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Tidally heated moons: from icy worlds to temperate habitats

机译:被加热的卫星:从冰冷的世界到温带栖息地

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Moons of giant planets may represent an alternative to the classical picture of habitable worlds. Within our own solar system Europa has long served as an intriguing candidate for a subsurface liquid water ocean. Sustained by tidal heating, such an ocean can exist well beyond the range at which stellar heating could raise surface temperatures to similar levels. For exoplanets, with their extraordinarily diverse orbital architectures, the same situation may arise, along with a host of other possibilities - including those where a combination of tidal and stellar heating results in water rich moons experiencing temperate surface conditions. The next generation of space-based planet finders and ground based large telescopes should begin to probe the population of moons around exoplanets - thereby opening up a new avenue in the search for life. We discuss some of these possibilities by investigating the dynamical constraints on moon systems of giant planets and by studying the characteristics of a set of 74 known extrasolar giant planets located beyond 0.6 AU from their parent stars - where moons should be long-lived with respect to removal by stellar tides. By estimating the stellar insolation that moons would experience for these exoplanet systems, and the implications for sublimation loss of volatiles, we find that between 15 and 27% of all known exoplanets may be capable of harboring small, icy, moons. In addition, by applying a simplified energy balance model, we find that some 22-28% of all known exoplanets could potentially harbor moons which, if large, could experience temperate surface conditions due to a combination of tidal and stellar heating. Large moons (0.1M?), at orbital radii commensurate with those of the Galilean satellites, could maintain temperate, or habitable, surface conditions during episodes of tidal heat dissipation ranging from that seen on Europa to 10-100 times greater. We discuss the implications of these findings in the context of habitability.
机译:巨大行星的卫星可以代表居住世界古典图景的替代品。在我们自己的太阳系中,Europa长期以来一直作为地下液体水域的兴趣候选人。通过潮汐加热持续,这种海洋可以远远超过恒星加热可以将表面温度提高到类似水平的范围。对于外产的轨道架构,可能出现同样的情况,以及一系列其他可能性 - 包括那些潮汐和恒星加热的组合在经历温带水平的水域中的水合。下一代基于太空的行星取景器和地面的大型望远镜应开始探讨绵延的卫星群体 - 从而在寻求寿命中开辟了新的大道。我们通过研究巨型行星月球系统的动态约束以及研究一组74个已知的额外巨型行星的动态约束来讨论一些这些可能性,从他们的父母星星中研究了超过0.6 Au的74个已知的extrasolar巨型行星 - 其中卫星应该长期存在恒星潮汐删除。通过估计Moons将对这些外产系统进行体验的恒星缺失,以及对挥发物的升华丧失的影响,发现15至27%的所有已知的外产上产能够覆盖小,冰冷的卫星。此外,通过应用简化的能量平衡模型,我们发现约有22-28%的所有已知的外产上产品可能会潜在港口沉船,如果大,则可能由于潮汐和恒星加热的组合而体验温带表面状况。在与伽利略卫星的轨道半径相称,大卫星(0.1米?)可以在潮汐散热过程中保持温带,或可居所,表面条件,从而从欧罗巴上观察到10-100倍。我们讨论了这些发现在居住地上的影响。

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