Supermassive black holes are extremely dense regions in space with a gravitational pull so strong that nothing, not even light, can escape from them. They are called "supermassive" because they can have masses millions or even billions of times greater than that of our sun.
Supermassive black holes are thought to form through the accumulation of mass over time, as smaller black holes merge and accrete matter from their surroundings. They are commonly found at the centers of galaxies, including our own Milky Way galaxy.
Supermassive black holes are characterized by their enormous mass and the intense gravitational forces they exert on nearby objects. They are often surrounded by an accretion disk of hot, glowing gas and dust, which emits powerful radiation as it spirals into the black hole.
These questions can help you gauge your understanding of supermassive black holes and prepare for further exploration of this fascinating topic.
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