[an error occurred while processing this directive]
BBC News
watch One-Minute World News
Last Updated: Monday, 7 November 2005, 12:19 GMT
Planet Venus: Earth's 'evil twin'
By Paul Rincon
BBC News science reporter

Nasa's Magellan spacecraft mapped 98% of Venus' surface with radar

The Babylonians called it "Ishtar". To the Mayans, it was known as "Chak ek", which translates as "great star".

Some ancient astronomers believed it was two separate objects: a "morning star" and an "evening star".

Venus is the brightest object in the sky except for the Sun and Moon. As such, the second planet from the Sun has fascinated humankind for millennia.

Europe's Venus Express spacecraft made its rendezvous with our nearest planetary neighbour in April to study it from orbit.

The mission aims to shed light on an enduring mystery about this world: how a planet so similar to our own in size, mass, and composition has evolved so differently over the last 4.6 billion years.

Earth can certainly take a very uncomfortable step towards Venus, though it's not likely to go all the way
Prof Fred Taylor, Oxford University
Venus has undergone runaway greenhouse warming, whereby trapped solar radiation has heated the planet's surface to an average temperature of 467C (872F) - hot enough to melt lead.

A dense atmosphere, composed chiefly of carbon dioxide (CO2), generates a surface pressure 90 times greater than that on Earth.

Exotic vision

Through Venus Express, scientists hope to understand better the mechanics of climate change on our own planet.

"Earth can certainly take a very uncomfortable step towards Venus, though it's not likely to go all the way," comments Fred Taylor, Halley Professor of Physics at the University of Oxford, UK.

"The point is, we're moving in that direction and many of the constituents and mechanisms involved are the same. Even a few degrees change in temperature can be a disaster on Earth."

Artist's impression of the surface of Venus
Greenhouse hell: How the surface of Venus might look
And studying our neighbour could help verify computer models to predict how climate change will affect Earth. "Venus provides an extreme test for the atmospheric physics models that we have for Earth," says Andrew Coates of the Mullard Space Science Laboratory at University College London, UK.

The prevailing view of Venus used to be very different. "Even though Venus is closer to the Sun, its cloud cover is very shiny and reflective," Fred Taylor explains.

"If you work out the energy balance, Venus is actually absorbing less heat from the Sun than the Earth is. By-and-large, you might expect surface conditions to be the same."

Probe train

With a 25km-thick layer of opaque cloud concealing the planet's surface from view, free rein has been given to science fiction writers, who have depicted Venus with lush jungle, swamp and oceans.

It was only when unmanned space probes were sent to explore the planet at close range that its romantic image was finally shattered.

Between 1961 and 1989, the US and USSR launched more than 30 spacecraft towards Venus. Some reached their destination, others did not.

Venus, Venera 13
Venera 13 took this colour photo of Venus' surface
The American Mariner 2 probe made the first successful flyby in 1962, confirming high surface temperatures.

Later missions sent back information about the thickness and chemical composition of the cloud layers as well as surface conditions.

The USSR's Venera 7 probe was first to land, surviving for 20 minutes before succumbing to the crushing pressure and burning heat. Its successor, Venera 9, sent back the first images from the surface.

Orbiting spacecraft have carried out radar surveys, peering through the planet's opaque clouds to map its surface. Principal among these was Nasa's Magellan probe which circled Venus eight times a day from 1990 to 1994.

Metallic 'snow'

Magellan's images show a youthful landscape where volcanism has covered up most of the ancient past. Volcanoes of every size and type are scattered across vast plains formed by lava coursing out from beneath the planet's surface.

The question is: did it once also have a landscape touched by running water, even large seas?

"Venus was born with the same sorts of constituents as Earth, which means there was some water in the environment. Some more probably came in from comets," Andrew Coates explains.

Venus, Nasa
Reflective clouds ensure Venus absorbs less sunlight than Earth
What water there was has long since boiled away - runaway greenhouse warming has left Venus one of the driest places in the Solar System.

Magellan also revealed that the Venusian highlands are unusually bright, reflecting radar beams much better than lower elevations. Several explanations have been put forward, ranging from the presence of loose soil to a covering of metal "snow".

