One of the most interesting set of planets discovered in this study is a system of four
potentially rocky planets, between 20 and 50 percent larger than Earth, orbiting a star less than half the size and with less light output than the Sun.
The Gliese 667C system is the first example of a system where such a low - mass star is seen to host several
potentially rocky planets in the habitable zone.
Some 39 light - years away, this sun has three
potentially rocky planets in its habitable zone and — bonus — four additional rocky planets.
Not exact matches
«In order to figure out whether these
planets, the most common in our galaxy, are mostly
rocky and
potentially habitable or mostly gaseous and probably not very habitable, we have to perform these measurements to learn where exactly this transition occurs and how broad it is.»
San Francisco State University astronomer Stephen Kane and an international team of researchers have announced the discovery of a new
rocky planet that could
potentially have liquid water on its surface.
By the time Webb is operational, Clampin says, another NASA mission, the Transiting Exoplanet Survey Satellite (TESS), slated for launch in 2017, will already be producing a short list of other
potentially habitable
rocky planets around nearby small stars.
On Aug. 24, 2016, astronomers announced a
potentially habitable, likely
rocky planet orbiting the star nearest us, Proxima Centauri.
Astronomers plan to measure masses for at least 50 TESS
planets that are smaller than Neptune in the hopes that many of them will have
rocky, and therefore
potentially habitable, surfaces.
In the Solar System, the asteroid belt contains the leftover building blocks for the terrestrial
planets Mercury, Venus, Earth, and Mars, so planetary scientists study the asteroids to gain a better understanding of how
rocky, and
potentially habitable
planets are formed.
To qualify as
potentially life - friendly, a
planet must be relatively small (and therefore
rocky) and orbit in the «habitable zone» of its star, which is loosely defined as a location where water can exist in liquid form on a world's surface.
Ever since the first exoplanet was discovered in 1996, astronomers have been scanning the heavens for another Earth: a
rocky planet orbiting its star at just the right distance for it to harbor liquid water and thus,
potentially, life.
According to models, the TRAPPIST - 1 system contains three
planets in the habitable zone, making it the record holder for stars we know of with
rocky planets that could
potentially support liquid water, Kaltenegger explained.
As it happens, there are star systems where
rocky planets — and
potentially habitable ones at that — are close enough to their star to transit quite frequently.
Observations of exoplanets have also shown that
rocky, and
potentially habitable,
planets are just as common around red dwarfs as yellow dwarfs.
SAN FRANCISCO, April 17, 2014 — San Francisco State University astronomer Stephen Kane and an international team of researchers have announced the discovery of a new
rocky planet that could
potentially have liquid water on its surface.
These molecules are the products of the
planet's composition, chemistry and — in the case of
rocky planets — geological and
potentially biological processes.