NASA Spitzer Space Telescope discovered that the exoplanet 55 Cancri e has a lower density, as previously reported. Astronomers first discovered 55 Cancri e in 2004, and continued investigation of the exoplanet has shown it to be a truly bizarre place.
Through the project, “Planet Hunters,” which was created for a detailed analysis of all data obtained by Kepler telescope, participants of this project was lucky to find two previously unknown exoplanets.
Scientists from the University of Geneva in Switzerland informed that they found a planet that may be habitable. This planet is located from us at 36 000 light years. Potentially habitable planet is located in orbit of the star HD 85 512.
Astronomers discovered the darkest alien planet in the galaxy, known as TrES-2b. The distant exoplanet TrES-2b is darker than the blackest coal. This planet belongs to a class of hot Jupiters, gas giants, orbit of which are very close to the star.
Astronomers have discovered that one of the planets in binary star system 55 Cancri is potentially habitable.The study’s authors, Kaspar von Braun of the California Institute of Technology and his colleagues describe the properties of the binary star system 55 in the constellation of Cancer, called 55 Cancri f.
More recently, scientists announced the discovery of new planets near the triple star HD 132 563.The main star, HD 132563A, is binary. The study conducted by a team of scientists led by Silvano Desidera of the Astronomical Observatory of Padua, Italy. The new planet moves on the orbit of the second star in the system HD 132563B. As in the binary component of the main star, the new planet was detected by spectral analysis.
Computer modeling shows that more than 5% of the giant exsoplanets may have habitable moon, if these planets orbit at a distance from their stars.This computer modeling developed by Simon Porter and his colleagues at Lowell Observatory in Arizona, includes 12 000 hypothetical Earth-sized exoplanets who had been captured by gas giants and became their satellites.
According to researchers from the U.S., UK and South Africa may be there are a pair of giant planets in a binary system UZ Ovens.In UZ includes white and red dwarfs, which are very close to each other. The substance, flowing from the red dwarf to companion , is heated and becomes a source of X-rays
An international team of astronomers has described a new exoplanet MOA-2009-BLG-266Lb, which is only 10 times larger than Earth by mass. Scientists have acted according to the method of gravitational microlensing, which can detect low-mass planets in wide orbits.As it turned out, the mass of the star is 0,56 ± 0,09 sunny. Planet moves around its orbit with semi-major axis of 3.2 (+1.9, -0.5) а.e.,making one revolution in 7.6 (+7.7, -1.4) years.MOA-2009-BLG-266Lb was one of the first low-mass exoplanet located in “snow line”, conventional boundary, which takes place at such a distance from the luminary, where the temperature allows the existence of hydrogen compounds (water, ammonia, methane) in the form of solid ice particles.