Mysterious Haze Found on Venus
Venus’s atmosphere, taken by the Venus Monitoring Camera (VMC) during Venus Express
orbit number 459 on 24 July 2007. The view shows the southern hemisphere of the planet.
Credit: ESA/ MPS/DLR/IDA
Venus’s atmosphere, taken by the Venus Monitoring Camera (VMC) during Venus Express
orbit number 459 on 24 July 2007. The view shows the southern hemisphere of the planet.
Credit: ESA/ MPS/DLR/IDA
The European Space Agency's Venus Monitoring Camera (VMC) captured a series of images showing the development of a bright haze over the southern latitudes of the planet in July 2007. Over a period of days, the high-altitude veil continually brightened and dimmed, moving towards equatorial latitudes and then back towards the south pole.
These transient dark and bright markings indicate regions on the cloud-covered world where solar ultraviolet radiation is being absorbed and reflected by sulfuric acid particles, mission scientists said this week.
Gaseous sulfur dioxide and small amounts of water vapor are usually found below altitudes of about 43 miles (70 kilometers) in Venus' carbon-dioxide rich atmosphere. These molecules are usually shrouded from view by cloud layers above that block our view to the surface at visible wavelengths.