News

Kepler-223 star system has four mini-Neptunes in synchronised orbits

A four-planet system orbiting the star Kepler-223 in the constellation Cygnus is actually a rarity: Its planets, all miniature Neptunes nestled close to the star, are orbiting in a unique resonance that has been locked in for billions of years. For every three orbits of the outermost planet, the second orbits four times, the third six times and the innermost eight times.

News

Possible exomoon signal found

Strong hints have been found of a possible exomoon candidate orbiting a gas giant planet over 4,000 light years away in the constellation of Cygnus the Swan. Should the moon be confirmed later this year by the Hubble Space Telescope, it will be the first moon ever discovered around a planet beyond our Solar System.

News

Warm Jupiters are not as lonely as expected

After analysing four years of observations from NASA’s Kepler space telescope, astronomers from the University of Toronto have given us our clearest understanding yet of a class of exoplanets called “warm Jupiters,” showing that many have unexpected planetary companions.

News

Understanding stellar adolescence through T-Tauri stars

A newborn star typically goes through four stages of adolescence. It begins life as a protostar, accreting material and developing a proto-planetary disc. Slowly, stellar winds and radiation blow away the surrounding shell of gas and dust. Next, when the surrounding envelope has cleared, is called the T-Tauri phase. Finally, accretion stops and the source’s radiation comes from the star’s photosphere.

News

A highly eccentric “hot Jupiter” exoplanet

Astronomers have observed the extreme temperature variations of HD 80606 b, a Jupiter-sized exoplanet with a highly eccentric, comet-like orbit that brings it scorchingly close to its parent star every 111 days. The researchers also calculated the planet’s rotation rate — the first exoplanet rotation rate ever obtained.

News

‘Cannibalism’ between stars

Stars are born inside a rotating cloud of interstellar gas and dust. Before finding itself on the star, however, most of the cloud lands onto a circumstellar disc forming around the star. The manner in which the material is transported through the disc onto the star, causing the star to grow in mass, has recently become a major research topic in astrophysics.