Discussion Overview
The discussion centers around the translational motion of black holes, exploring whether they can exhibit such motion in addition to their known spin or rotational components. Participants delve into the implications of black holes' motion relative to galaxies and other cosmic structures, as well as the nature of black holes themselves.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
Main Points Raised
- Some participants propose that black holes may have translational motion, but this is dependent on the frame of reference considered.
- One participant theorizes that a star losing its translational motion is more likely to become a nova or supernova before forming a black hole.
- Another participant notes that while black holes are theorized to have spin, not all black holes necessarily possess this property.
- There is a discussion about the stability of galaxies versus stars, with some arguing that galaxies are stable against gravitational collapse while stars are not.
- Questions are raised regarding quasars and whether they can be considered exploding galaxies, with a participant admitting limited knowledge on the topic.
- One participant explains that while black holes generally retain angular momentum from their progenitor stars, it is theoretically possible to describe a black hole without spin.
- The "black holes have no hair" theorem is mentioned, which states that black holes are characterized by their mass, angular momentum, and charge.
Areas of Agreement / Disagreement
Participants express differing views on the existence of translational motion in black holes and the implications of their spin. There is no consensus on whether all black holes have spin or the nature of quasars, indicating multiple competing views remain.
Contextual Notes
Some claims depend on definitions and assumptions about black holes and their properties, and there are unresolved questions regarding the nature of quasars and the stability of galaxies versus stars.