Birth of Black Hole Possibly Being Observed 32
TheTXLibra writes "Robert Roy Britt reports on
Space.com that we may now be witnessing the earliest stages of black hole development. Star SN 1986J, began to collapse in 1983 into a neutron star, resulting in a supernova explosion in 1986. If the mass of the neutron star reaches 1.4 times the mass of Earth's Sun, it will theoretically collapse into a black hole, if not, it will stabilize as a neutron star."
Not quite accurate. (Score:5, Informative)
Re:Not quite accurate. (Score:5, Informative)
Re:Not quite accurate. (Score:2, Funny)
Re:Not quite accurate. (Score:5, Informative)
Holes? (Score:1, Interesting)
Re:Holes? (Score:5, Informative)
Re:Holes? (Score:5, Informative)
Fine. _I'll_ reply.
Gravastars are an interesting idea, but they:
a) Propose modifications to physics (the phase transition that gives rise to a different type of space in the interior).
and
b) Attempt to solve a problem that doesn't necessarily exist (embodiment of entropy in black holes, which string theory takes a fairly good stab at explaining).
Thus, I'm skeptical of claims that gravastars exist, barring observations supporting their existance or wider acceptance by the scientific community.
At least in the paper [arxiv.org] I've managed to dig up so far, they acknowledge many othe potential models of how black holes work, and suggest types of observations that would help determine whether their model is accurate (i.e., they don't claim it's the One True Model off the bat). This is one of the hallmarks of good science.
Observations to look for are gravity-wave signatures of resonance modes in the stiff shell surrounding the gravastar, and optical signatures of impacting matter interacting with this shell. The first should be possible when we get sufficiently sensitive gravity wave detectors online, and the second should be possible from observations of accretion disks in known black hole/other star binary pairs once Mazur and Mottola have worked through the math to figure out what the observational signatures should _be_. Thirdly, if you could get close enough to take good measurements, you'd be able to distinguish between gravastar-type black holes and Hawking-Bekenstein black holes by different radiation signatures coming off of them, but that requires being right next to the hole and having instruments sensitive enough to detect very faint, low-frequency thermal radiation.
In summary, claiming that the gravastar model _is_ what black holes are is very, very premature.
Interesting and monumental! (Score:4, Interesting)
The collapse into a black hole in such a short time (also in the article) is somewhat expected, because the gravity will be so strong. This should be a pretty neat and real way to verify if our view on black hole formation and the associated astro-physics that accompany it are mostly correct.
Re:Interesting and monumental! (Score:2, Interesting)
Still, very awesome. It
Knowing where to look... (Score:5, Insightful)
(I guess you could also theoretically look for black holes by their gravitational lensing effects, but you would have to monitor a huge number of stars and hope that a black hole intercepts your line-of-sight to one of them, so not very practical.)
Probabilistic fallacy in article (Score:1, Informative)
Just because you don't know whether or not an event occurs doesn't mean that it stands a "roughly equal" chance of occurring and not occurring
The Nature of Probability (Score:2, Insightful)
For example, let's say someone flips a coin and you call the result in mid-air. In reality, the result of the coin toss is already determined at this point. However, as far as you're concerned the probability of either result is 50%. Or even better, let's say that you're trying to guess which of two cups holds a ball. The person who placed the ball knows with complete certainty which cup holds it, but as far as you're conce
Re:The Nature of Probability (Score:1)
Re:The Nature of Probability (Score:2, Insightful)
I think he was trying to say that for "roughly equal" to apply, we must presume to know that P(black hole) ~= P(neutron star). Maybe we do know that, perhaps because that's generally the case (due to distribution of stars of different masses), or because we know something special about this particular case.
But if not, then the quote in the article is falling into the "either it'll happen or it won't"
Re:The Nature of Probability (Score:1, Interesting)
Re:Probabilistic fallacy in article (Score:2)
*Then* it would be a "roughly equal" chance of it being a black hole.
Re:Probabilistic fallacy in article (Score:2, Informative)
How long until they know? (Score:3, Insightful)
What I didn't see was any indication when they'll be able to determine whether the star is going to remain a stable neutron star or become a black hole. Does anybody with actual knowledge in the subject care to comment?
Re:How long until they know? (Score:2, Informative)
The stellar furnace operates in several distinct stages where each stage fuses a particular element and the byproduct is the element used in the next stage. The first is hydrogen, the second is helium. The third is the Cargon - Nitrogen - Oxygen cycle (I think this is the third stage). The CNO cycle produces Silicon. This is where things get interesting
Re:How long until they know? (Score:1)
Re:How long until they know? (Score:2)
1.4 solar masses is the limit for a core supported by electron degeneracy - a white dwarf. Stellar remnants exceeding this mass will collapse to form a neutron star.
The maximum mass of neutron stars is less well known; the properties of neutronium cannot easily be tested in the laboratory! The absolute maximum, assuming that neutronium i