Widdekind Posted June 16, 2013 Share Posted June 16, 2013 Gravitational Potential Energy (GPE) ~ GM2/R equivalent rest-mass energy = mc2 GM2/R = mc2 m/M ~ RS/R (actually, 1/5 x RS/R) So, order-of-magnitude, the rest-mass equivalent, of some self-gravitating body, is a similar fraction of the total actual mass, as that body's Schwarzschild radius is, to its actual physical radius. Link to comment Share on other sites More sharing options...
xyzt Posted June 16, 2013 Share Posted June 16, 2013 (edited) Gravitational Potential Energy (GPE) ~ GM2/R equivalent rest-mass energy = mc2 GM2/R = mc2 m/M ~ RS/R (actually, 1/5 x RS/R) So, order-of-magnitude, the rest-mass equivalent, of some self-gravitating body, is a similar fraction of the total actual mass, as that body's Schwarzschild radius is, to its actual physical radius. I assume that in the above "M" is the gravitational mass while "m" is the inertial mass. If so, your conjecture is many orders of magnitude off since it is well known (google "Eotvos experiment", "Einstein equivalence principle") that the two are equal to a very high order of precision. Edited June 16, 2013 by xyzt Link to comment Share on other sites More sharing options...
Widdekind Posted July 3, 2013 Author Share Posted July 3, 2013 no -- the amount of anti-matter required to obliterate a gravity-bound ball-shaped world/planet Link to comment Share on other sites More sharing options...
xyzt Posted July 3, 2013 Share Posted July 3, 2013 (edited) no -- the amount of anti-matter required to obliterate a gravity-bound ball-shaped world/planet In this case you would have indeed: [math]m=M \frac{r_s}{R}[/math] For example, for Earth, the ratio [math]\frac{r_s}{R}=\frac{10^{-2}}{6.4*10^6} =\frac{1}{6.4*10^8}[/math] Thus, [math]m=10^{16} kg[/math] Edited July 3, 2013 by xyzt Link to comment Share on other sites More sharing options...
Widdekind Posted July 4, 2013 Author Share Posted July 4, 2013 very vaguely, about a billionth of an earth-mass of AM => "Aldebaran" such seemed readily rememberable, "mass ratio (AM:M) ~ radius ratio (RS:R)", and seemingly works well(-est) for "classical" or "sub-relativistic" ball-shaped bodies In this case you would have indeed: [math]m=M \frac{r_s}{R}[/math] For example, for Earth, the ratio [math]\frac{r_s}{R}=\frac{10^{-2}}{6.4*10^6} =\frac{1}{6.4*10^8}[/math] Thus, [math]m=10^{16} kg[/math] Link to comment Share on other sites More sharing options...
Recommended Posts
Create an account or sign in to comment
You need to be a member in order to leave a comment
Create an account
Sign up for a new account in our community. It's easy!
Register a new accountSign in
Already have an account? Sign in here.
Sign In Now