The innermost stable circular orbit (often called the ISCO) is the smallest marginally stable circular orbit in which a test particle can stably orbit a massive object in general relativity. The location of the ISCO, the ISCO-radius ( r i s c o {\displaystyle r_{\mathrm {isco} }} ), depends on the angular momentum (spin) of the central object.
The ISCO plays an important role in black hole accretion disks since it marks the inner edge of the disk.
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