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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

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