Hubble finds Mass of White Dwarf 126
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.'"
More on White Dwarfs... (Score:5, Informative)
additionally, more can be found on the white dwarfs in general Here [nasa.gov].
Re:More on White Dwarfs... (Score:2, Informative)
Re:More on White Dwarfs... (Score:1)
More on Karma Whoring... (Score:3, Funny)
More on Anonymous Coward... (Score:2, Funny)
Re:More on Karma Whoring... (Score:1)
Re:More on Karma Whoring... (Score:2)
Re:More on Karma Whoring... (Score:2)
Relax, it's Wiki. If you don't like it, just change it yourself.
Something like "predictable, emotive knee-jerk reactions mixed with the kind of homogenous racism and misogyny we have learned to expect from the internet."
It will be months before anyone notices, then Wired will have something else to write articles on to make t
It'll be more interesting when they find.. (Score:5, Funny)
Re:It'll be more interesting when they find.. (Score:2, Insightful)
Re:It'll be more interesting when they find.. (Score:1)
Re:It'll be more interesting when they find.. (Score:2)
Is there anyone that can comment intelligently on this?
Re:It'll be more interesting when they find.. (Score:5, Informative)
It's a shame... (Score:5, Interesting)
http://washingtontimes.com/upi-breaking/20050420-1 25927-9641r.htm [washingtontimes.com]
Re:It's a shame... (Score:5, Insightful)
Shame (Score:1, Insightful)
Re:Mods wake up (Score:3, Funny)
Re:Mods wake up (Score:2)
Re:Mods wake up (Score:2)
The Nommo are ancestral spirits (sometimes referred to as deities) worshipped by the Dogon tribe of Mali, Africa. The word Nommos is derived from a Dogon word meaning, "to make one drink"
Considering how the slashdot mods tapped into this thread and harvested 2-3 Karma pints^^^^^points from every contributor, yes, it does seem appropriate
The Dogon reportedly related to Griaule and Dieterlen a belief that the Nommos were inhabitants of a world circling the star Sirius
Oh, yeah and that too.
Re:Mods wake up (Score:2)
Hubble (Score:5, Insightful)
Re:Hubble (Score:2)
I don't even want to defend NASA's decision (I really don't know the tradeoffs well enough), but merely observing that Hubble is still useful tells you little about whether it makes sense to continue funding it. The real question is whether the cost/benefit calculations work out overall. In particular, is it worth trying to fix Hubble again and again, rathe
Re:Hubble (Score:2)
Re:Hubble (Score:5, Insightful)
The shuttle is not necessary, nor is the not yet designed or built robotic servicing capability. The Hubble Origins Probe could be in orbit by the time the original fails, continuing and extending the original mission while the James Webb mission design, construction, and launch is completed.
Additionally, if the US ever figures out how to put people back in space, or really does design robotic satellite repair capability the is nothing preventing the Hubble Origins Probe from having an extremely long and productive life.
Re:Hubble (Score:4, Insightful)
It has to be cheaper just to build another one than to build a robotic telescope repair system, and launch that!
Re:Hubble (Score:2)
Figure (Score:1)
Re:Hubble (Score:2)
If it's such a boon to mankind, convince some multigajillionaire to buy it for naming rights. Instead of the "Hubble Space Telescope" we could be getting this sort of data from the U2 Space Telescope or the Bjorn Bayley Space Telescope.
Re:Time to update Wikipedia? (Score:2)
Actually, I may have spoken too soon:
Many white dwarfs are approximately the size of the Earth, typically 100 times smaller than the Sun. They may have the same mass as the Sun and so are very compact.
Do they really vary in density that much?
Re:Time to update Wikipedia? (Score:2, Informative)
The upper limit, known as the Chandrasekhar limit, for a white dwarf is 1.4 solar masses (more or less).
Re:Time to update Wikipedia? (Score:2)
Just to expand that a bit, 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
Re:Time to update Wikipedia? (Score:5, Informative)
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.
Re:Time to update Wikipedia? (Score:2, Informative)
Re:Time to update Wikipedia? (Score:3, Informative)
What type of supernova? Simply collapsing to a neutron star doesn't *cause* a supernova, although a neutron star can be a supernova remnant.
It sounds like you're saying that if you have a white dwarf sitting there, and it accretes mass from some other source, like a binary companion, when its mass grows to be greater than the C-limit, it collapses into a neutron star, and that the energy released in the collapse generat
Re:Time to update Wikipedia? (Score:1)
Re:Time to update Wikipedia? (Score:2)
Re:Time to update Wikipedia? (Score:4, Informative)
Re:Time to update Wikipedia? (Score:2)
No, that's not right. If the dwarf collapses to, say, a neutron star, energy will be liberated when the radius of the star decreases. The change in gravitational potential is negative, so that extra energy has to go somewhere. This fuels Type 2 supernovas. I'm just not sure where that energy fits into the Type 1a.
I've heard that it might be that no neutron star is formed in 1a supernovas (the star is jus
Re:Time to update Wikipedia? (Score:2)
The iron core of a core-collapse supernova progenitor (similar to a white dwarf in size and mass, but made of un-fusable iron) has negative gravitational energy. The 12-k
Re:Time to update Wikipedia? (Score:5, Informative)
No, white dwarfs do become fusion-powered supernovae, not gravity-powered. IAAA (I am an astrophysicist.)
