Modeling Exoplanets with Thick Cloud Layers

Planetary modelers have been particularly puzzled by some of the latest observations of the only multi-planet system that has been directly imaged so far, HR 8799. The photometry of the HR 8799 planets showed that these planets look much redder in color than can be explained by the classic brown dwarf models, suggesting a need for thick iron or silicate cloud layers in exoplanetary atmospheres.

Dip-Detection in the Kepler Data

Dip-Detection in the Kepler Data

Following the data release, a slew of Kepler papers went up on astro-ph this evening. In my previous post, I went straight to the numbers, but here I’ll discuss the Kepler mission and data in some depth, which I think will generally be useful for understanding current and future Kepler results.