Astronomers using NASA’s Hubble Space Telescope have found the building blocks of solid exoplanets that are capable of having substantial amounts of water. This rocky debris, currently orbiting a white dwarf star called GD 61, is considered a relic of an exoplanetary system that survived the burnout of its parent star. The finding suggests [continue reading]
CfA astronomers made a remarkable and fortuitous discovery in 2005: an extremely fast moving star, clocked going over three million kilometers an hour. It appears to have been ejected from the vicinity of the galactic center’s supermassive black hole around 80 million years ago by powerful gravitational effects as it swung past the black [continue reading]
Astronomers have used ESO’s Very Large Telescope, along with radio telescopes around the world, to find and study a bizarre stellar pair consisting of the most massive neutron star confirmed so far, orbited by a white dwarf star. This strange new binary system allows tests of Einstein’s theory of gravity — general relativity — [continue reading]
Even dying stars could host planets with life – and if such life exists, we might be able to detect it within the next decade. This encouraging result comes from a new theoretical study of Earth-like planets orbiting white dwarf stars. Researchers found that we could detect oxygen in the atmosphere of a white [continue reading]
January 17, 2013 Fleming 1, a planetary nebula in Centaurus Image Credit: ESO/H. Boffin Fleming 1 is a planetary nebula that lies about 10,000 light-years away in the constellation of Centaurus, while moving away from us at approximately 28.6 kilometers per second. It is named after the Scottish astronomer Williamina Fleming, who discovered the nebula [continue reading]
An international team of nuclear astrophysicists has shed new light on the explosive stellar events known as novae. Artistic view of a nova explosion depicting the binary stellar system. Image Credit: David A Hardy and STFC These dramatic explosions are driven by nuclear processes and make previously unseen stars visible for a short time. [continue reading]