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Monday, 19 August 2019

There Could Be Up to 10 Billion Habitable Earth-Like Planets in Our Galaxy Alone




Our galaxy could be filled
with warm, water harboring planets like Earth. That's the deduction of students
at Penn State University, who used data from NASA's Kepler telescope to approximate the
number of Earth-like planets in our home galaxy. Their outcomes, issued
in The
Astronomical Journal
 this week, propose that an Earth-like planet circles
one in every four Sun-like stars.





Image result for There Could Be Up to 10 Billion Earth-Like Planets in Our Galaxy Alone





Totaled up, that means there
could be up to 10 billion Earth-like worlds in the Milky Way. The assessment is
a significant step in the search for alien life, as any potential life on other
planets would most probably be discovered on an Earth-like world warm enough to
sustain liquid water. So a better understanding of the possible number of
Earth-like planets in the galaxy can notify projects like the Wide-Field
Infrared Survey Telescope, which will launch into space in the mid-2020s and search
for clues of oxygen and water vapor on distant planets.





"We get a lot more
return on our investment if we know when and where to look," Eric Ford, a university
teacher of astrophysics and co-author of the recent study, said to Business
Insider.





Ford's team defined an Earth-like
planet as being anyplace from three-quarters to one-and-a-half times the size
of Earth, and revolving around its star every 237 to 500 days. That is probably
inside the star's habitable zone – the "kind of orbital distances at which
the planets could sustain liquid water on their surfaces," as Ford said it
in a media statement.





"For astrophysicists
who are trying to find out what is a good design for the next major space
observatory, this piece of info is an essential part of that design
process," he said.





5 to 10 billion planets like
Earth



The scientists' approximation
is established on data from NASA's Kepler space telescope. Launched in 2009,
the telescope used what is recognized as the transit method to discover worlds
outside our Solar System. It observed over 530,000 stars for tiny inclines in a
star's brightness that could be produced by a planet passing in front of it –
transits, in other words. This work changed our understanding of the galaxy.
Kepler discovered more than 2,600 exoplanets, revealed that there are more
planets than stars in the Milky Way, and gave students new understanding into
the diversity of planet types.





The telescope also permitted
researchers to confirm for the first time that many exoplanets are like Earth. The
telescope retired last
year after it ran out of fuel, but passed the planet-hunting mission to the
Transiting Exoplanet Survey Satellite (TESS), which launched in April 2018. General,
Kepler's outcomes proposed that 20% to 50% of the stars observable in the night
sky had Earth-like planets in their habitable zones.





But Ford's team did not want
to estimate the number of Earth-like planets in the galaxy based only on the
exoplanets Kepler discovered, as the transit method is only good at discovering
large planets adjacent to their stars (since they block out more light). It is
not great, though, at discovering small planets away from their stars. Plus,
Kepler's method was biased toward small, dim stars about one third the mass of
our Sun.





So to evaluate how many
planets Kepler might have missed, the scientists made computer simulations of theoretical
universes of stars and planets, based on a combination of Kepler's planet record
and an analysis of our galaxy's stars from the European Space Agency's Gaia spacecraft.
Then the scientists' program "observed" those stars as Kepler would
have. The simulation provided the researchers a sense of how many exoplanets in
each hypothetical universe Kepler would have discovered, and which kinds.





They could then compare that
data to what the real Kepler telescope discovered in our universe to evaluate
the quantity of Earth-sized planets in the habitable zones of Sun-like stars.





"There are substantial
uncertainties in what range of stars you label 'Sun-like,' what range of
orbital distances you consider to be 'in the habitable zone,' what range of
planet sizes you consider to be 'Earth-like,'" Ford said. "Given
those uncertainties, both 5 and 10 billion are reasonable estimates."





Improving the search for
aliens



The next step in the hunt
for alien life is to study possibly habitable planets to figure out what they are
made of.





"Researchers are mainly
interested in searching for biomarkers – molecules suggestive of life – in the
atmospheres of approximately Earth-size planets," Ford said.





Even if a planet is in a
star's habitable zone, it still requires a considerable atmosphere to trap sufficient
heat to bear liquid water on its surface. Researchers can compute the
composition of an exoplanet's atmosphere by calculating how its star's light
behaves as it passes through. This is where Ford's study comes into play: If
Earth-like worlds are plentiful, there could be sufficient of them close by for
NASA researchers to study with a smaller, inexpensive telescope. If all the
Earth-y worlds are far away, however, NASA would need to depend on more
far-reaching telescopes. The scientists suggested that future space missions
plan for a range of probable incidences of Earth-like planets – between one for
every 33 Sun-like stars and one for every two sun-like stars.





"One of the important
things here is not just giving a single number but understanding the range of
possibilities," Ford said. "So that people who have to make decisions
could hope for the best and plan for the worst and still be able to come up
with a solid scientific strategy."





This article was originally published by Business
Insider
.

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