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Earth-like oceans may be common on other planets

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Press Trust of India London
Last Updated : May 07 2015 | 4:42 PM IST
Water delivery via asteroids or comets is likely taking place in many other planetary systems, just as it happened on Earth, according to a new research that suggests Earth-like oceans may be common on other planets.
The research led by the University of Warwick found evidence for numerous planetary bodies, including asteroids and comets, containing large amounts of water.
The findings add further support to the possibility that water can be delivered to Earth-like planets via such bodies to create a suitable environment for the formation of life, researchers said.
"Our research has found that, rather than being unique, water-rich asteroids similar to those found in our Solar System appear to be frequent," said lead researcher Dr Roberto Raddi, of the University of Warwick's Astronomy and Astrophysics Group.
"Accordingly, many planets may have contained a volume of water, comparable to that contained in the Earth," Raddi said.
"It is believed that the Earth was initially dry, but our research strongly supports the view that the oceans we have today were created as a result of impacts by water-rich comets or asteroids," Raddi said.

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In observations obtained at the William Herschel Telescope in the Canary Islands, the University of Warwick astronomers detected a large quantity of hydrogen and oxygen in the atmosphere of a white dwarf (known as SDSS J1242+5226).
The quantities found provide the evidence that a water-rich exo-asteroid was disrupted and eventually delivered the water it contained onto the star.
The asteroid, the researchers discovered, was comparable in size to Ceres - at 900 km across, the largest asteroid in the Solar System.
"The amount of water found on SDSS J1242+5226 is equivalent to 30-35 per cent of the oceans on Earth," said Raddi.
The impact of water-rich asteroids or comets onto a planet or white dwarf results in the mixing of hydrogen and oxygen into the atmosphere. Both elements were detected in large amounts in SDSS J1242+5226.
"Oxygen, which is a relatively heavy element, will sink deep down over time, and hence a while after the disruption event is over, it will no longer be visible," said research co-author Professor Boris Gansicke, also of the University of Warwick.
"In contrast, hydrogen is the lightest element; it will always remain floating near the surface of the white dwarf where it can easily be detected.
"There are many white dwarfs that hold large amounts of hydrogen in their atmospheres, and this new study suggests that this is evidence that water-rich asteroids or comets are common around other stars than the Sun," Gansicke said.
The research is published in the Monthly Notices of the Royal Astronomical Society.

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First Published: May 07 2015 | 4:42 PM IST

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