Spitzer observations of the thermal emission from WASP-43b
Jasmina Blecic, Joseph Harrington, Nikku Madhusudhan, Kevin B., Stevenson, Ryan A. Hardy, Patricio E. Cubillos, Matthew Hardin, Sarah, Nymeyer, David R. Anderson, Coel Hellier, Alexis M. S. Smith, Andrew, Collier Cameron

TL;DR
This study uses Spitzer observations to measure the thermal emission of WASP-43b, refining its orbital parameters and constraining its atmospheric composition, indicating no strong thermal inversion and low energy redistribution.
Contribution
First detailed infrared measurements of WASP-43b's thermal emission, improving orbital period estimates and constraining atmospheric models without thermal inversion.
Findings
Eclipse depths at 3.6 and 4.5 μm measured
Orbital period refined by a factor of three
No evidence for strong thermal inversion
Abstract
WASP-43b is one of the closest-orbiting hot Jupiters, with a semimajor axis of a = 0.01526 +/- 0.00018 AU and a period of only 0.81 days. However, it orbits one of the coolest stars with a hot Jupiter (Tstar = 4520 +/- 120 K), giving the planet a modest equilibrium temperature of Teq = 1440 +/- 40 K, assuming zero Bond albedo and uniform planetary energy redistribution. The eclipse depths and brightness temperatures from our jointly fit model are 0.347% +/- 0.013% and 1670 +/- 23 K at 3.6 {\mu}m and 0.382% +/- 0.015% and 1514 +/- 25 K at 4.5 {\mu}m. The eclipse timings improved the estimate of the orbital period, P, by a factor of three (P = 0.81347436 +/- 1.4*10-7 days) and put an upper limit on the eccentricity (e = 0.010+0.010 -0.007). We use our Spitzer eclipse depths along with four previously reported ground-based photometric observations in the near-infrared to constrain the…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Astronomy and Astrophysical Research · Spacecraft and Cryogenic Technologies
