The fastest pulsar spins at 716Hz; its equator spins at 24% the speed of light
en.wikipedia.org
en.wikipedia.org
Fascinating - and I think humanity is "winning"
How 'bout that for the correlation=causation folks!
The historical preindustrial peak human population was around 500-800 million. Maybe we'd be lucky and be able to sustain somewhat more than that, say 2 billion. I have a hard time seeing much more given energy and resource limitations.
Prediction's hard, especially about the future, but I suspect we're looking at a crisis well within 100 years. Possibly a few decades out, if that.
Look up Limits to Growth.
If you allow rotating reference frames then you've got to talk about transformation rules in gory detail. Everyone understands centrifugal force, but what about the coriolis and euler forces? Our intuition doesn't tell us when they apply and when they don't, so we have to be systematic about it, and that means "gory details". And guess what "being systematic about it" involves? Moving to an inertial frame of reference and taking derivatives!
You can't be intuitively correct or systematic about rotating frames without thoroughly understanding inertial frames, so that's what you learn first, along with strongly worded advice to stay away from non-inertial frames (e.g. defining frame-dependent forces as "fictitious").
Anyone doing general relativity is comfortable enough with coordinate transformations that they can understand the caveats that come with frame-dependent forces and even take advantage of them to simplify calculations or definitions (the process of going from a "global" to a "local" coordinate system is highly nontrivial in GR).
That's why the Coriolis, Euler, and Centrifugal forces are called "fictitious" while gravity isn't.
Comments like this point out just how much I do not know, they sweep their arms across a horizon of maths and hard won understanding and say "only express that opinion after you know what that means"
Anti-trolling.
It's what keeps us honest about our own limitations, and reluctant to spout off crap.
love it. Now going to look up inertial frames and start translating.
Yet another reason I like the "don't change the title; the title is not for editorializing" policy on HN.
Because hn's anti editorialization policy is useless in both cases. For, in the first case, without editorialization, the title is completely useless except for experts on the subject. And for the second case, it has nothing to do with title editorialization, but with content.
EDIT:
My amateur physics say that the gravitational well adds 9.7% to that.
I tried the same calculation for earth and it gave a sensible result: a change of 6.95 * 10^-10.
Here is an answer from physics exchange which gets the same result: http://physics.stackexchange.com/questions/10089/gravitation...
Edit: I may have been reading too much into it. The effects you see will depend on which positions you're comparing, and people in this thread haven't really specified.
(Don't try this at home.) (And if you do, don't touch the walls.)
It's like you didn't read your link
Just as if you were inertially moving at 0.9c relative to me, the time frame would be different despite both me and you being 'the same as a point in empty space'.
I know that for rotating black holes the Kerr solution to the Einstein equations offers the best way to test these metric-based questions but I'm not sure if that's what you'd use for a Neutron Star.
They seem to overlook the fact that we don't know anything; compared to what is out there our knowledge might approach a millionth of a millionth percent of all knowable things; but even that is just for illustration because if you only take into account the scale of the known universe it's going to be a number so small as to approach 0. We know literally nothing.
It's fine to come up with grand theories of how things work - human imagination is a wonderful thing. Just don't mistake it for facts.
The strontium clock at Boulder loses one second in five billion years. [1][2][3]
Does anyone have any information supporting the pulsar clock claim? I have a sneaking suspicion that the author of this claim --just like the catalog in the chair pocket on airplanes--thinks my radio clock that syncs to WWVB/DCF77 is "an atomic clock."
[1] http://www.theverge.com/2014/1/22/5333324/nist-atomic-clock-...
[2] http://www.nature.com/nature/journal/vaop/ncurrent/full/natu...
[3] http://www.colorado.edu/news/releases/2014/01/22/jila-stront...
Normally though, stars or planets are caught from clouds catching and revolving around each other for a couple of million years until the condense to a solid object. Thus the spin.
In the case of our own Moon, one side is more massive than the other and over the course of millions of years became tidally locked so that the heavier side always points towards the Earth.
This minute physics video (about the shape of the solar system) explains it probably better than I can put into words myself:
http://www.youtube.com/watch?v=tmNXKqeUtJM
The relevent part starts at about 1:03, but I recommend watching the whole thing.
In the classical approximation (1/2 Iω^2), assuming a uniform sphere of 2.0 solar masses and r=16 km.
That's about 3% of the mass-energy (mc^2 = 3e47 J).
This could be way off.
[1] - http://www.wolframalpha.com/input/?i=mass-energy+of+two+sola...
edit: Back-of-the-envelope says it's a very bad idea, which is just barely plausible if your asteroid is extremely large, and has an extremely high tensile strength (maybe iron-nickel?). Oh well.
edit2: Also apparently there's a failure mode where if you do overestimate the strength of the asteroid's interior, it tears apart and (from e.g geosynchronous orbit) has a >5% chance of destroying most of the planet. D: Yeah, where I said "no mechanical safety hazards", I retract that.
(this would need to have a reference in the main star, otherwise it would just spin with the planet)
Nope. You could launch generator pods in a hyperbolic trajectory that would start out escaping the neutron star, but generate electricity from the rotating magnetic field in such a way that it's captured in orbit and comes back to its launch point.