Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights into their atmospheres, but the properties of lower-mass exoplanets (sub-Neptune) remain largely unconstrained because of the challenges of observing small planets. Numerous efforts to observe the spectra of super-Earths—exoplanets with masses of one to ten times that of Earth—have so far revealed only featureless spectra. Here we report a longitudinal thermal brightness map of the nearby transiting super-Earth 55 Cancri e (refs 4, 5) revealing highly asymmetric dayside thermal emission and a strong day–night temperature contrast. Dedicated space-based monitoring of the planet in the infrared revealed a modulation of the thermal flux as 55 Cancr...
Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Considerable progress has been made in recent years in observations of atmospheric signatures of gia...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
'Hot Jupiter' extrasolar planets are expected to be tidally locked because they are close (<0.05 ast...
'Hot Jupiter' extrasolar planets are expected to be tidally locked because they are close (<0.05 ast...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
We report on the detection of infrared light from the super-Earth 55 Cnc e, based on four occultatio...
Exoplanets that orbit close to their host stars are much more highly irradiated than their solar sys...
Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun...
Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights int...
Considerable progress has been made in recent years in observations of atmospheric signatures of gia...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
'Hot Jupiter' extrasolar planets are expected to be tidally locked because they are close (<0.05 ast...
'Hot Jupiter' extrasolar planets are expected to be tidally locked because they are close (<0.05 ast...
One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whe...
We report on the detection of infrared light from the super-Earth 55 Cnc e, based on four occultatio...
Exoplanets that orbit close to their host stars are much more highly irradiated than their solar sys...
Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun...
Most known terrestrial planets orbit small stars with radii less than 60 per cent of that of the Sun...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...
The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest t...