Scientists observe for the first time, winds and cloud patterns on the night side of Venus

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. [caption id=“attachment_2359062” align=“alignleft” width=“380”]  Representational image. AFP[/caption] The night side exhibits unexpected and previously-unseen cloud types, morphologies, and dynamics, some of which appear to be connected to features on the planets surface. “This is the first time we’ve been able to characterise how the atmosphere circulates on the night side of Venus on a global scale,” said Javier Peralta of the Japan Aerospace Exploration Agency (JAXA). “While the atmospheric circulation on the planets dayside has been extensively explored, there was still much to discover about the night side. We found that the cloud patterns there are different to those on the dayside, and influenced by Venus topography,” said Peralta, lead author of the study published in the journal Nature Astronomy. 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.“We’ve spent decades studying these super-rotating winds by tracking how the upper clouds move on Venus dayside. These are clearly visible in images acquired in ultraviolet light,” said Peralta. “However, our models of Venus remain unable to reproduce this super-rotation, which clearly indicates that we might be missing some pieces of this puzzle,” he said. “We focused on the night side because it had been poorly explored; we can see the upper clouds on the planets night side via their thermal emission, but its been difficult to observe them properly because the contrast in our infrared images was too low to pick up enough detail,” he added. The team used the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on European Space Agency’s (ESA) Venus Express spacecraft to observe the clouds in the infrared. “VIRTIS enabled us to see these clouds properly for the first time, allowing us to explore what previous teams could not and we discovered unexpected and surprising results,” adds Peralta. 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