Sunday Times (Sri Lanka)

The second Earth that we could visit in our lifetime

Planet is discovered just four light years away and scientists say it may have liquid water and alien life

- By Abigail Beall

We may have been given our best chance of finding alien life outside our solar system. A rocky planet that may harbour life has been discovered just four light years from Earth - close enough to be reached by future space missions.

The planet, dubbed 'a second Earth', is the right distance from its star to host liquid water, which means it has the potential for alien life.

It is the closest exoplanet we could ever discover, and experts say missions to the planet to search for signs of life could be feasible 'within our lifetime'.

Astronomer­s have found clear evidence that our nearest star, Proxima Centauri, is the sun to another Earth-like world. The group of researcher­s, using the European Southern Observator­y (ESO) telescopes, have named the exciting world Proxima b.

Thousands of exoplanets have been discovered before, but unlike the others, this planet is within our reach.

While four light years is a long way - more than 25 trillion miles -- future generation­s of super-fast space craft could conceivabl­y travel to the planet within the next few decades.

Much further in the future the planet may even be colonised by space travellers from Earth.

One possible obstacle to life evolving and flourishin­g on the planet is the way it hugs its parent star.

Proxima b is only 4.6 million miles (7.5 million km) from the star, 5 per cent of the distance between the Earth and the sun, and takes just 11.2 days to complete one orbit. It is around 1.3 times as massive as Earth.

But because Proxima Centauri is a dim red dwarf star radiating much less heat than the sun, it still occupies the 'habitable zone' where temperatur­es are mild enough to permit liquid surface water.

The temperatur­e on the surface of the planet could be between -90° and 30° Celsius (-130 and 86 Fahrenheit).

On the other hand, the planet is blasted by powerful ultraviole­t rays and X-rays from the star. Any life that evolved on its surface would have to be hardened against the radiation.

But the prospect of finding life on Proxima b has excited scientists.

'Many exoplanets have been found and many more will be found, but searching for the closest potential Earth-analogue and succeeding has been the experience of a lifetime for all of us,' Dr Guillem Anglada-Escudé, lead author of the paper, said.

'Many people's stories and efforts have converged on this discovery. The result is also a tribute to all of them. The search for life on Proxima b comes next.'

Two separate papers have been published on Thursday, describ- ing the habitabili­ty of Proxima b and its climate.

The papers find the existence of liquid water on the planet 'cannot be ruled out'.

This means water may be present over the surface of the planet. But it would only be in the sunniest regions, either in an area in the hemisphere of the planet facing the star.

The way Proxima b rotates, strong radiation from its star and the formation history of the planet makes its climate quite different from that of the Earth.

It is unlikely that Proxima b has seasons. But if liquid water does exist on the planet, it could mean alien life might thrive there.

If this is the case, we could discover it within decades, experts have said.

A team called Pale Red Dot is behind the discovery, which includes researcher­s from the University of Hertfordsh­ire, Queen Mary University of London, the Instituto de Astrofísic­a de Andalucía in Granada, Spain and the University of Göttingen in Germany, among others.

The researcher­s used the High Accuracy Radial velocity Planet Searcher (HARPS), an instrument on the European Southern Observator­y's 3.6metre La Silla telescope in Chile's Atacama Desert.

The telescope measured light from Proxima, the fingerprin­ts that reveal what the star is made of.

Small shifts in the frequency of the starlight can be used to work out tiny movements of the star in response to an orbiting planet's gravitatio­nal pull.

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