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pro vyhledávání: '"J. M. Rodríguez-Mozos"'
Autor:
J. M. Rodríguez-Mozos, A. Moya
For a planet to be considered habitable on its surface, it is an important advantage for it to have a magnetic field that protects its atmosphere from stellar winds as well as cosmic rays. Magnetic protection of potentially habitable planets plays a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6dd391d30ec9d24996109d674fc93e12
http://arxiv.org/abs/2203.01065
http://arxiv.org/abs/2203.01065
Nowadays, we know thousands of exoplanets, some of them potentially habitable. Next technological facilities (JWST, for example) have exoplanet atmosphere analysis capabilities, but they also have limits in terms of how many targets can be studied. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2c1e56b14ef3ad069cb79d90479c20c
Autor:
J. M. Rodríguez-Mozos, A. Moya
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:4628-4636
A new Statistical-likelihood Exo-Planetary Habitability Index (SEPHI) is presented. It has been developed to cover the current and future features required for a classification scheme disentangling whether any discovered exoplanet is potentially habi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::89e3b893fdd2c412a2ffdc059cb560ff
https://doi.org/10.1093/mnras/stx1910
https://doi.org/10.1093/mnras/stx1910
Autor:
J. M. Rodríguez-Mozos, A. Moya
Publikováno v:
Astronomy & Astrophysics
Rodriguez-Mozos, J M & Moya, A 2019, ' Erosion of an exoplanetary atmosphere caused by stellar winds ', Astronomy & Astrophysics, vol. 630, 52 . https://doi.org/10.1051/0004-6361/201935543
Rodriguez-Mozos, J M & Moya, A 2019, ' Erosion of an exoplanetary atmosphere caused by stellar winds ', Astronomy & Astrophysics, vol. 630, 52 . https://doi.org/10.1051/0004-6361/201935543
We present a formalism for a first-order estimation of the magnetosphere radius of exoplanets orbiting stars in the range from 0.08 to 1.3 Mo. With this radius, we estimate the atmospheric surface that is not protected from stellar winds. We have ana
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6f2e46c8fd186a0adf464ab02c676a3