论文标题
从内而外的巨型行星
Giant Planets from the Inside-Out
论文作者
论文摘要
巨型行星在行星系统的早期地层阶段获得气体，冰和岩石，从而告知我们编队过程本身。从内而外进行，研究深度内部和可观察到的气氛之间的联系，将太阳系中巨型行星的详细测量与棕矮星和巨型系外行星的大量数据联系起来，我们旨在为这些行星形成模型的室内结构和组成提供全球限制。朱诺和卡西尼任务之后的新事态发展指出，木星和土星具有强大的组成梯度和从大气到深层内部的稳定区域。基于这些行星的可用数据，天王星和海王星也是如此。巨型系外行星和棕色矮人为我们提供了新的机会，可以将大气丰度与散装，内部丰度\ rev {并将这些丰度和同位素比的融合到地层场景联系起来。分析可用数据的财富}将需要新的模型，以说明行星内部和气氛的复杂性
Giant planets acquire gas, ices and rocks during the early formation stages of planetary systems and thus inform us on the formation process itself. Proceeding from inside out, examining the connections between the deep interiors and the observable atmospheres, linking detailed measurements on giant planets in the solar system to the wealth of data on brown dwarfs and giant exoplanets, we aim to provide global constraints on interiors structure and composition for models of the formation of these planets. New developments after the Juno and Cassini missions point to both Jupiter and Saturn having strong compositional gradients and stable regions from the atmosphere to the deep interior. This is also the case of Uranus and Neptune, based on available, limited data on these planets. Giant exoplanets and brown dwarfs provide us with new opportunities to link atmospheric abundances to bulk, interior abundances \rev{and to link these abundances and isotopic ratios to formation scenarios. Analysing the wealth of data becoming available} will require new models accounting for the complexity of the planetary interiors and atmospheres
