NASA discovers planet ‘Kepler-452b’ that is most similar to Earth

Kepler-452b is first near-Earth-size planet in ‘habitable zone’ around a sun-like star, says NASA.

Newly discovered Kepler-452b is first near-Earth-size planet in 'habitable zone' around a sun-like star, says NASA. (Image: NASA)
Newly discovered Kepler-452b is first near-Earth-size planet in 'habitable zone' around a sun-like star, says NASA. (Image: NASA)

A planet believed to be remarkably similar to Earth has been discovered orbiting a distant sun-like star, bolstering hopes of finding life elsewhere in the universe, US scientists said on Thursday.

The planet, which is about 60 percent bigger than Earth, is located 1,400 light years away in the constellation Cygnus. It was discovered by astronomers using NASA’s Kepler space telescope and circles a star that is similar in size and temperature to the sun, but older.

“In my mind, this is the closest thing we have to another planet like the Earth,” astronomer Jon Jenkins, with the U.S. space agency’s Ames Research Center in Moffett Field, California, told reporters on a conference call.

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The planet, dubbed Kepler-452b, orbits a star that is about 6 billion years old, compared to the 4.6 billion year age of the sun.

kepler 452b, earth like planet

“It’s simply awe-inspiring to consider that this planet has spent 6 billion years in the habitable zone of its star,” Jenkins said.

“That’s considerable time and opportunity for life to arise somewhere on its surface or in its oceans should all the necessary ingredients and conditions for life exist on this planet,” he said.

Kepler-452b is positioned about as far from its parent star as Earth is from the sun, completing an orbit in 385 days, compared to Earth’s 365-day orbit.  At that distance, surface temperatures would be suitable for liquid water, a condition believed to be critical for life.

Scientists previously have found Earth-sized planets orbiting in stars’ so-called “habitable zones,” but those stars are cooler and smaller than the sun, a G2 type yellow star.

NASA launched the Kepler telescope in 2009 to survey a sampling of nearby stars in an attempt to learn if planets like Earth were common in the galaxy.

“This is great progress in finding a planet like Earth that is similar in size and temperature around a sun-like star,” said Kepler scientist Jeff Coughlin, with the SETI Institute in Mountain View, California.

kepler 452b
The planet, dubbed Kepler-452b, orbits a star that is about 6 billion years old, compared to the 4.6 billion year age of the sun. (Image: NASA)

Based on its size, scientists believe Kepler-452b should be rocky, like the Earth, though that theory is based on statistical analysis and computer modeling, not direct evidence.

“With a radius 60 percent larger than the Earth, this planet has a somewhat better than even chance of being rocky,” Jenkins said.

If so, Kepler-452b could be about five times as massive as Earth and have gravity that is twice as strong as what exists on Earth’s surface. The planet also could have a thick atmosphere, cloudy skies and active volcanoes, Jenkins said.

With the discovery of Kepler-452b, the telescope has found 1,030 confirmed planets and identified about 4,700 candidate planets. The list of potential planets includes 11 other near-Earth twins, nine of which circle sun-like stars.

The telescope cannot see planets directly, but measures minute changes in light coming from target stars.

Sophisticated computer programs and follow-up observations with a ground-based telescopes then determine if some of the light dips were caused by planets passing in front of their parent stars, relative to Kepler’s line of sight.

A positioning system failure ended the telescope’s prime planet-hunting mission in 2013, but it has since been repurposed for other astronomical observations.

Attempts to learn if Kepler-452b has an atmosphere likely will have to wait for a new generation of more sensitive space telescopes, said NASA’s associate administrator John Grunsfeld.

The research will be published in The Astronomical Journal.

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First published on: 24-07-2015 at 08:39 IST
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