Scientists spot 'potentially 

habitable' super-Earth 

planet just 21 light-years 

away

  • Scientists say the planet is about 2.8 Earth masses, 
  • and sits 21 light-years away
  • It could even be habitable, as it sits on the inner edge
  •  of star's habitable zone
  • They say it may be rocky world, and could be cool 
  • enough to sustain liquid water
Scientists have detected a new ‘super-Earth’ planet just 21 light-years away, and they say it could be habitable. It's roughly three times more massive than Earth, and is thought to be a rocky world that may even be cool enough to sustain liquid water. Artist's impression pictured
Scientists have detected a new ‘super-Earth’ planet just 21 
light-years away, and they say it could be habitable.
 It's roughly three times more massive than Earth, and is 
thought to be a rocky world that may even be cool enough to
 sustain liquid water. Artist's impression pictured

THE

 'SUPER-EARTH'

The new planet is situated 
relatively close to our solar
 system,
 being just 21 light years
 away.
Scientists estimate the 
planet to
 be about 2.8 Earth
 masses, 
and sit about .08 
astronomical 
units (AU) from its host
 star,
 placing it in the habitable 
zone.
Researchers are now 
hoping to characterize its 
atmosphere 
and other features to better
 assess its potential to
 support life.
It's thought to be a rocky 
world that may even be 
cool
 enough to sustain liquid
 water.

Scientists have detected a new ‘super-Earth’ planet just 21 light-years away, and they say it could be habitable.
The planet is roughly three times more massive than Earth, and is thought to be a rocky world that may even be cool enough to sustain liquid water.
It orbits along the inner edge of an M-dwarf star’s habitable zone, and researchers are now hoping to characterize its atmosphere and other features to better assess its potential to support life.





The planet was spotted by researchers at the Canary Islands Institute of Astrophysics (IAC) using the 3.6-meter Galileo National Telescope at the Roque de los Muchachos Observatory.
Using the High Accuracy Radial Velocity Planet Searcher for the Northern Hemisphere spectrograph (HARPS-N), they obtained 151 spectra over a period of 3.5 years.
Small variations in its radial velocity revealed the presence of the planet, as a result of its gravitational pull
 as it circles the red dwarf star GJ625 (Gliese 625).
Each complete orbit takes roughly 14 days, the researchers say.
Scientists estimate the planet to be about 2.8 Earth masses, and sit 
about .08 astronomical units (AU) from its host star, placing it in the 
habitable zone.
‘As GJ625 is a relatively cool star, the planet is situated at the edge
 of its habitability zone, in which liquid water can exist on the surface,’
 says Alejandro Suárez Mascareño, one of the study’s authors.

‘In fact, depending on the cloud cover of its atmosphere
 and on its rotation, 
it could potentially be habitable.’

The new planet is situated relatively close to our solar system, being just 21
 light years away, and the researchers say it’s the least massive of the 
super-Earths found to date.
Moving forward, scientists will attempt to observe the planet as it passes
 in front of its star, to figure out its density, radius, and characterize its 
atmosphere, according to Rafael Rebolo, one of the study's authors.

The new planet is situated relatively close to our solar system, being just 21 light years away, and the researchers say it’s the least massive of the super-Earths found to date. This can be seen in the graph above
The new planet is situated relatively close to our solar system,
 being just 21 light years away, and the researchers say it’s
 the least massive of the super-Earths found to date. 
This can be seen in the graph above


This could be done by 'using the high resolution high stability 
spectrographs on the GTC, or on telescopes of the next
 generation in the northern hemisphere, such as the 
Thirty Meter Telescope (TMT),' Rebolo says. 
‘In the future, new observing campaigns of photometric 
observations will be essential to try to detect the transit of this 
planet across its star, given its proximity to the sun,’ said 
Jonay González Hernández.
‘There is a possibility that there are more rocky planets around
 GJ625 in orbits which are nearer to, or further away from the star,
 and within the habitability zone, which we will keep on combing.’ 
(The Mail, UK)
NASA on Kepler's mission to find planets in 'habitable zones'
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