Evidence for a significant new class of supernova has been found with the European Space Agency's XMM-Newton and NASA's Chandra X-ray Observatory. These results strengthen the case for a population of stars that evolve rapidly and are destroyed by thermonuclear explosions. Such 'prompt' supernovas could be valuable tools for probing the early history of the cosmos.

The COROT mission is scheduled for launch on the 27th December 2006, from Baikonur in Kazakhstan. COROT will detect planets orbiting around other stars and probe the secrets of stellar interiors as never before.

Stars die when they have exhausted the fuel in their centres and until now it has been believed, that stars could only die in two ways - one way for the smaller and medium size stars and one way for the very massive stars. Our sun is a middle size star. When stars that are smaller than our sun or up to 8 times more massive than the sun die, they expel the outer layers and leave behind a white dwarf in the centre

A new, stunning image of the cosmic spider, the Tarantula Nebula and its surroundings, finally pays tribute to this amazing, vast and intricately sculpted web of stars and gas. The newly released image, made with ESO's Wide Field Imager on the 2.2-m ESO/MPG Telescope at La Silla, covers 1 square degree on the sky and could therefore contain four times the full Moon.

Nature has again thrown astronomers for a loop. Just when they thought they understood how gamma-ray bursts formed, they have uncovered what appears to be evidence for a new kind of cosmic explosion. These seem to arise when a newly born black hole swallows most of the matter from its doomed parent star.

Faint cosmic glow appears to be remnant radiation from first stars or black holes born in our universe

According to the "Strange Matter Hypothesis," which gained popularity in the paranormal 1980's, nuclear matter, too, can be strange. The hypothesis suggests that small conglomerations of quarks, the infinitesimally tiny particles that attract by a strong nuclear force to form neutrons and protons in atoms, are the true ground state of matter. The theory has captivated particle physicists worldwide, including one of Washington University's own.

The stars and gas which are seen in galaxies account for only a few percent of the gravitating material in the Universe.

How heavy can a star be? This conundrum has haunted astronomers for decades. Theory indicates that there should be an upper stellar mass limit somewhere between 120 and 300 solar masses. Even though heavy stars are very bright, measurements of their masses can be complicated.