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Scientists Spot Rare 'In Between' Black Hole
An anonymous reader writes "Scientists have found a doomed star orbiting what appears to be a medium-sized black hole. This black hole appears to be a theorized 'in-between' category of black hole that has eluded confirmation and frustrated scientists for more than a decade."
...gray hole?
Authority questions you. Return the favor.
It's a trap!
[Fuck Beta]
o0t!
No. I think "in between" is where the switch is stuck in the middle (i.e., "subl" or "she's gonna blow"). Either way, something bad is gonna happen.
If stars had been given categories like 'Doomed', i think i'd have paid more attention in my astronomy course. What Would Chandrasekar Do?
-AlexC
I think it's somewhere near Uranus.
I heard that there used to be plenty of those in the .cx domain.
... Breakfast and lunch ?
Hmm, maybe they did spot it inbetween breakfast and lunch, the statistics of that happening are high.
A slashdotting - you get the stick first and then the carrot !
I may be very high ... but I think poster has a point .. please mod up ...
www.gaian-mind.org - eco-punk/crust coop and collective | www.anarchistfederation.org - so cal anarchist federation
Experts say we're better off without those extra 5-7 words of information.
Who are you to argue with the experts?
Think of someone with average intelligence. Now think 1/2 the world is dumber than that guy.
There are three ways in which elements heavier than iron are produced. In two (s and r process), the basic process is to add neutrons one at a time to a nucleus. In the p process, protons are added one at a time.
What you describe is the r (rapid) process. A very high neutron flux adds neutrons very quickly. Once the neutron pulse has passed, the highly-neutron-rich nuclei beta-decay (neturon turns to proton) multiple times until a stable element is reached.
The s (slow) process has a low neutron flux, so that there is sufficient time after each neutron is absorbed for beta decay to occur. The neutrons come from a comparatively neutron-rich nucleus left over from the CNO cycle for burning hydrogen (N15?) At sufficient temperature/pressure, it starts to lose its excess neutron. The new heavy nuclei can then convect to the surface of the star and escape in the stellar wind. The detection of technetium (which has no stable isotope) in the spectra of these stars is the smoking gun proving this scenario.
I don't know much about the p process.
The r and p processes occur in supernovae. The s process occurs in red giant stars (strictly, asymptotic giant branch stars.) In terms of importance in creating heavy elements on the earth, s process is most important, followed by r process and then p process. From memory, it is something like 90% s proccess, 9% r process, 1% p process, but that is *very* rough.
Now we need a q process, so we can p, q, r and s processes. (Or S, P, Q, R if you're a Romanophile.)
Quattuor res in hoc mundo sanctae sunt: libri, liberi, libertas et liberalitas.
> What scientists spotted it?
From TFA, "A team led by Prof. Philip Kaaret of the University of Iowa, Iowa City, announced these results today in Science Express."
> What scientists were frustrated?
Although TFA doesn't specify, I think they're talking about "scientists" in general. Much as your comment talks about "stories"... in general, I presume.
You know, reading TFA wouldn't break the bank and it would really make your comment feel less lazy.
-David