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A Catalog of Spectra, Albedos, and Colors of Solar System Bodies for Exoplanet Comparison

机译:用于系外行星比较的光谱,反照率和太阳系主体颜色的目录

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We present a catalog of spectra and geometric albedos, representative of the different types of solar system bodies, from 0.45 to 2.5 mu m. We analyzed published calibrated, uncalibrated spectra, and albedos for solar system objects and derived a set of reference spectra and reference albedos for 19 objects that are representative of the diversity of bodies in our solar system. We also identified previously published data that appear contaminated. Our catalog provides a baseline for comparison of exoplanet observations to 19 bodies in our own solar system, which can assist in the prioritization of exoplanets for time intensive follow-up with next-generation extremely large telescopes and space-based direct observation missions. Using high- and low-resolution spectra of these solar system objects, we also derive colors for these bodies and explore how a color-color diagram could be used to initially distinguish between rocky, icy, and gaseous exoplanets. We explore how the colors of solar system analog bodies would change when orbiting different host stars. This catalog of solar system reference spectra and albedos is available for download through the Carl Sagan Institute.
机译:我们提供了一个光谱和几何反照率的目录,代表了从0.45到2.5微米的不同类型的太阳系物体。我们分析了已发布的校准过的,未校准过的光谱和太阳系天体的反照率,并得出了一组代表19个物体的参考光谱和参考反照率,它们代表了我们太阳系中物体的多样性。我们还确定了以前发布的看起来受污染的数据。我们的目录为比较系外行星观测与我们自己太阳系中的19个天体提供了基线,这可以帮助对系外行星进行优先排序,以进行下一代超大型望远镜和空基直接观察任务的时间密集型后续行动。利用这些太阳系物体的高分辨率和低分辨率光谱,我们还可以得出这些物体的颜色,并探索如何使用彩色图表初步区分岩石系,冰系和气态系外行星。我们探索了绕着不同的恒星运行时,太阳系类似物体的颜色将如何变化。该太阳系参考光谱和反照率目录可通过卡尔·萨根研究所下载。

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