Astrophysicists have found the first evidence of a water-rich rocky planetary body outside our solar system in its shattered remains orbiting a white dwarf 170 light years away.
The analysis of the dust and debris surrounding the white dwarf star GD 61 was conducted by scientists at the Universities of Warwick and Cambridge and appears in the journal Science.
Using observations obtained with Hubble and the Keck telescope, the team 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 percent water by mass. By contrast, only approximately 0.023 percent of the Earth’s mass is water.
Evidence for water outside our solar system has previously been found in the atmosphere of gas giants, but this study marks the first time it has been pinpointed in a rocky body, making it of significant interest in our understanding of the formation and evolution of habitable planets and life.
The researchers suggest it is most likely that the water detected around the white dwarf GD 61 came from a minor planet at least 90 km in diameter (but potentially much bigger) that once orbited the parent star before it became a white dwarf.
In its former life, GD 61 was a star somewhat bigger than our Sun, and host to a planetary system. 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. The researchers believe that destabilizing the orbit of the minor planet requires a so far unseen, much larger planet going around the white dwarf.
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