A New Analysis of 8 Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b
Erin May, Kevin Stevenson, Jacob Bean, Taylor Bell, Nicolas Cowan,, Lisa Dang, Jean-Michel Desert, Jonathan Fortney, Dylan Keating, Eliza, Kempton, Thaddeus Komacek, Nikole Lewis, Megan Mansfield, Caroline Morley,, Vivien Parmentier, Emily Rauscher, Mark Swain, Robert Zellem

TL;DR
This study analyzes multiple Spitzer phase curves of hot Jupiters to identify trends in atmospheric heat redistribution and hot spot offsets, revealing potential classifications and dependencies related to orbital period, temperature, and gravity.
Contribution
It provides a uniform reanalysis of seven new and existing Spitzer phase curves, revealing new trends and classifications in hot Jupiter atmospheric properties.
Findings
Hot spot offset increases with orbital period.
Evidence for two classes of planets based on redistribution and temperature.
Tentative correlation between hot spot offset and planetary surface gravity.
Abstract
With over 30 phase curves observed during the warm Spitzer mission, the complete data set provides a wealth of information relating to trends and three-dimensional properties of hot Jupiter atmospheres. In this work we present a comparative study of seven new Spitzer phase curves for four planets with equilibrium temperatures of T 1300K: Qatar-2b, WASP-52b, WASP-34b, and WASP-140b, as well as the reanalysis of the 4.5 Qatar-1b phase curve due to the similar equilibrium temperature. In total, five 4.5 phase curves and three 3.6 phase curves are analyzed here with a uniform approach. Using these new results, in combination with literature values for the entire population of published Spitzer phase curves of hot Jupiters, we present evidence for a linear trend of increasing hot spot offset with increasing orbital period, as well as observational…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Scientific Research and Discoveries
