Hubble finds Mass of White Dwarf

Chris Bradshaw writes "The mass of the nearest white dwarf star to Earth has been measured accurately for the first time. from the article: 'Sirius B is just 12,000 km (7,500 miles) in diameter, similar to Earth, but its mass is 98% that of the Sun. Studying Sirius B has been difficult because of the bright light coming from its neighbour Sirius A, the "Dog Star." The results, published in the Monthly Notices of the Royal Astronomical Society, come from astronomers using the Hubble Space Telescope.'"

Comments

More on White Dwarfs...

[Cherita Chen]

It's important to note that with out supplemental information from other sources, this would not have been possible. another space-born observatory that has aided greatly in the study of white dwarfs Here

additionally, more can be found on the white dwarfs in general Here.

It'll be more interesting when they find..

[Anonymous Coward]

Mass of RED Dwarf

It's a shame...

[chrstphrb]

It is a shame that Hubble is on borrowed time...

http://washingtontimes.com/upi-breaking/20050420-1 25927-9641r.htm

Hubble

[jurt1235]

Although NASA (or the US goverment, it is all politics) does not want to fund Hubble anymore, the telescope proves that it is valuable every time again. Astronomers just need more time with the equipment to take more readings of an object so that they can catch the details. Is it an idea that a commercial company adopts the Hubble telescope and rents the time on the telescope out again to different agencies around the globe? The price for the adoption could be the operational cost of keeping Hubble in orbit in working order.

Interesting Background...

[guygee]

not mentioned in the article, at http://columbia.thefreedictionary.com/Sirius

Selected excerpt:

"Sirius A is about twice the size of the sun and about 20 times as luminous. It is also one of the nearest stars, lying at a distance of 8.7 light-years, so that it has been studied extensively. From an analysis of its motions, F. W. Bessel concluded (1844) that it had an unseen companion, which was later (1862) confirmed by observation. The companion, Sirius B, is a white-dwarf star and has also been the object of considerable study because it is the first white dwarf whose spectrum was found to exhibit a gravitational red shift, as predicted by the General Theory of Relativity."

Re:Time to update Wikipedia?

[meringuoid]

if the mass of a white dwarf goes over 1.4 solar masses, the gravitational collapse is strong enough to trigger a supernova explosion. In other words, at masses greater than the Chandrasekhar limit, the (inward) gravitational pressure overcomes the (outward) thermal/fusion pressure, thus causing a collapse and the ignition of most of the remainder of the stars fuel, thus the supernova explosion.

Right idea, wrong mechanism.

A white dwarf is not supported by thermal pressure, or by nuclear fusion; it is supported by degeneracy pressure between electrons, a consequence of the exclusion principle in quantum mechanics that forbids two electrons from occupying the same quantum state.

1.4 solar masses is correctly given as the critical point at which gravity prevails over the internal pressure; at this point, the star switches from degeneracy pressure between electrons to degeneracy pressure between neutrons, in the process dropping considerably more than the weight of the Sun from the size of the Earth to something more like the size of Belgium, through an enormously strong gravitational field. This releases an awful lot of energy, and is the main power source for such a supernova.

There's another type of supernova which is driven by fusion, but that's more typical of accretion systems in which the infalling matter has heated the white dwarf sufficiently to reignite fusion processes; then the fusion reaction is an uncontrolled runaway and can wholly disrupt the star.