Scientists believe the discovery of the remnants of a rocky world with huge amounts of water is the first time they have found these basic ingredients for life in one place outside the Solar System.
A new study at the Universities of Warwick and Cambridge analysed the dust and debris surrounding the white dwarf star GD61 170 light years away.
Using observations from Hubble Space Telescope and the large Keck telescope on Hawaii, scientists found an excess of oxygen - a chemical signature that indicates that the debris had once been part of a bigger body originally composed of 26 per cent water by mass. By contrast, only approximately 0.023 per cent of Earth's mass is water.
In its former life, GD 61 was a star somewhat bigger than our Sun, and host to a planetary system, researchers said.
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About 200 million years ago, GD 61 entered its death throes and became a white dwarf, yet, parts of its planetary system survived.
The water-rich minor planet was knocked out of its regular orbit and plunged into a very close orbit, where it was shredded by the star's gravitational force.
"At this stage in its existence, all that remains of this rocky body is simply dust and debris that has been pulled into the orbit of its dying parent star," Professor Boris Gansicke of the Department of Physics at the University of Warwick.
"In these remnants lie chemical clues which point towards a previous existence as a water-rich terrestrial body.
"Those two ingredients - a rocky surface and water - are key in the hunt for habitable planets outside our solar system so it's very exciting to find them together for the first time outside our solar system," said Gansicke.
"These water-rich building blocks, and the terrestrial planets they build, may in fact be common - a system cannot create things as big as asteroids and avoid building planets, and GD 61 had the ingredients to deliver lots of water to their surfaces," Farihi said.
The study was published in the journal Science.