Innermost Stable Circular Orbit

The Innermost Stable Circular Orbit (often called the ISCO) is the smallest orbit in which a test particle can stably orbit a massive object in general relativity.[1] The location of the ISCO, the ISCO-radius (r_{isco}), depends on the angular momentum (spin) of the central object. For a non-spinning object, a where the gravitational field can be expressed with the Schwarzschild metric, the ISCO is located at,

r_{isco} = \frac{6 \, GM}{c^2}.

As the angular momentum of the central object increases, r_{isco} decreases. Even for a non-spinning object, the ISCO radius is only three times the Schwarzschild Radius, suggesting that only black holes have innermost stable circular orbits outside of their surfaces.

References

External links

This article is issued from Wikipedia - version of the Sunday, January 24, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.