Hot Jupiters are a class of extrasolar planet that orbit their parent stars at very short distances and are expected to be tidally locked, which can lead to a large temperature difference between the dayside and the nightside. Here, the day–night contrast of the transiting extrasolar planet HD 188733b is 'mapped' using infrared observations; the data are consistent with the nightside hemisphere being entirely black, with the dayside flux dominating the optical phase curve.
- Ignas A. G. Snellen
- Ernst J. W. de Mooij
- Simon Albrecht