‘Black hole’ is a
star which has collapsed into itself and has large acceleration due to gravity on its surface
A ‘black hole’ is one of the most fascinating objects in space. It is not an empty space, but rather a region where gravity is so strong that nothing, including light and other electromagnetic waves, has enough energy to escape its pull.
Black holes typically form from the collapse of a massive star at the end of its life cycle. When a very massive star runs out of nuclear fuel, its core collapses under its own gravity. This collapse can lead to a supernova explosion, leaving behind a dense remnant.
If the remnant's mass is above a certain limit (the Tolman-Oppenheimer-Volkoff limit for neutron stars, and potentially higher for black holes), the collapse continues infinitely, crushing all the matter into an infinitely dense point called a singularity. This creates the black hole.
Key characteristics include:
Let's look at the given options based on our understanding:
This is incorrect. While black holes are related to stars, they are not typical "stars". More importantly, they have extremely large acceleration due to gravity, not zero.
This is incorrect. Black holes have immensely strong gravity, far exceeding a "moderate" level.
This aligns with the formation process (collapsed star) and the key characteristic of intense gravity (large acceleration due to gravity).
This is incorrect. A collapsed star that forms a black hole has very large, not zero, acceleration due to gravity.
Based on the characteristics of black holes formed from collapsed stars, the description that fits best is a collapsed star with a large acceleration due to gravity on its surface (near the event horizon). The term "surface" in this context usually refers to the event horizon, the effective boundary.
Therefore, a ‘black hole’ is understood as a region formed from the collapse of a star, characterized by an extremely strong gravitational field leading to very large acceleration due to gravity.
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