A white dwarf becomes a Type Ia supernova when, at around 1.4 solar masses, the pressure at the center reaches the point where it can burn by fusion the carbon-nitrogen-oxygen left over from previous rounds of burning. This leads to a fusion-driven explosion that gets no net energy from gravitational collapse, leading to an expanding gas cloud that is largely hot iron-group elements.
There is another class of supernova that is gravitationally driven. Core collapse supernovae are produced when a massive star (>8 solar masses, last I heard) has burned 1.4 solar masses at its center to iron. (The 1.4 solar mass value is semi-coincidental with that in the previous paragraph, based on similar but not identical physics.) This is a gravity-powered supernova that blows the outer parts of the core away, leaving a neutron star or black hole where the core was.
There is no way for a white dwarf to become a core collapse supernova, the fusion kicks in and blows it apart before that happens.
Re:Time to update Wikipedia? (Score:2)
Re:Time to update Wikipedia? (Score:3, Informative)
Do they really vary in density that much?
Yes. White dwarfs vary in density a whole lot; degenerate gases behave quite oddly. If you add matter to a white dwarf, it actually gets a little smaller. The limit is about 1.4 solar masses, at which point the white dwarf collapses to form a neutron star.
Re:Time to update Wikipedia? (Score:2)
Re:Time to update Wikipedia? (Score:1)
Very recently, Superman was able to easily support 200 quintillion tons with one arm, no straining. This is roughly 1/30,000th of the mass of the Earth itself. (Hence he could, with effort, actually move the earth, and without taking eons to slowly accelerate it.) Yes, he was over-amped on sun juice, and may be "dying", but his strength was only up by 3x over its normal level according to the poi
Re:Time to update Wikipedia? (Score:2)
Does anyone know?
Re:Time to update Wikipedia? (Score:2)
Interesting Background... (Score:5, Informative)
not mentioned in the article, at http://columbia.thefreedictionary.com/Sirius [thefreedictionary.com]
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:Interesting Background... (Score:2, Informative)
Re:Interesting Background... (Score:3, Insightful)
Re:Interesting Background... (Score:1)
Re:Interesting Background... (Score:1)
Re:Interesting Background... (Score:2)
Re:Interesting Background... (Score:1)
OK, so would that mean that to some degree, light leaving the sun is slightly red shifted on the way out, and slightly blue shifted when we see it on earth? Would a telescope at one of the Lagrange points not have that blue
Re:Interesting Background... (Score:2)
I guess a telescope at an L-point would indeed not show blueshift of incoming light, but the effect is so small for gravity wells like Earth's that I suspect the difference is undetectable.
I think the James Webb Space Tel
Re:Interesting Background... (Score:1)
Re:Interesting Background... (Score:1)
Re:Interesting Background... (Score:1)
According to that guy it seems so. Also there seems to be this notion of "tired light" floating around in various articles trying to falsify the red-shift/distance relation. These theories seems to have problems [ucla.edu] though. I don't know the weak spots in LaViolette's gravity/light model, but it sure was very interesting. Maybe there's some cosmological paradigm shift sneaking upon us. See e.g., http://www.metaresear [metaresearch.org]
An operation of public communication (Score:1, Interesting)
I still keep thinking the HST isn't really needed anymore
redshift (Score:2, Informative)
Re:redshift (Score:2)
Re:redshift (Score:2)
Re:When (Score:3, Informative)
Luminous? (Score:1)
Detectig and studying non-luminous objects like Buffy is a lot harder than luminous ones like Sirius B.
What about detecting and studying Lumines [ubi.com] itself? And, if you value Freedom, what about Luminesweeper [pineight.com]?
Sirius? (Score:3, Funny)
Re:Sirius? (Score:1)
I was wrong.
Good thing... (Score:2)
Re:Good thing... (Score:2)
Every available scope IS useful, but the Hubble has reached a point where
White Dwarf... (Score:2, Funny)
Re:White Dwarf... (Score:2)
just curious... (Score:2)
That's easy. (Score:2)
Get the paper here (Score:1, Informative)
what about.. (Score:1)
The Dogon Mystery (Score:4, Interesting)
All these things happen to be true. But what makes this so remarkable is that the companion star of Sirius, called Sirius B, was first photographed in 1970. While people began to suspect its existence around 1844, it was not seen through a telescope until 1862 -- and even then its great density was not known or understood until the early decades of the twentieth century. The Dogon beliefs, on the other hand, were supposedly thousands of years old.
http://www.dreamscape.com/morgana/thalass2.htm [dreamscape.com]
Wiki to the rescue (Score:2)
Re:The Dogon Mystery (Score:3, Informative)
Super nova remnant? (Score:2)
Is that really true?
It seems like an event like that only 8 light years away would have fried our little pitiful planet in a away that would be very noticeble today, or more likely exterminate all life.
Anyone know?
Re:Super nova remnant? (Score:2)
White dwarfs are the remnant of Sun-like stars -- they are not formed in supernova explosions. However, some white dwarfs in binary star systems can accumulate mass from their companion and explode in a nova or in some cases a Type Ia supernova.
The nearest star most likely to go supernova (and not Type Ia,
So that's where they went... (Score:2)
Re:White dwarf? (Score:2, Funny)
Or "Caucasian vertically challenged person"
Re:White dwarf? (Score:1)