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A paucity of proto-hot Jupiters on super-eccentric orbits
Rebekah I. Dawson, Ruth A. Murray-Clay, John Asher Johnson
Gas giant planets orbiting within 0.1 AU of their host stars, unlikely to have formed in situ, are evidence for planetary migration. It is debated whether the typical hot Jupiter s…
The Photoeccentric Effect and Proto-Hot Jupiters II. KOI-1474.01, a candidate eccentric planet perturbed by an unseen companion
Rebekah I. Dawson, John Asher Johnson, Timothy D. Morton +4
The exoplanets known as hot Jupiters---Jupiter-sized planets with periods less than 10 days---likely are relics of dynamical processes that shape all planetary system architectures…
The Photoeccentric Effect and Proto-Hot Jupiters I. Measuring photometric eccentricities of individual transiting planets
Rebekah I. Dawson, John Asher Johnson
Exoplanet orbital eccentricities offer valuable clues about the history of planetary systems. Eccentric, Jupiter-sized planets are particularly interesting: they may link the "cold…
Neptune's wild days: constraints from the eccentricity distribution of the classical Kuiper Belt
Rebekah I. Dawson, Ruth Murray-Clay
Neptune's dynamical history shaped the current orbits of Kuiper belt objects (KBOs), leaving clues to the planet's orbital evolution. In the "classical" region, a population of dyn…