Scientists have characterised wind and cloud patterns of the night side of planet Venus for the first time, and found that it behaves very differently from the part facing the Sun.
The night side exhibits unexpected and previously-unseen cloud types, morphologies, and dynamics - some of which appear to be connected to features on the planet's surface.
This is the first time humans have been able to characterise how the atmosphere circulates on the night side of Venus on a global scale.
Scientists found that the cloud patterns there are different to those on the dayside, and influenced by Venus' topography on the dark side.
Venus' atmosphere is dominated by strong winds that whirl around the planet far faster than Venus itself rotates.
This phenomenon, known as 'super-rotation', sees Venusian winds rotating up to 60 times faster than the planet below, pushing and dragging along clouds within the atmosphere as they go.
These clouds travel fastest at the upper cloud level, some 65 to 72 kilometres above the surface.
The team used the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on European Space Agency (ESA)'s Venus Express spacecraft to observe the clouds in the infrared.
VIRTIS enabled scientists to see these clouds properly for the first time, allowing them to explore what previous teams could not and we discovered unexpected and surprising results.
Rather than capturing single images, VIRTIS gathered a 'cube' of hundreds of images of Venus acquired simultaneously at different wavelengths.
This allowed the team to combine numerous images to improve the visibility of the clouds, and see them at unprecedented quality.
The VIRTIS images thus reveal phenomena on Venus' night side that have never before been seen on the dayside.
