Re-evaluating the Very Hot Gas Giant WASP-12b
Re-evaluating the Very Hot Gas Giant WASP-12b
Re-evaluating the Very Hot Gas Giant WASP-12b
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Campo+2011<br />
Cowan+2012<br />
4.5µm Eclipses of <strong>WASP</strong>-<strong>12b</strong>:<br />
0.382 ± 0.019 %<br />
A consistent analysis of all Spitzer data,<br />
and fur<strong>the</strong>r measurements, are called for!<br />
0.39 ± 0.03 %<br />
(very prolate planet)<br />
Or<br />
0.50 ± 0.04 %<br />
(non-prolate planet)<br />
14