Habitable zone super Jupiter-sized exoplanet found in Milky Way bulge

October 17, 2013 by Bob Yirka, Phys.org report
Light curve of MOA-2011-BLG-293 from Yee et al. (2012). Credit: arXiv:1310.3706 [astro-ph.EP]

(Phys.org) —A multinational team of astronomers has discovered the existence of a large (four times the size of Jupiter) sized exoplanet lurking in the Milky Way bulge—the first discovery of its kind. The team has reported on their findings in a paper they've uploaded to the preprint server arXiv.

The researchers on the project were using technology to study microlensing events—where one star passes in front of another allowing measurements to be taken of the star that is closer, due to magnification brought about by gravity (bending of spacetime). Measuring such light allows scientists to note transient brightening which reveals information not only about the star but about any planets that may be orbiting it. The overall objective is to find of the right size with planets of the right kind orbiting at just the right distance to allow for the possible existence of life—known commonly as the habitable or Goldilocks zone.

The microlensing event that led to the has been named MOA-2011-BLG-293Lb—observations were made from three facilities, one of which, the Keck facility in Hawaii was able to follow the initial discovery with a closer analysis that revealed finer details of the star and its . The newly discovered planet has not yet been named, but because it's a gas giant, there is little hope that it might harbor life on its surface. Microlensing isn't precise enough to discern whether the planet has any moons, but if it does, the researchers suggest, they could perhaps, because they too would exist in the , possibly allow for life.

The discovery marks the first time a habitable zone exoplanet has been found in the dense patch of the Milky Way known as the bulge and further highlights just how sophisticated Earth measuring devices have become—the new exoplanet is approximately 25,000 light years away. The star was found to be a G type of dwarf, a little smaller than our own sun, while the exoplanet was found to be just 1.1 AU from its star (1 AU is the distance of Earth from our sun). The researchers report that because of the small distance there is a 53 percent chance that the planet lays in the habitable zone, though it's also likely to be near its outer edges.

Explore further: How common are earths around small stars?

More information: MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone, arXiv:1310.3706 [astro-ph.EP] arxiv.org/abs/1310.3706

We used Keck adaptive optics observations to identify the first planet discovered by microlensing to lie in or near the habitable zone, i.e., at projected separation r⊥=1.1±0.1AU from its ML=0.86±0.06M⊙ host, being the highest microlensing mass definitely identified. The planet has a mass mp=4.8±0.3MJup, and could in principle have habitable moons. This is also the first planet to be identified as being in the Galactic bulge with good confidence: DL=7.7±0.44 kpc. The planet/host masses and distance were previously not known, but only estimated using Bayesian priors based on a Galactic model (Yee et al. 2012). These estimates had suggested that the planet might be a super-Jupiter orbiting an M dwarf, a very rare class of planets. We obtained high-resolution JHK images using Keck adaptive optics to detect the lens and so test this hypothesis. We clearly detect light from a G dwarf at the position of the event, and exclude all interpretations other than that this is the lens with high confidence (95%), using a new astrometric technique. The calibrated magnitude of the planet host star is HL=19.16±0.13. We infer the following probabilities for the three possible orbital configurations of the gas giant planet: 53% to be in the habitable zone, 35% to be near the habitable zone, and 12% to be beyond the snow line, depending on the atmospherical conditions.

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not rated yet Nov 05, 2013
Likely the moons around this planet will be warm, from internal heating from tidal forces exerted by the host planet, and not only by the central star but also by reflected light from the host planet as well. That host planet would be a gas giant and highly reflective. There is some small possibility that the host planet may also be a 'brown dwarf' and provide some heat as well. With life being everywhere space, floating in and on various ejecta, asteroids, and transitory exobodies, the seeding of these moons able to be seeded is assumed. The presence of life becomes logically plausible on these moons, and the next questions are then how well it has developed over time and in what forms.

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