At Venus's hot lower layers, many metals would be vaporised and exist as a metallic mist. But at higher elevations, where it is a little cooler, they could condense to form a thin, highly reflective layer on the ground.

As for what the snow is made from, the rare metal tellurium and iron pyrites, or "Fool's Gold", have both been proposed as candidates.

Recent work by a team at the Washington University at St Louis suggests the metallic frost is more likely to be sulphides of lead or bismuth.

Acid rain

Fred Taylor thinks the greenhouse effect on Venus has been driven all along by volcanism. Active volcanoes would have pumped copious quantities of the greenhouse gas carbon dioxide (CO2) into the atmosphere.

Water evaporating from the surface would then have acted in concert with CO2 to trap solar radiation and heat up the planet (water vapour is a stronger greenhouse gas per molecule than CO2).

Sunlight then split the water into its constituents, hydrogen and oxygen.

Unlike Earth, Venus is not protected by a magnetic field, so particles can be siphoned off from the top of its atmosphere. This allowed "light" hydrogen to escape from Venus, leaving more of its heavier form - deuterium - in place.

"On Earth, the amount of carbon dioxide is controlled because it dissolves in the surface water, that's why you get deposition on the ocean floor of carbonates," says Dr Coates.

"On Venus, there was no surface water and no natural 'sink' for CO2."

Today, Venus' atmosphere consists almost entirely (97%) of carbon dioxide, with clouds containing droplets of sulphuric acid along with compounds of chlorine and fluorine.

These precipitate an acid rain called virga, which evaporates before it has the chance to reach the surface.

In the upper part of the atmosphere, clouds swirl by at a rate of 300km/h, driven by fierce winds.

Venus itself sluggishly rotates in an East to West (retrograde) direction, turning on its axis once every 243 Earth days.

This is strange - especially since its orbital path around the Sun lasts 225 Earth days. If one were to stand on the surface, one would get the impression that the day was longer than the year.

A 'relaxed' Venus

Scientists have no way of telling how long present-day conditions have existed on Venus.

Venus Express, European Space Agency

According to one theory, the current surface temperature might be stabilised through a complex interaction between the atmosphere and minerals in the rocks. But this idea requires a lot of the crust to be in contact with the atmosphere.

If this idea is discarded for a moment, and one assumes that the greenhouse warming is driven by volcanism, then conditions could be fluctuating on a relatively short timescale.

"At some point the volcanism will run out. It ran out on Mars a long time ago, and it has partially run out on Earth," says Fred Taylor.

"The volcanism will eventually subside to the point where it can't maintain these high temperatures and pressures. It's interesting to ask yourself what will happen then."

Recent atmospheric models predict that the harsh conditions on Venus will eventually relax, and the planet will become more Earth-like.

"You might get the oceans back, if there's enough water vapour to condense. And once you get the oceans back, they hasten the removal of CO2 from the atmosphere because they dissolve it and turn it into rocks," said Professor Taylor.

"You might end up with a Venus that's quite a lot like people thought it was going to be in the 1950s."

PLANETS COMPARED
VENUS
EARTH
Distance from Sun 108,200,000km 149,600,000km
Diameter 12,103.6km 12,756.3km
Mass 0.82 Earth masses 1.0 Earth masses
Axial rotation period (sidereal day) 243 Earth days (retrograde) 23 hours 56 minutes
Year length 224.7 Earth days 365 days
Atmosphere 96% carbon dioxide
3% nitrogen
77% nitrogen
21% oxygen
Mean temperature 464C 15C
Surface pressure 92 bar 1 bar
Moons 0 1
Global magnetic field No Yes




SEE ALSO:
Mission guide: Venus Express
18 Oct 05 |  Science/Nature
Planet Venus completes transit
08 Jun 04 |  Science/Nature
Venus clouds 'might harbour life'
25 May 04 |  Science/Nature
Reworked images reveal hot Venus
13 Jan 04 |  Science/Nature
Venus has 'heavy metal mountains'
25 Nov 03 |  Science/Nature
Venus mission is on
08 Nov 02 |  Science/Nature


RELATED BBC LINKS:

RELATED INTERNET LINKS:
The BBC is not responsible for the content of external internet sites


PRODUCTS AND SERVICES

Americas Africa Europe Middle East South Asia Asia Pacific