Astronomers have discovered a giant exoplanet is larger than Jupiter, but has extremely low for this class of planets mass. But first and foremost interest to the object's composition, density similar to Styrofoam, which allowed him even jokingly nicknamed "fluffy planet."
The team that identifies the KELT-11b (the so-called planet), whose orbit is located about 320 light years from Earth, says that this "unusual" world is the third in density among the planets, which was exactly fitted their mass and radius. And this on all sides the strange sphere could tell us more about how appear and develop such unusual exoplanets.
"She is very inflated. Having only 1/5 the mass of Jupiter, she's almost 40% more, making it a density similar to a giant foam, covered with a dense atmosphere," — says astronomer Joshua pepper Lyaskovo from the University of Pennsylvania.
In Addition to the unusual density, the planet KELT-11b distinguished by the fact that wraps around sviryanki star KELT-11, which is in the process of transition to a red giant. This may indicate that in the framework of the fusion process the star began to burn hydrogen outside its core. Scientists say that for about the next 100 million years the outer layers of the atmosphere of the star KELT-11 will expand, and eventually star fully engulf the planet KELT-11b. Absorption will not take much time, since the planet is very close to the star. Complete revolution around its sun exoplanet makes less than 5 earth days.
But before his death, this "world of foam", thanks to the brightness of the star KELT-11, can tell scientists about the composition of its atmosphere. Astronomers say that the star of this system is the brightest in the sky of the southern hemisphere among famous stars, who thanks to the transit search, was discovered on the planet.
The Transit method of finding new exoplanets is one of the most popular among astronomers. Thanks to the passage of the planet between the star and our telescopes decreases the brightness of the observed stars. This indicates to scientists that in front of the star at this point might be exoplanet. However, in the case sviryanki star KELT-11 the decrease of the luminosity by the passage of the planet is so insignificant that astronomers did not immediately able to confirm the presence of planets with KELT (Kilodegree Extremely Little Telescope) – two robotic telescopes working in unison and in Arizona and South Africa.
"Open it was quite difficult. The original observation of the star with KELT showed only a slight change in the curve on the graph", — shared pepper website Phys.org last year, when astronomers first announced their discovery and were expecting critical analysis in their research.
"because the transit trip has had so little impact (level of brightness of the stars has fallen below 0.3 per cent), getting tested and fully validated data in the framework of the observations was difficult."
However, the new observations were able to confirm the existence of exoplanets KELT-11b in the system, and now the parameters of the luminosity of stars, which initially made it difficult to scientists to prove its existence, can be used to determine its atmosphere. Due to this data, the researchers plan to find out why this "tenoplasty" the world is so inflated in size. It is almost two times more than you might expect, given its mass and distance to the star.
"I think that KELT-11b offers us a great chance to better understand the mechanisms that result in the planet so swell", — said pepper.
"in addition, because the star system is in its transitional state, on the basis of these data we plan to better understand the behavior of planetary systems, whose lights are at the end of its life cycle".
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