- Venus might once had have more water
- Water split by sunlight; hydrogen/oxygen escaped to space
- If it was wetter, could it have had life?
The Venus Express spacecraft is helping planetary scientists investigate whether Venus once had oceans. If it did, it may even have begun its existence as a habitable planet similar to Earth.
These days, Earth and Venus seem completely different. Earth is a lush, clement world teeming with life, whilst Venus is hellish, its surface roasting at temperatures of a furnace.
But underneath it all the two planets share a number of striking similarities. They are nearly identical in size and now, thanks to the European Space Agency’s (ESA) Venus Express orbiter, planetary scientists are seeing other similarities too.
“The basic composition of Venus and Earth is very similar,” says Håkan Svedhem, ESA Venus Express Project Scientist.
One difference stands out—the planet has very little water. Were the contents of Earth’s oceans to be spread evenly across Venus, they would create a layer 3km deep. If you were to condense the current amount of water vapour in Venus’ atmosphere onto its surface, it would create a global puddle just 3cm deep.
Water lost into space
Yet there is another similarity here. Billions of years ago, Venus probably had much more water. Venus Express has confirmed that the planet has lost a large quantity of water into space.
This happens because ultraviolet radiation from the Sun streams into Venus’ atmosphere and breaks the water molecules into their atoms—two of hydrogen and one of oxygen. These then escape to space.
Venus Express has measured the rate of this escape and confirmed that roughly twice as much hydrogen is escaping as oxygen. It’s therefore thought that water is the source of these escaping atoms.
It has also shown that a heavy form of hydrogen, called deuterium, is enriched in the upper echelons of Venus’s atmosphere, because the heavier hydrogen finds it harder to escape the planet’s grip.
“Everything points to there being large amounts of water on Venus in the past,” says Colin Wilson, Oxford University, UK. But that doesn’t necessarily mean there were oceans on the planet’s surface.
No oceans, but life anyway?
Eric Chassefière, Université Paris-Sud, France, has developed a computer model that suggests the water was largely atmospheric and existed only during the very earliest times, when the surface of the planet was completely molten.
As the water molecules were broken into atoms by sunlight and escaped into space, the subsequent drop in temperature probably triggered the solidification of the surface. In other words, no oceans.
Although it is difficult to test this hypothesis, it does raise a key question. If Venus ever did possess surface water, could planet have had an early habitable period?
Even if true, Chassefière’s model does not preclude the chance that colliding comets might have brought additional water to Venus after its surface solidified, and these could have created bodies of standing water in which life may have been able to form.
Adapted from information issued by ESA / MPS / DLR / IDA / J. Whatmore.