英文科普：火星环境曾经适宜生物的生存

Conditions favourable¹ to life may once have existed all over Mars. Detailed² studies of minerals found inside craters³（火山口） show that liquid water was widespread, not only in the southern highlands, but also beneath the northern plains. ESA's Mars Express and NASA's Mars Reconnaissance（侦查，勘探） Orbiter have discovered hydrated（含水的） silicate⁴ minerals（硅酸盐矿物） in the northern lowlands of Mars, a clear indication that water once flowed there.

The spacecraft have previously⁵ discovered thousands of small outcrops in the southern hemisphere where rock minerals have been altered by water. Many of these exist in the form of hydrated clay（粘土） minerals known as phyllosilicates（层状硅酸盐） , and indicate that the planet's southern hemisphere was once much warmer and wetter than it is today.

However, until this week, no sites with hydrated silicate minerals had been found in the northern lowlands, where thick blankets of lava⁷（火山岩浆） and sediments⁸ up to several kilometres thick hamper⁹ efforts to probe the underlying¹⁰ bedrock.

The first hints that there may be hydrated silicates⁶ beneath the northern plains were provided by Mars Express' OMEGA sensor¹¹. However, the outcrops were small and more detailed observations were required to confirm their presence. The OMEGA team sifted¹² higher resolution data from a sensor on NASA's orbiter.

Their search concentrated on 91 sizeable impact craters where incoming asteroids（小行星） had punched down several kilometres, exposing ancient crustal（地壳的） material. As reported this week in the journal Science, at least nine craters were found to contain phyllosilicates or other hydrated silicates.

These minerals, which formed in wet environments on the surface or underground, were identical to those found in the southern hemisphere.

"We can now say that the planet was altered on a global scale by liquid water more than 4 billion years ago," says John Carter, University of Paris, the report's lead author.

With the small sample of widely scattered¹³ sites, it is difficult to draw conclusions about the type of environment all that time ago. However, the nature and locations of the minerals provide some clues.

"They are rich in iron and magnesium（镁） , but less in aluminium¹⁴. Together with the close proximity¹⁵ of olivine, which is easily modified by water, this indicates that the exposure to water lasted only tens to hundreds of millions of years," says Jean-Pierre Bibring, the OMEGA Principal Investigator¹⁶ from the University of Paris.

Although Mars' potential habitability did not last long, remarkably¹⁷ its record is still preserved in phyllosilicate-rich spots.

A number of scientists have suggested that a shallow ocean subsequently covered the lava-coated northern plains. However, no evidence in support of this is provided by the new results.

"Our studies do not find any signs of the lava plains in the north being altered by water," says Dr Bibring.

On a positive note, the new results may suggest sites for future landers because evidence for water during the early history of Mars suggests that conditions may have been favourable for the evolution of primitive（原始的，远古的） life.

"These results reveal the history of Mars derived¹⁸ from the planet's mineralogy（矿物学） ," says Olivier Witasse, ESA Project Scientist for Mars Express. "It is another example of the fruitful cooperation between European and American scientists."