November 30, 2010
Venus Could Hold Warning For Earth
A mysterious high-altitude layer of sulphur dioxide discovered by ESA's Venus Express has been explained. As well as telling us more about Venus, it could be a warning against injecting our atmosphere with sulphur droplets to mitigate climate change.
Venus is blanketed in sulphuric acid clouds that block our view of the surface. The clouds form at altitudes of 50"“70 km when sulphur dioxide from volcanoes combines with water vapor to make sulphuric acid droplets. Any remaining sulphur dioxide should be destroyed rapidly by the intense solar radiation above 70 km.
So the detection of a sulphur dioxide layer at 90"“110 km by ESA's Venus Express orbiter in 2008 posed a complete mystery. Where did that sulphur dioxide come from?
"We had not expected the high-altitude sulphur layer, but now we can explain our measurements," says HÃ¥kan Svedhem, ESA's Venus Express Project Scientist.
"However, the new findings also mean that the atmospheric sulphur cycle is more complicated than we thought."
As well as adding to our knowledge of Venus, this new understanding may be warning us that proposed ways of mitigating climate change on Earth may not be as effective as originally thought.
Nobel prize winner Paul Crutzen has recently advocated injecting artificially large quantities of sulphur dioxide into Earth's atmosphere at around 20 km to counteract the global warming resulting from increased greenhouse gases.
The proposal stems from observations of powerful volcanic eruptions, in particular the 1991 eruption of Mount Pinatubo in the Philippines that shot sulphur dioxide up into Earth's atmosphere. Reaching 20 km in altitude, the gas formed small droplets of concentrated sulphuric acid, like those found in Venus' clouds, which then spread around Earth. The droplets created a haze layer that reflected some of the Sun's rays back into space, cooling the whole planet by about 0.5°C.
However, the new work on the evaporation of sulphuric acid on Venus suggests that such attempts at cooling our planet may not be as successful as first thought, because we do not know how quickly the initially protective haze will be converted back into gaseous sulphuric acid: this is transparent and so allows all the Sun's rays through.
"We must study in great detail the potential consequences of such an artificial sulphur layer in the atmosphere of Earth," says Jean-Loup Bertaux, Universit© de Versailles-Saint-Quentin, France, Principal Investigator of the SPICAV sensor on Venus Express. "Venus has an enormous layer of such droplets, so anything that we learn about those clouds is likely to be relevant to any geo-engineering of our own planet."
In effect, nature is doing the experiment for us and Venus Express allows us to learn the lessons before experimenting with our own world.
Image 1: This false-color ultraviolet image of the south pole of Venus was obtained by the Venus Monitoring Camera (VMC) on board ESA's Venus Express on 25 February 2008 from a distance of about 20 000 km, at a wavelength of 365 nanometers. The octagonal shape of the image is due to the VMC field of view. It is a zoom-in on the south polar "Ëcap', located inside a 60-degree-latitude circle. It shows a very bright and uniform appearance and lacks small-scale markings. However several global dark streaks usually cross the polar regions and seem to indicate strong jet-winds in the atmosphere around the pole. Credits: ESA/MPS/DLR/IDA
Image 2: Venus Express has two solar cell panels per wing comprising alternating rows of standard triple junction solar cells as well as highly reflective mirrors to reduce the operating temperatures. There is twice as much sunlight in Venus's orbit as there is in Earth's orbit, plus additional thermal input from the Venusian surface and atmosphere "“ 75% of sunlight being reflected up from it. In certain cases, this results in Venus Express receiving an equivalent of the thermal input from 3.5 Suns.
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