A hot potential habitable exoplanet around Gliese 163

Aug 31, 2012 by Abel Mendez Torres
Artistic representation of Gliese 163c as a rock-water world covered with a dense cloud layer (left). It looks reddish, instead of white, due to the reflected light from its red dwarf parent star. Actual false-color image of the Gliese 163 star taken by NASA's WISE Mission (center). Map with the location of Gliese 163 in the constellation Dorado (right). CREDIT: PHL @ UPR Arecibo, NASA/IPAC IRSA, IAU, Sky & Telescope.

A new superterran exoplanet (aka Super-Earth) was found in the stellar habitable zone of the red dwarf star Gliese 163 by the European HARPS team. The planet, Gliese 163c, has a minimum mass of 6.9 Earth masses and takes nearly 26 days to orbit its star. Superterrans are those exoplanets between two and ten Earth masses, which are more likely composed of rock and water. Gliese 163 is a nearby red dwarf star 50 light years away in the Dorado constellation. Another larger planet, Gliese 163b, was also found to orbit the star much closer with a nine days period. An additional third, but unconfirmed planet, might be orbiting the star much farther away.

Gliese 163c could have a size between 1.8 to 2.4 radii, depending if it is composed mostly of rock or water, respectively. It receives on average 40% more light from its parent star than Earth from the Sun, making it hotter. In comparison, Venus receives 90% more light from the Sun than Earth. We do not know the properties of the atmosphere of Gliese 163c but, if we assume that it is a scaled up version of Earth's atmosphere, then its surface temperature might be around 60°C. Most complex (plants, animals, and even humans) are not able to survive at temperatures above 50°C, however, plenty of extremophilic forms can thrive at those temperatures or higher.

The detection of potential habitable exoplanets is pacing up. There are now six including the debated Gliese 581g, most of them detected just in the last year. Four of these bodies, Gliese 581d, Gliese 667Cc, Gliese 581g, and now Gliese 163c are around red dwarfs (M-star). HD 85512 is around a K-star (a middle star between the smaller red dwarfs and the Sun). Only -22b is around a Sun-like star (G-star). All of these planets are bigger than Earth but still considered potentially habitable, at least to simple life forms. Scientists are trying to construct better ground and space observatories in the next decades to be able to detect smaller worlds, those more resembling Earth. The Habitable Exoplanet Catalog of the Planetary Habitability Laboratory @ UPR Arecibo (phl.upr.edu), which was not involved in the discovery, now includes and ranks Gliese 163c as number five in its main list of best objects of interest for life.

Current six potential habitable exoplanets ranked by similarity with Earth (Earth = 1.00). Four of these objects have been detected in the last year, from September 2011 to today. Gliese 163c is represented here as a rock-water world of 2.4 Earth radii, however, it could be as small as 1.8 Earth radii if composed mostly of rock, like Earth. CREDIT: PHL @ UPR Arecibo

The potential for habitable planets around stars has been and issue of much debate. Tidal effects on the planets around these stars might cause extra surface heating or even tidal locking (always giving the same face to its ). Also, these stars are more active and their stellar wind might erode planetary atmospheres much faster. These factors might preclude the potential for life on smaller planets but not for planets with thicker atmospheres, something expected for superterran planets. Our Solar System lacks an example of a superterran. Its eight planets are either the smaller terrestrial kind, like Earth, or the larger gas giants, like Jupiter. Understanding superterrans around red dwarf stars, a non Sun-like star, just adds to the challenge of assessing their habitability.

The NASA Kepler Mission has detected about 27 potential habitable exoplanets candidates out of their over 2,300 exoplanets that are waiting to be confirmed. Some of these bodies seem very Earth-like. Unfortunately, they are much farther away from us than Gliese 163 and it will be nearly impossible to determine if they are really habitable worlds by future observations. However, the statistical analysis of Kepler suggests that these planets are very common in the galaxy. Therefore, many more Earth-like worlds are waiting to be discovered in our solar neighborhood too, such as Gliese 163c.

The new around Gliese 163 were discovered by the European HARPS team leaded by Xavier Bonfils from the UJF-Grenoble/CNRS-INSU, Institut de Plane ́tologie et d'Astrophysique of Grenoble, France. Other participating scientists are from France, Germany, Portugal, Switzerland, and Belgium. Gliese 163c was announced by team member Thierry Forveille from the Observatoire de Grenoble during the International Astronomical Union session Formation, Detection, and Characterization of Extrasolar Habitable  from August 27th to 31st, 2012 in Beijing, China. A paper was submitted to the scientific journal Astronomy & Astrophysics.

Explore further: A star's early chemistry shapes life-friendly atmospheres

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geokstr
2.3 / 5 (3) Aug 31, 2012
IIRC, the transit method is mostly used now to find exoplanets, and they are finding a ton of them, but not that many earth sized and in the goldilocks zone.

However, keep in mind that Earth, at its distance from the sun, takes only 13 hours to transit, so it will be in transit only .0014% of any year. It is easy to see why many, many more are out there to be discovered, and will be, but we need to be monitoring every star for years to catch them in transit.

And that does not include the solar systems with planes so inclined that their planets will never transit from our perspective and thus will not be found with this method.

It is now highly probable that there are trillions of planets in this galaxy alone, and millions of earths in the goldilocks zone.

Torbjorn_Larsson_OM
not rated yet Aug 31, 2012
Reading the part on superterrans atmosphere likely mitigating the effects of orbiting red dwarfs in the habitable zone, I had to backtrack to the author. No wonder, it is Mr Habitable Index himself, always on top of things.

Except possibly the caveat on the surface temperatures. Now astrobiology has gone back and forth on this, but reasonably certain fossil thermometers like salt inclusions and carefully derived and calibrated cherts samples shows ~ 40 degC ocean temperature on Earth after ~ 1.5 billion years. This system's age is poorly constrained it seems, given as ">1 Gyears" (from HEC). So it is perhaps not unlike early Earth at all.

At the later time when the domains diversified with their respective cellular structures, which seems to after the atmosphere oxygenated (from trace fossils and genome dating), the temperature was probably quite like today or lower as we see global glaciations around that time. Hence mesophiles prefer 20 degC. No reason Gliese 163c life needs that.

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