Intermediate Black Holes

Intermediate black holes are a hypothetical class of black holes that are larger than stellar black holes but smaller than supermassive black holes.

Characteristics of Intermediate Black Holes

• Mass: Intermediate black holes have masses ranging from 100 to 100,000 times the mass of the sun.
• Formation: They are thought to form through the merging of stellar black holes or through the direct collapse of massive gas clouds.
• Observation: Intermediate black holes have not been directly observed yet, but their existence is inferred from indirect evidence such as the observation of star clusters and galactic nuclei.

Study Guide

Here are some key points to study about intermediate black holes:

1. Formation mechanisms of intermediate black holes
2. Methods for detecting and studying intermediate black holes
3. Theoretical implications of the existence of intermediate black holes
4. Possible role of intermediate black holes in the evolution of galaxies

Be sure to understand the differences between intermediate black holes, stellar black holes, and supermassive black holes, and how they contribute to our understanding of the universe.