Tuesday, June 16, 2015

Mars NEVER had oceans

'Mars NEVER had oceans': New theory says the red planet used to be cold and icy, not warm and wet

  • A team of scientists in Massachusetts studied Mars 3 to 4 billion years ago
  • Previous evidence had suggested that it used to have seas and oceans
  • But this new theory says it was more likely just covered in ice
  • This would apparently explain the appearance of certain valleys 
In the hunt for past or present life on Mars, scientists have been building evidence that proves the planet was once covered in liquid water - a key condition for life as we know it.
But a new study suggests that the red planet never had seas or oceans - it was instead too cold and was just covered in ice.
The disappointing theory, if true, says that most of the features on the red planet can be explained by ice - meaning the chances of life ever having existed there are slim.

A team of scientists in Massachusetts studied Mars 3 to 4 billion years ago. Previous evidence had suggested that it used to have seas and oceans (left). But this new theory says it was more likely just covered in ice (right). This would apparently explain the appearance of valleys in certain locations
A team of scientists in Massachusetts studied Mars 3 to 4 billion years ago. Previous evidence had suggested that it used to have seas and oceans (left). But this new theory says it was more likely just covered in ice (right). This would apparently explain the appearance of valleys in certain locations

The research was led by Dr Robin Wordsworth of the Harvard Paulson School of Engineering and Applied Sciences in Cambridge, Massachusetts.
With his team, they modelled two scenarios for Mars three to four billion years ago - one where it was warm and wet at 10°C (50°F), and the other cold and icy at -48°C (-54°F).
Based on the history of the sun and the tilt of Mars’ axis during this period, the team found that the cold scenario was more likely to occur.
It also could more easily explain certain ‘water erosion’ features on Mars, such as valleys and cliffs.
‘I'm still trying to keep an open mind about this,’ said Dr Wordsworth.
‘There is lots of work to be done. But our results show that the cold/icy scenario matches the surface distribution of erosion features more closely.
‘This strongly suggests that early Mars was generally cold, and water was supplied to the highland regions as snow, not as rain.’
Mars only gets 43 per cent of the solar energy that Earth does, while the sun was 25 per cent dimmer than it is today three to four billion years ago.
Dr Wordsworth said this makes it very likely Mars was cold and icy.
In addition, an extreme tilt of the Martian axis would have pointed the planet’s poles towards the sun and moved ice towards the equator.
This could have formed the water drainage and erosion features seen today.

Some regions on the equator near the giant canyon Valles Marineris (shown) were thought to have little rainfall, but are strewn with valleys that must have been formed by water. The new theory says rapidly melting ice - possibly by a meteorite impact or volcanic eruption - would have created short-lived water for this to happen
Some regions on the equator near the giant canyon Valles Marineris (shown) were thought to have little rainfall, but are strewn with valleys that must have been formed by water. The new theory says rapidly melting ice - possibly by a meteorite impact or volcanic eruption - would have created short-lived water for this to happen

Evidence from missions such as the Curiosity rover (pictured) has previously shown fairly conclusively that Mars used to have water on its surface. However, the key questions now are how long this water remained on the surface, and whether the planet was hot or cold
Evidence from missions such as the Curiosity rover (pictured) has previously shown fairly conclusively that Mars used to have water on its surface. However, the key questions now are how long this water remained on the surface, and whether the planet was hot or cold

The theory is in stark contrast to the warm and wet theory, which suggests that clouds, dust and carbon dioxide kept the planet warm enough to have water for millions of years. 
In May this year, for example, Nasa scientists said that Mars had more water than the Arctic Ocean 3.7 billion years ago, mostly in its northern hemisphere.
They said it would have kept this water for 1.5 billion years before ultimately losing almost all its water when its atmosphere disappeared, for reasons unknown.
Dr Wordsworth, though, says that a warm and wet Mars does not explain the network of valleys at the Martian equator.

THE WET PLANET? MOUNTING EVIDENCE FOR WATER ON MARS 

Evidence of water on Mars dates back to the Mariner 9 mission, which arrived in 1971. It revealed clues of water erosion in river beds and canyons as well as weather fronts and fogs.
Viking orbiters that followed caused a revolution in our ideas about water on Mars by showing how floods broke through dams and carved deep valleys.
Mars is too cold and barren now for liquid water to exist on its surface.
But in June 2013, the Curiosity rover found powerful evidence that water good enough to drink once flowed on Mars.
In September of the same year, the first scoop of soil analysed by Curiosity revealed that fine materials on the surface of the planet contain two per cent water by weight.
Earlier this year, scientists provided the best estimates for water on Mars, claiming it once had more than the Arctic Ocean - and the planet kept these oceans for more than 1.5 billion years.
The findings suggest there was ample time and water for life on Mars to thrive, but over the last 3.7 billion years the red planet has lost 87 per cent of its water - leaving it barren and dry. 

In May this year, Nasa scientists said that Mars had more water than the Arctic Ocean 3.7 billion years ago, mostly in its northern hemisphere. Dr Wordsworth, though, says that a warm and wet Mars does not explain the network of valleys at the Martian equator
In May this year, Nasa scientists said that Mars had more water than the Arctic Ocean 3.7 billion years ago, mostly in its northern hemisphere. Dr Wordsworth, though, says that a warm and wet Mars does not explain the network of valleys at the Martian equator

Is this what Mars once looked like? Previous evidence has suggested that the planet would have kept its water for 1.5 billion years before ultimately losing almost all its water when its atmosphere disappeared 2.2 billion years ago, for reasons unknown
Is this what Mars once looked like? Previous evidence has suggested that the planet would have kept its water for 1.5 billion years before ultimately losing almost all its water when its atmosphere disappeared 2.2 billion years ago, for reasons unknown

Regions where lots of rain is predicted to have failed - such as the Arabia area around the Hellas basin - have few water drainage features.
But others, such as Margaritifer Sinus that is predicted to have had ten to twenty times less water, has many supposedly water-carved valleys.
Dr Wordsworth said the cold and icy scenario, while not perfect, can explain these features.
In this scenario, the climate would have been cool most of the time, but short-lived events such as meteor impacts and volcanic eruptions would have melted it and formed water, carving the valleys.
Under this scenario, water could have existed for brief periods, but a key question in resolving whether Mars was warm or cold is how long water was on the surface.

How Mars lost its water is a key question that remains. It is thought to have been due to the atmosphere leaving the planet - a process that also remains a mystery. Understanding what happened to Mars may also indicate what will happen to Earth in the future
How Mars lost its water is a key question that remains. It is thought to have been due to the atmosphere leaving the planet - a process that also remains a mystery. Understanding what happened to Mars may also indicate what will happen to Earth in the future

‘We know from rover- and orbiter-based data that there were lakes on ancient Mars,’ said Bethany Ehlmann, a planetary scientist at California Institute of Technology and Nasa's Jet Propulsion Laboratory in Pasadena, California, who was not involved in the new study.
‘Key questions are: how long did they persist? Were they episodic or persistent? And does the feeder valley network demand rain or is snow and ice melt sufficient?’
The research was published in the Journal of Geophysical Research - Planets.

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