The two ‘second Earths’ that could harbour alien life

Two exoplanets, 500 and 1,200 light years away are far more similar to earth than though, astronomers have revealed. 

Kepler-186f, 500 light-years away, is the first identified Earth-sized planet outside the solar system orbiting a star in the habitable zone.

A new study from the Georgia Institute of Technology provides new clues indicating that along with Kepler-62f, a super-Earth-sized planet orbiting around a star about 1,200 light-years away from us, it could be extremely similar to our own planet.

   

Kepler-62f, left, and Kepler-186f (right)., 500 light-years away, the Georgia Institute of Technology found both the exoplanets have ‘regular seasons and a stable climate’.

The Georgia Tech study used simulations to analyze and identify the exoplanet’s spin axis dynamics. 

Those dynamics determine how much a planet tilts on its axis and how that tilt angle evolves over time. 

Axial tilt contributes to seasons and climate because it affects how sunlight strikes the planet’s surface.

The researchers suggest that Kepler-186f’s axial tilt is very stable, much like the Earth, making it likely that it has regular seasons and a stable climate. 

The Georgia Tech team thinks the same is true for Kepler-62f, a super-Earth-sized planet orbiting around a star about 1,200 light-years away from us. 

The say the measurement is key – and that large variability in axial tilt could be a key reason why Mars transformed from a watery landscape billions of years ago to today’s barren desert.

KEPLER-186F REVEALED

Kepler-186f is less than 10 percent larger in radius than Earth, but its mass, composition and density remain a mystery. 

It orbits its host star every 130 days. 

According to NASA, the brightness of that star at high noon, while standing on 186f, would appear as bright as the sun just before sunset here on Earth.

Kepler-186f is located in the constellation Cygnus as part of a five-planet star system.

This image of Kepler-186f based on what the astronomers expect it might look like. Plant life is yellow due to the manner in which it reflects light from the star but the water and clouds would probably be more orange

This image of Kepler-186f based on what the astronomers expect it might look like. Plant life is yellow due to the manner in which it reflects light from the star but the water and clouds would probably be more orange

The find was made by a team of astronomers led by Elisa Quintana of the SETI Institute at Nasa Ames Research Center, who pored through planetary data from Nasa’s Kepler space telescope.

To date, the telescope has found hundreds of planets, but most are uninhabitable worlds that are either too large or orbit too close to their host star to support life.

The discovery of Kepler-186f, therefore, is a big milestone in the field of planet hunting.

Kepler-186f is less than 10 percent larger in radius than Earth, but its mass, composition and density remain a mystery. 

Kepler-186f is less than 10 percent larger in radius than Earth, but its mass, composition and density remain a mystery. 

It is the fifth and outermost world of the planetary system around red dwarf star Kepler-186 and is almost certainly a rocky planet.

The find is significant because it is the first Earth-sized world we’ve found in the habitable zone of a star.

Habitable zones, also known as ‘Goldilocks zones’, are regions around a star where the temperature is just right for water to form.

 

 

‘Mars is in the habitable zone in our solar system, but its axial tilt has been very unstable – varying from zero to 60 degrees,’ said Georgia Tech Assistant Professor Gongjie Li, who led the study together with graduate student Yutong Shan from the Harvard-Smithsonian Center for Astrophysics. 

‘That instability probably contributed to the decay of the Martian atmosphere and the evaporation of surface water.’

As a comparison, Earth’s axial tilt oscillates more mildly – between 22.1 and 24.5 degrees, going from one extreme to the other every 10,000 or so years.

The orientation angle of a planet’s orbit around its host star can be made to oscillate by gravitational interaction with other planets in the same system. 

If the orbit were to oscillate at the same speed as the precession of the planet’s spin axis (akin to the circular motion exhibited by the rotation axis of a top or gyroscope), the spin axis would also wobble back and forth, sometimes dramatically.

Mars and Earth interact strongly with each other, as well as with Mercury and Venus.

As a result, by themselves, their spin axes would precess with the same rate as the orbital oscillation, which may cause large variations in their axial tilt. Fortunately, the moon keeps Earth’s variations in check. 

KEPLER-62F: A GIANT EARTH 1,200 LIGHT YEARS AWAY 

Kepler-62f was the most Earth-like exoplanet until scientists noticed 186f in 2014. 

It’s about 40 percent larger than our planet and is likely a terrestrial or ocean-covered world. 

It’s in the constellation Lyra and is the outermost planet among five exoplanets orbiting a single star.

Kepler-62 and the Solar System: The diagram compares the planets of the inner solar system to Kepler-62, a five-planet system about 1,200 light years from Earth in the constellation Lyra discovered last April. Until now, these were the closest planets to Earth, in terms of size

Kepler-62 and the Solar System: The diagram compares the planets of the inner solar system to Kepler-62, a five-planet system about 1,200 light years from Earth in the constellation Lyra discovered last April. Until now, these were the closest planets to Earth, in terms of size

The planet, which is about 1,200 light-years from Earth in the direction of the constellation Lyra, is approximately 40 percent larger than Earth.

At that size, Kepler-62f is within the range of planets that are likely to be rocky and possibly could have oceans.

Nasa’s Kepler mission discovered the planetary system that includes Kepler-62f in 2013, and it identified Kepler-62f as the outermost of five planets orbiting a star that is smaller and cooler than the sun.

Kepler-62f was the most Earth-like exoplanet until scientists noticed 186f in 2014.

Kepler-62f was the most Earth-like exoplanet until scientists noticed 186f in 2014.

 

 

The moon increases our planet’s spin axis precession rate and makes it differ from the orbital oscillation rate. 

Mars, on the other hand, doesn’t have a large enough satellite to stabilize its axial tilt. 

‘It appears that both exoplanets are very different from Mars and the Earth because they have a weaker connection with their sibling planets,’ said Li, a faculty member in the School of Physics. 

‘We don’t know whether they possess moons, but our calculations show that even without satellites, the spin axes of Kepler-186f and 62f would have remained constant over tens of millions of years.’

Kepler-186f was the first Earth-size planet astronomers ever found inside the 'Goldilocks' or 'habitable' zone around another star.

Kepler-186f was the first Earth-size planet astronomers ever found inside the ‘Goldilocks’ or ‘habitable’ zone around another star.

That’s not to say either exoplanet has water, let alone life. 

But both are relatively good candidates.

‘Our study is among the first to investigate climate stability of exoplanets and adds to the growing understanding of these potentially habitable nearby worlds,’ said Li.

‘I don’t think we understand enough about the origin of life to rule out the possibility of their presence on planets with irregular seasons,’ added Shan. 

‘Even on Earth, life is remarkably diverse and has shown incredible resilience in extraordinarily hostile environments.

‘But a climatically stable planet might be a more comfortable place to start.’

 



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