Discussion Overview
The discussion revolves around the concept of whether a stellar object, such as a star, can become a black hole through relativistic mass increase as it approaches the speed of light. Participants explore the implications of the Theory of Relativity on mass, gravity, and the conditions necessary for black hole formation, including considerations of energy input and the star's lifecycle.
Discussion Character
- Exploratory
- Debate/contested
- Theoretical physics
Main Points Raised
- Some participants propose that if a star were to move at relativistic speeds, it could gain enough mass for gravity to pull it into a black hole.
- Others argue that black holes can only form from collapsed stars and not from a star accelerating to the speed of light.
- A participant suggests that if sufficient energy is applied to a star, it could theoretically lead to black hole formation, but questions remain about the mechanism of energy application.
- Some participants clarify that in its own frame of reference, a star does not gain mass and thus has no reason to collapse into a black hole.
- There is a discussion about the nature of kinetic energy and its inability to create stronger gravitational effects or cause a star to collapse into a black hole.
- Concerns are raised about the teaching of relativistic mass and its implications in modern physics, with some suggesting that the concept is outdated or misinterpreted.
Areas of Agreement / Disagreement
Participants express multiple competing views on the possibility of a star becoming a black hole through relativistic mass increase. The discussion remains unresolved, with no consensus on the mechanisms involved or the validity of the claims made.
Contextual Notes
Limitations include varying interpretations of relativistic mass, the dependence on definitions of energy application, and unresolved questions about the conditions necessary for black hole formation.