1. Stellar black holes: Formed from the collapse of massive stars, with a mass ranging from a few times that of the Sun to around 20 times the mass of the Sun.
2. Intermediate-mass black holes: With a mass between that of stellar black holes and supermassive black holes, ranging from hundreds to thousands of times the mass of the Sun.
3. Supermassive black holes: Found at the centers of galaxies, with a mass ranging from millions to billions of times the mass of the Sun.
4. Primordial black holes: Hypothetical black holes that could have formed in the early universe, with a mass much smaller than stellar black holes.
5. Micro black holes: Theoretical black holes with a mass much smaller than stellar black holes, possibly formed in high-energy particle collisions.
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Google Gemini AI
Jul 3
- Stellar black holes: These are the most common type of black hole, and they are formed when a massive star collapses at the end of its life. Stellar black holes can have masses ranging from a few solar masses to several dozen solar masses. - Supermassive black holes: These are the largest type of black hole, and they are found at the centers of most galaxies. Supermassive black holes can have masses ranging from millions to billions of solar masses. - Intermediate-mass black holes: These are black holes that have masses between stellar black holes and supermassive black holes. Intermediate-mass black holes are thought to be formed by the merger of smaller black holes. - Primordial black holes: These are black holes that are thought to have formed in the early universe. Primordial black holes could have masses ranging from a fraction of a solar mass to several solar masses. - Quantum black holes: These are hypothetical black holes that are thought to have extremely small masses, perhaps only a few Planck masses. Quantum black holes could be formed by the collapse of matter in the early universe.