by neufer » Sun Mar 14, 2010 7:02 pm
Chris Peterson wrote:biddie67 wrote:The sense of what could be the possible ripple effect on our little world if those two black holes collide and explode, black hole style, is fearsome to speculate.
I wouldn't worry. Gravity waves are not destructive. Black holes like these have collided many times in the history of the Universe, without effect outside their immediate environs. It is only now that we have the technology to possibly detect the waves created by such collisions- nothing but the most exquisitely sensitive instruments can do so.
http://en.wikipedia.org/wiki/Ligo wrote:
<<Based on current models of astronomical events, and the predictions of the general theory of relativity, gravitational waves that originate tens of millions of light years from Earth are expected to distort the
Laser
Interferometer
Gravitational-Wave
Observatory (
LIGO) 4 kilometer mirror spacing by about 10
−18 m, less than one-thousandth the "diameter" of a proton. Equivalently, this is a relative change in distance of approximately one part in 10
21. A typical event which might cause a detection event would be the late stage inspiral and merger of two 10 solar mass black holes, not necessarily located in the Milky Way galaxy, which is expected to result in a very specific sequence of signals often summarized by the slogan chirp, burst, quasi-normal mode ringing, exponential decay.
As of November 2005, sensitivity had reached the primary design specification of a detectable strain of one part in 10
21 over a 100 Hz bandwidth. The baseline inspiral of two roughly solar-mass neutron stars is typically expected to be observable if it occurs within about 8,000,000 parsecs (26,000,000 ly), or the vicinity of our Local Group of galaxies, averaged over all directions and polarizations.
In 2004, it was reported that theorists were estimating the chances of unambiguous direct detection by 2010 at one in six.
In February 2007, GRB 070201, a short gamma-ray burst, arrived at Earth from the direction of the Andromeda Galaxy, a nearby galaxy. The prevailing explanation of most short gamma-ray bursts is the merger of a neutron star with either a neutron star or black hole. LIGO reported a non-detection for GRB 070201, ruling out a merger at the distance of Andromeda with high confidence. Such a constraint is predicated on LIGO eventually demonstrating a direct detection of gravitational waves.>>
[quote="Chris Peterson"][quote="biddie67"]The sense of what could be the possible ripple effect on our little world if those two black holes collide and explode, black hole style, is fearsome to speculate.[/quote]
I wouldn't worry. Gravity waves are not destructive. Black holes like these have collided many times in the history of the Universe, without effect outside their immediate environs. It is only now that we have the technology to possibly detect the waves created by such collisions- nothing but the most exquisitely sensitive instruments can do so.[/quote]
[quote=" http://en.wikipedia.org/wiki/Ligo"]
<<Based on current models of astronomical events, and the predictions of the general theory of relativity, gravitational waves that originate tens of millions of light years from Earth are expected to distort the [b]L[/b]aser [b]I[/b]nterferometer [b]G[/b]ravitational-Wave [b]O[/b]bservatory ([url=http://antwrp.gsfc.nasa.gov/apod/ap001030.html][b]LIGO[/b][/url]) 4 kilometer mirror spacing by about 10[sup]−18[/sup] m, less than one-thousandth the "diameter" of a proton. Equivalently, this is a relative change in distance of approximately one part in 10[sup]21[/sup]. A typical event which might cause a detection event would be the late stage inspiral and merger of two 10 solar mass black holes, not necessarily located in the Milky Way galaxy, which is expected to result in a very specific sequence of signals often summarized by the slogan chirp, burst, quasi-normal mode ringing, exponential decay.
As of November 2005, sensitivity had reached the primary design specification of a detectable strain of one part in 10[sup]21[/sup] over a 100 Hz bandwidth. The baseline inspiral of two roughly solar-mass neutron stars is typically expected to be observable if it occurs within about 8,000,000 parsecs (26,000,000 ly), or the vicinity of our Local Group of galaxies, averaged over all directions and polarizations. [b]In 2004, it was reported that theorists were estimating the chances of unambiguous direct detection by 2010 at one in six.[/b]
In February 2007, GRB 070201, a short gamma-ray burst, arrived at Earth from the direction of the Andromeda Galaxy, a nearby galaxy. The prevailing explanation of most short gamma-ray bursts is the merger of a neutron star with either a neutron star or black hole. LIGO reported a non-detection for GRB 070201, ruling out a merger at the distance of Andromeda with high confidence. Such a constraint is predicated on LIGO eventually demonstrating a direct detection of gravitational waves.>>[/quote]