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the claim

Stable orbits exist around black holes

the verdict
SUPPORTED
the evidence backs this
Recorded sources
8 sources for · 0 against

Counts group repeated records of the same source within each side. They do not measure evidence strength or source independence.

Extensive theoretical and astrophysical research confirms the existence of stable circular orbits, including innermost stable circular orbits (ISCOs), around various types of black holes.

The analysis

The retrieved literature extensively discusses and calculates stable circular orbits (such as ISCOs) around various black hole models (Kerr, Einstein-Gauss-Bonnet, Hayward, etc.). The evidence robustly supports the claim that stable orbits exist around black holes.

Evidence for · 8
Innermost stable circular orbit and shadow of the 4D Einstein–Gauss–Bonnet black hole
Recorded source metadata

Minyong Guo, Peng-Cheng Li. Innermost stable circular orbit and shadow of the 4D Einstein–Gauss–Bonnet black hole. 2020. https://doi.org/10.1140/epjc/s10052-020-8164-7

Paper [0] analyzes innermost stable circular orbits in the spacetime of 4D Einstein-Gauss-Bonnet black holes.

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More for · 7
Circular orbits and collisions of particles with magnetic dipole moment near magnetized Kerr black holes in modified gravity
Recorded source metadata

Saeed Ullah Khan, Uktamjon Uktamov, J. Rayimbaev, A. Abdujabbarov, Inomjon Ibragimov, Zhi-Min Chen. Circular orbits and collisions of particles with magnetic dipole moment near magnetized Kerr black holes in modified gravity. 2024. https://doi.org/10.1140/epjc/s10052-024-12567-2

Paper [1] investigates circular orbits and innermost stable circular orbits of magnetized particles near Kerr black holes.

Circular orbits and polarized images of charged particles orbiting a Kerr black hole with a weak magnetic field
Recorded source metadata

Tsai-Chen Lee, Zezhou Hu, Minyong Guo, Bin Chen. Circular orbits and polarized images of charged particles orbiting a Kerr black hole with a weak magnetic field. 2022. https://doi.org/10.1103/PhysRevD.108.024008

Paper [2] examines circular motions and innermost stable circular orbits of charged particles around a Kerr black hole.

Energy extraction from the accelerating Kerr black hole via magnetic reconnection in the plunging region and circular orbit region
Recorded source metadata

Ke Wang, Xiao-Xiong Zeng. Energy extraction from the accelerating Kerr black hole via magnetic reconnection in the plunging region and circular orbit region. 2025. https://doi.org/10.1088/1475-7516/2025/11/026

Paper [3] discusses circular orbits and innermost stable circular orbits in the context of accelerating Kerr black holes.

Innermost stable circular orbit of Kerr-Bertotti-Robinson black holes and inspirals from it: Exact solutions
Recorded source metadata

Towe Wang. Innermost stable circular orbit of Kerr-Bertotti-Robinson black holes and inspirals from it: Exact solutions. 2025

Paper [4] derives exact solutions for innermost stable circular orbits around Kerr-Bertotti-Robinson black holes.

Circular motion and the innermost stable circular orbit for spinning particles around a charged Hayward black hole background
Recorded source metadata

Eduard Larrañaga. Circular motion and the innermost stable circular orbit for spinning particles around a charged Hayward black hole background. 2020. https://doi.org/10.1142/s0218271820501217

Paper [5] investigates circular motion and innermost stable circular orbits for spinning particles around a charged Hayward black hole.

Tilted circular orbits around a Kerr black hole
Recorded source metadata

A. Al Zahrani. Tilted circular orbits around a Kerr black hole. 2023. https://doi.org/10.1103/PhysRevD.109.024029

Paper [7] explores tilted circular orbits and innermost stable circular orbits around a Kerr black hole.

Quasinormal ringing of Kerr black holes. III. Excitation coefficients for equatorial inspirals from the innermost stable circular orbit
Recorded source metadata

Matteo Della Rocca, Laura Pezzella, E. Berti, L. Gualtieri, A. Maselli. Quasinormal ringing of Kerr black holes. III. Excitation coefficients for equatorial inspirals from the innermost stable circular orbit. 2025

Paper [8] studies point particles plunging from the innermost stable circular orbit of a Kerr black hole.

The paper trail · every fact has a biography
first checked01 Aug 2026
judged → SUPPORTED · 9001 Aug 2026
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