/ D. Kubyshkina [et al.]> // Astrophys. J. - 2019. -
Vol. 879,
Is. 1. - Ст. 26,
DOI 10.3847/1538-4357/ab1e42. - Cited References:44. - We acknowledge the FFG project P853993, the FWF/NFN projects S11607-N16 and S11604-N16, and the FWF projects P27256-N27 and P30949-N36. N.V.E. acknowledges support from the Russian Science Foundation grant No. 18-12-00080. We thank the anonymous referee for insightful comments.
. - ISSN 0004-637X. - ISSN 1538-4357
РУБ Astronomy & Astrophysics
Аннотация: Planet atmospheric escape induced by high-energy stellar irradiation is a key phenomenon shaping the structure and evolution of planetary atmospheres. Therefore, the present-day properties of a planetary atmosphere are intimately connected with the amount of stellar flux received by a planet during its lifetime, thus with the evolutionary path of its host star. Using a recently developed analytic approximation based on hydrodynamic simulations for atmospheric escape rates, we
track within a Bayesian framework the evolution of a planet as a function of stellar flux evolution history, constrained by the measured planetary radius. We find that the ideal objects for this type of study are close-in sub-Neptune-like planets, as they are highly affected by atmospheric escape, and yet retain a significant fraction of their primordial hydrogen-dominated atmospheres. Furthermore, we apply this analysis to the HD 3167 and K2-32 planetary systems. For HD 3167, we find that the most probable irradiation level at 150 Myr was between 40 and 130 times solar, corresponding to a rotation period of 1.78(-1.23)(+2.69) days. For K2-32, we find a surprisingly low irradiation level ranging between half and four times solar at 150 Myr. Finally, we show that for multi-planet systems, our framework enables one to constrain poorly known properties of individual planets.
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Scopus Держатели документа: Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria.
Russian Acad Sci, Siberian Branch, Inst Computat Modeling, Krasnoyarsk 660036, Russia.
Siberian Fed Univ, Krasnoyarsk 660041, Russia.
Univ Vienna, Inst Astron, Turkenschanzstr 17, A-1180 Vienna, Austria.
Karl Franzens Univ Graz, IGAM Inst Phys, Univ Pl 5, A-8010 Graz, Austria.
Доп.точки доступа: Kubyshkina, D.; Cubillos, P. E.; Fossati, L.; Erkaev, N. V.; Johnstone, C. P.; Kislyakova, K. G.; Lammer, H.; Lendl, M.; Odert, P.; Gudel, M.; Fossati, Luca; FFG project [P853993]; FWF/NFN projects [S11607-N16, S11604-N16]; FWF projects [P27256-N27, P30949-N36]; Russian Science Foundation [18-12-00080]