Extremely massive exoplanet discovered in the Milky Way's bulge

November 6, 2017 by Tomasz Nowakowski report
Light curve of OGLE-2016-BLG-1190. The data points are colored as indicated by observatory in the top panel, which shows the full light curve. Credit: Ryu et al., 2017.

(Phys.org)—As a result of NASA's Spitzer Space Telescope observations of a microlensing event, astronomers have found an extremely massive alien world circling a star located in the Milky Way's bulge. The newly discovered planet, designated OGLE-2016-BLG-1190Lb, is the first Spitzer microlensing exoworld residing in the galactic bulge. The finding was presented October 27 in a paper published on arXiv.org.

Microlensing is very useful technique for detecting alien worlds in the inner galactic disk and bulge, where it is difficult to search for with other methods. It facilitates the discovery of distant objects by using background as flashlights. If a star moves in front of an another star, the light from the is bent by the gravitational pull of the nearer star and the more distant star is magnified. Microlensing does not rely on the light from the host stars; thus, it can detect planets, even when the host stars cannot be detected.

OGLE-2016-BLG-1190 was discovered in June 2016 as a event by the Optical Gravitational Lensing Experiment (OGLE) collaboration. OGLE is a Polish astronomical project based at the University of Warsaw, searching for dark matter and extrasolar planets. It utilizes the 1.3 meter Warsaw telescope mounted at the Las Campanas observatory in Chile.

Spitzer observed this microlensing event a few days after its discovery. An international team of researchers led by Yoon-Hyun Ryu of the Korea Astronomy and Space Science Institute in Daejon, South Korea, reports that these Spitzer observations detected a new, massive planet orbiting a dwarf star.

"We report the discovery of OGLE-2016-BLG-1190Lb, which is likely to be the first Spitzer microlensing planet in the galactic bulge/bar, an assignation that can be confirmed by two epochs of high-resolution imaging of the combined source-lens baseline object," the astronomers wrote in the paper.

According to the study, OGLE-2016-BLG-1190Lb appears to be an extremely massive planet with a mass of about 13.4 Jupiter masses. Such high mass puts the object right at the deuterium burning limit—the conventional boundary between planets and brown dwarfs. Therefore, the researchers do not exclude the possibility that the newly found planet could be a low-mass brown dwarf.

OGLE-2016-BLG-1190Lb orbits its parent star approximately every three years at a distance of about 2.0 AU. The host is a G dwarf with a mass of 0.89 solar masses. The system is located some 22,000 light years away from the Earth.

The authors of the paper emphasize that OGLE-2016-BLG-1190Lb is the first exoplanet discovered thanks to microlensing and the Spitzer spacecraft. Moreover, what makes this planet remarkable is that it is right at the edge of the so-called brown dwarf desert, what raises questions about whether such objects are really planets or failed stars.

"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' (by formation mechanism) and therefore reacts back upon its role tracing the galactic distribution of planets," the paper reads.

Explore further: Gas giant planet discovered near the Milky Way's bulge

More information: OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary, arXiv:1710.09974 [astro-ph.EP] arxiv.org/abs/1710.09974

Abstract
We report the discovery of OGLE-2016-BLG-1190Lb, which is likely to be the first Spitzer microlensing planet in the Galactic bulge/bar, an assignation that can be confirmed by two epochs of high-resolution imaging of the combined source-lens baseline object. The planet's mass M_p= 13.4+-0.9 M_J places it right at the deuterium burning limit, i.e., the conventional boundary between "planets" and "brown dwarfs". Its existence raises the question of whether such objects are really "planets" (formed within the disks of their hosts) or "failed stars" (low mass objects formed by gas fragmentation). This question may ultimately be addressed by comparing disk and bulge/bar planets, which is a goal of the Spitzer microlens program. The host is a G dwarf M_host = 0.89+-0.07 M_sun and the planet has a semi-major axis a~2.0 AU. We use Kepler K2 Campaign 9 microlensing data to break the lens-mass degeneracy that generically impacts parallax solutions from Earth-Spitzer observations alone, which is the first successful application of this approach. The microlensing data, derived primarily from near-continuous, ultra-dense survey observations from OGLE, MOA, and three KMTNet telescopes, contain more orbital information than for any previous microlensing planet, but not quite enough to accurately specify the full orbit. However, these data do permit the first rigorous test of microlensing orbital-motion measurements, which are typically derived from data taken over <1% of an orbital period.

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Molecular hydrogen
not rated yet Nov 07, 2017
I would like to see more study for exoplanets in Andromeda galaxy as this will catch us up in 4 billions years while the Suns fuel depletes in 5 billion years gives us a good time to plan to jump ship
antialias_physorg
5 / 5 (3) Nov 07, 2017
Therefore, the researchers do not exclude the possibility that the newly found planet could be a low-mass brown dwarf.

I wonder if there could be something like a pulsating brown dwarf. Just above the deuterium burning limit, but once fusion starts the radiation pressure causes it to expand to the point where fusion stops...upon which it would collapse again under its own gravity until the deuterium burning limit is reached again.

..I'm not sure how fast such a system would settle into a stable state (just barely on either side of the limit) or whether the size and inhomogeneity of a star would allow for this to continue to happen for some time.
MarsBars
5 / 5 (1) Nov 07, 2017
MH - how stupendously (and ludicrously) optimistic of you to imagine that homo sapiens will still be around 4 billion years from now.
Molecular hydrogen
1 / 5 (1) Nov 07, 2017
Of course they will but maybe not in the form of present day and to be honest the only way to interstellar travel is to send out our DNA in ships to be re animated by being reprinted out once arrived at our destination ...
jonesdave
5 / 5 (4) Nov 07, 2017
I would like to see more study for exoplanets in Andromeda galaxy as this will catch us up in 4 billions years while the Suns fuel depletes in 5 billion years gives us a good time to plan to jump ship


And why would we need to go all the way to Andromeda, when we have our own galaxy full of stars to choose from?
Gigel
4 / 5 (1) Nov 08, 2017
I would like to see more study for exoplanets in Andromeda galaxy as this will catch us up in 4 billions years while the Suns fuel depletes in 5 billion years gives us a good time to plan to jump ship

In1 billion years it is said the Sun will heat the Earth and accelerate chemical processes at its surface, so that we will lose the carbon dioxide with catastrophic consequences (no more plants). But then again, complex life existed for far less than 1 billion years, so that horizon is still a long time from now on the human or even life scales.

Let's hope we don't blow something up until then.

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