic chromium isotope evidence for the earliest planetary volcanism and crust formation in the Solar system

Autor: Ke Zhu, Harry Becker, Shi-Jie Li, Yan Fan, Xiao-Ning Liu, Tim Elliott

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d93630532d63a702a2701344d0ebda7f
https://doi.org/10.1093/mnrasl/slac061

Lightning-induced chemistry on tidally-locked Earth-like exoplanets

Autor: Marrick Braam, Paul I Palmer, Leen Decin, Robert J Ridgway, Maria Zamyatina, Nathan J Mayne, Denis E Sergeev, N Luke Abraham

Publikováno v: Braam, M, Palmer, P I, Decin, L, Ridgway, R J, Zamyatina, M, Mayne, N J, Sergeev, D E & Abraham, N L 2022, ' Lightning-induced chemistry on tidally-locked Earth-like exoplanets ', Monthly Notices of the Royal Astronomical Society, vol. 517, no. 2, pp. 2383–2402 . https://doi.org/10.1093/mnras/stac2722

Determining the habitability and interpreting atmospheric spectra of exoplanets requires understanding their atmospheric physics and chemistry. We use a 3-D Coupled Climate-Chemistry Model, the Met Office Unified Model with the UK Chemistry and Aeros

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::75d1bc0baae4ec6e5f0673e31c2beab8
https://hdl.handle.net/20.500.11820/f98643df-ed84-4fa3-b543-f918282fb409

Large Interferometer For Exoplanets (LIFE)

Autor: Quanz, S. P., Ottiger, M., Fontanet, E., Kammerer, J., Menti, F., Dannert, F., Gheorghe, A., Absil, O., Airapetian, V. S., Alei, E., Allart, R., Angerhausen, D., Blumenthal, S., Buchhave, L. A., Cabrera, J., Carrión-González, Ó., Chauvin, G., Danchi, W. C., Dandumont, C., Defrére, D., Dorn, C., Ehrenreich, D., Ertel, S., Fridlund, M., García Muñoz, A., Gascón, C., Girard, J. H., Glauser, A., Grenfell, J. L., Guidi, G., Hagelberg, J., Helled, R., Ireland, M. J., Janson, M., Kopparapu, R. K., Korth, J., Kozakis, T., Kraus, S., Léger, A., Leedjärv, L., Lichtenberg, T., Lillo-Box, J., Linz, H., Liseau, R., Loicq, J., Mahendra, V., Malbet, F., Mathew, J., Mennesson, B., Meyer, M. R., Mishra, L., Molaverdikhani, K., Noack, L., Oza, A. V., Pallé, E., Parviainen, H., Quirrenbach, A., Rauer, H., Ribas, I., Rice, M., Romagnolo, A., Rugheimer, S., Schwieterman, E. W., Serabyn, E., Sharma, S., Stassun, K. G., Szulágyi, J., Wang, H. S., Wunderlich, F., Wyatt, M. C., Collaboration, the LIFE

Publikováno v: Quanz, S P, Ottiger, M, Fontanet, E, Kammerer, J, Menti, F, Dannert, F, Gheorghe, A, Absil, O, Airapetian, V S, Alei, E, Allart, R, Angerhausen, D, Blumenthal, S, Buchhave, L A, Cabrera, J, Carrión-González, Ó, Chauvin, G, Danchi, W C, Dandumont, C, Defrére, D, Dorn, C, Ehrenreich, D, Ertel, S, Fridlund, M, García Muñoz, A, Gascón, C, Girard, J H, Glauser, A, Grenfell, J L, Guidi, G, Hagelberg, J, Helled, R, Ireland, M J, Janson, M, Kopparapu, R K, Korth, J, Kozakis, T, Kraus, S, Léger, A, Leedjärv, L, Lichtenberg, T, Lillo-Box, J, Linz, H, Liseau, R, Loicq, J, Mahendra, V, Malbet, F, Mathew, J, Mennesson, B, Meyer, M R, Mishra, L, Molaverdikhani, K, Noack, L, Oza, A V, Pallé, E, Parviainen, H, Quirrenbach, A, Rauer, H, Ribas, I, Rice, M, Romagnolo, A, Rugheimer, S, Schwieterman, E W, Serabyn, E, Sharma, S, Stassun, K G, Szulágyi, J, Wang, H S, Wunderlich, F, Wyatt, M C & Collaboration, T LIFE 2022, ' Large Interferometer For Exoplanets (LIFE) ', Astronomy and Astrophysics, vol. 664, A21 . https://doi.org/10.1051/0004-6361/202140366

Context. One of the long-term goals of exoplanet science is the atmospheric characterization of dozens of small exoplanets in order to understand their diversity and search for habitable worlds and potential biosignatures. Achieving this goal require

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1202::97ae27b4363b62546edcbc55e7a06576
https://orbit.dtu.dk/en/publications/99e7cc47-6f91-4ad4-b2b2-df8e8229210e

Observability of evaporating lava worlds

Autor: Zilinskas, M., Buchem, C.P.A. van, Miguel, Y., Louca, A., Lupu, R., Zieba, S., Westrenen, W. van

Publikováno v: Astronomy and Astrophysics, 661:A126, 1-14. EDP Sciences
Zilinskas, M, Van Buchem, C P A, Miguel, Y, Louca, A, Lupu, R, Zieba, S & Van Westrenen, W 2022, ' Observability of evaporating lava worlds ', Astronomy and Astrophysics, vol. 661, A126, pp. 1-14 . https://doi.org/10.1051/0004-6361/202142984
Bulletin of the American Astronomical Society, 503.05. Washington: AAS Publishing
ISSUE=5;STARTPAGE=503.05;TITLE=Bulletin of the American Astronomical Society
Astronomy & Astrophysics, 661:A126

Lava worlds belong to a class of short orbital period planets reaching dayside temperatures high enough to melt their silicate crust. Theory predicts that the resulting lava oceans outgas their volatile components, attaining equilibrium with the over

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5eaf12306f2c413ec025b147d22ceb79
https://hdl.handle.net/1887/3515449