12 October 2013

Discovery Of Water In Rocky Asteroid Suggests Possibility Of Habitable Exoplanets

Image Caption: This is an artist's impression of a rocky and water-rich asteroid being torn apart by the strong gravity of the white dwarf star GD 61. Similar objects in our solar system likely delivered the bulk of water on Earth and represent the building blocks of the terrestrial planets. Credit: NASA, ESA, M.A. Garlick (space-art.co.uk), University of Warwick, and University of Cambridge

For the first time, researchers have discovered two essential components required for habitable planets – water and a rocky surface – existing together outside of our solar system.

Researchers from the University of Cambridge, the University of Warwick and the University of Kiel report in the latest edition of the journal Science that they had analyzed the dust and debris surrounding the white dwarf star GD61, which is located some 170 light years away.

That dust and debris was the shattered remains of an asteroid that contained considerable amounts of water, the researchers claim. Furthermore, the planetary system surrounding GD61 reportedly had a similar water delivery system to our own, suggesting that it had the potential to contain exoplanets similar in nature to Earth.

“Using observations obtained with the Hubble Space Telescope and the large Keck telescope in Hawaii, they 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,” the University of Warwick explained in a statement. “By contrast, only approximately 0.023 per cent of the Earth’s mass is water.”

Researchers have previously located evidence for the existence of water outside of the Milky Way, but only in the atmosphere of gas giants. This research marks the first time that it has been detected in rocky debris, making it of special interest to scientists attempting to gain new insight into how life and habitable planets form and evolve.

“The finding of water in a large asteroid means the building blocks of habitable planets existed – and maybe still exist – in the GD 61 system, and likely also around substantial number of similar parent stars,” said lead author Dr. Jay Farihi of the Cambridge Institute of Astronomy.

“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 GD61 had the ingredients to deliver lots of water to their surfaces,” he added. “Our results demonstrate that there was definitely potential for habitable planets in this exoplanetary system.”

The dwarf planet Ceres, discovered in our own solar system, contains ice buried beneath an outer crust. The authors of the new study state that there are several parallels between it and the newly-discovered rocky body. Furthermore, the investigators suggest that the water detected around GD61 probably came from a minor planet that was at least 55 miles (90 km) in diameter that had orbited the parent star before it became a white dwarf.

The researchers believe that, like with Ceres, the water on this body was most likely in the form of ice located below the planet’s surface. They discerned the diameter of the disrupted entity based on the amount of rocks and water they detected in the outer envelope of the white dwarf. However, since such observations can only detect recent accumulations, the approximated mass of the planet is said to be somewhat conservative, and that the object was likely as large as Vesta (the largest minor planet in the solar system).

“In its former life, GD61 was a star somewhat bigger than our Sun, and host to a planetary system,” the University of Warwick said. “About 200 million years ago, GD61 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.”

“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. However this planetary graveyard swirling around the embers of its parent star is a rich source of information about its former life,” added Boris Gänsicke, a professor in the UK institution’s department of physics. “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.”

Read now: Researchers propose new theory to explain signs of life in asteroids


Post a Comment

Get every new post delivered to your Inbox.


Copyright © 2018 Tracktec. All rights reserved.

Back to Top