Astronomers have discovered a massive alien world circling a star located 22,000 light years away, at the centre of the Milky Way’s bulge.
The object, dubbed OGLE-2016-BLG-1190Lb, is 13 times the size of Jupiter and is so vast that experts are unsure whether it is even a planet.
Experts used Nasa’s Spitzer Space Telescope and the light-warping effects of gravity to uncover the mysterious celestial body.
Although it is orbiting its own star, researchers say ‘Planet X’ may in fact be a failed star, known as a brown dwarf.
Astronomers have discovered a massive alien world circling a star located 22,000 light years away, at the centre of the Milky Way. The object is 13 times the size of Jupiter and is so vast, experts believe it may be a failed brown dwarf star (artist’s impression)
An international team of researchers, led by Yoon-Hyun Ryu of the Korea Astronomy and Space Science Institute in Daejon, South Korea, reported the find in a paper published on the online print repository Arxiv.org.
It was made using a technique known as microlensing, that facilitates the discovery of distant objects by using background stars as flashlights.
OGLE-2016-BLG-1190Lb was discovered in June 2016 by the Optical Gravitational Lensing Experiment (OGLE) collaboration.
OGLE is a Polish astronomical project based at the University of Warsaw, which is searching the universe for dark matter and extrasolar planets.
It uses the five foot (1.3 metre) Warsaw telescope mounted at the Las Campanas observatory in Chile.
The team used readings taken from Nasa’s Spitzer space telescope which has uncovered a number of microlensing events, to narrow their search.
Writing in the paper, its authors said: ‘We report the discovery of OGLE-2016-BLG-1190Lb, which is likely to be the first Spitzer microlensing planet in the galactic bulge/bar.
‘It is precisely measured to be right at the edge of the brown dwarf desert.
‘This is somewhere between 13 and 14 Jupiter masses. OGLE-2016-BLG-1190Lb has about 13.4 Jupiter masses.
‘Since the existence of the brown dwarf desert is the signature of different formation mechanisms for stars and planets, the extremely close proximity of OGLE-2016-BLG-1190Lb to this desert raises the question of whether it is truly a “planet”.’
Brown dwarfs are thought to be the missing link between planets and stars, with masses up to 80 times that of Jupiter.
![OGLE-2016-BLG-1190 was discovered in June 2016 by the Optical Gravitational Lensing Experiment (OGLE) collaboration. This image shows the light curve readings as indicated by the observatory in the top panel, which shows the full light curve](https://i.dailymail.co.uk/i/pix/2017/11/10/11/46334BF100000578-0-image-a-30_1510314445001.jpg)
OGLE-2016-BLG-1190 was discovered in June 2016 by the Optical Gravitational Lensing Experiment (OGLE) collaboration. This image shows the light curve readings as indicated by the observatory in the top panel, which shows the full light curve
![The team used readings taken from Nasa's Spitzer space telescope (artist's impression), which has uncovered a number of microlensing events, to narrow their search](https://i.dailymail.co.uk/i/pix/2017/11/10/11/46334C1200000578-0-image-a-26_1510314406028.jpg)
The team used readings taken from Nasa’s Spitzer space telescope (artist’s impression), which has uncovered a number of microlensing events, to narrow their search
But their centres are not hot or dense enough to generate energy through nuclear fusion the way stars do.
OGLE-2016-BLG-1190Lb’s mass puts it right at the deuterium burning limit, the conventional boundary between planets and brown dwarfs.
Scientists have found that, for stars roughly the mass of our sun, less than one per cent have a brown dwarf orbiting within three AU.
One AU is the distance between Earth and the sun. This phenomenon is called the ‘brown dwarf desert.’
OGLE-2016-BLG-1190Lb orbits its parent star approximately every three years at a distance of about two AU.
The host is a yellow dwarf star, similar to our own Sun, that has 89 per cent of its mass.
The newly discovered planet aids scientists in their quest to figure out the distribution of planets in our galaxy.
Astronomers still don’t know whether there is a difference in the frequency of planets in the Milky Way’s central bulge compared to its disk, the pancake-like region surrounding the bulge.
OGLE-2016-BLG-1190Lb is located in the disk, as are three planets previously detected through microlensing by Nasa’s Spitzer Space Telescope.