The solitary life of this newly
discovered planet, with the catchy name PSO J318.5-22, has astronomers
excited.
Only 80 light-years from Earth,
the 12 million-year-old planet has properties similar to those of gas-giant
planets orbiting young stars.
But because it is floating alone
through space, rather than around a host star, astronomers can study it much
more easily.
"We have never before seen an
object free-floating in space that looks like this," said Dr. Michael Liu of the
Institute for Astronomy at the University of Hawaii at Manoa, who led the
international team that discovered the planet.
"It has all the characteristics
of young planets found around other stars, but it is drifting out there all
alone. I had often wondered if such solitary objects exist, and now we know they
do." While about a thousand planets
have been discovered outside our solar system in the past decade by indirect
means -- such as observing the wobbling or dimming of their host stars as they
orbit -- only a handful of new planets have been directly imaged, all of them
around young stars, according to a release from the Institute for Astronomy. Young stars are those less than
200 million years old.
PSO J318.5-22's solitary
existence and its similarity to those directly observed planets makes it a rare
find. "Planets found by direct imaging
are incredibly hard to study, since they are right next to their much brighter
host stars. PSO J318.5-22 is not orbiting a star so it will be much easier for
us to study," said Dr. Niall Deacon of the Max Planck Institute for Astronomy in
Germany and a co-author of the study.
"It is going to provide a
wonderful view into the inner workings of gas-giant planets like Jupiter shortly
after their birth." The astronomers stumbled across
it as they sifted through a mountain of data produced by the Pan-STARRS 1 (PS1)
wide-field survey telescope on Haleakala, Maui.
The planet, which has only six
times the mass of Jupiter, was identified by its faint and unique heat
signature. The astronomers were actually
searching for failed stars known as brown dwarfs when they came across PSO
J318.5-22, which stood out because of its red color.
Subsequent infrared observations
using other telescopes in Hawaii showed it was no brown dwarf, but rather a
young, low-mass planet. By monitoring the planet's
position for the next two years, using the Canada-France-Hawaii Telescope, the
team was able directly to measure its distance from Earth.
This means the astronomers have
placed it within a collection of young stars called the Beta Pictoris moving
group that formed about 12 million years ago. The star that lends its name to
the group, Beta Pictoris, has another young gas-giant planet in orbit around it,
the astronomers say. But PSO J318.5-22, which appears
to be even lower in mass than that planet, continues to wend its solitary way
through the universe, unattached to any star.
Of course a planet is known as an object that orbits another dominant object, so is this really a planet or a 'micro' Brown Dwarf? I would say it is not a 'planet' as we would call one, but a remnant from stellar formation that found itself out in space alone.
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