Discussion Overview
The discussion revolves around the time it takes for a giant molecular cloud to undergo gravitational collapse, exploring the factors influencing this process, including density and the relationship between potential and kinetic energy. Participants examine the implications of free-fall time and the conditions necessary for particles to achieve high velocities during collapse.
Discussion Character
- Debate/contested
- Technical explanation
- Mathematical reasoning
Main Points Raised
- One participant questions how long gravitational collapse takes, suggesting that the weak nature of gravity implies a long acceleration time for particles.
- Another participant presents the free-fall time equation, $$t_{ff}=\sqrt{\frac{3\pi}{32G\rho}}$$, emphasizing its dependence on density and clarifying that particles in cold molecular clouds are not charged and do not achieve high accelerator-range velocities.
- A later reply suggests that using the density of hydrogen for calculations may indicate a collapse time of thousands of years, linking this to the high temperatures necessary for nuclear fusion.
- Some participants argue that while potential energy converts to kinetic energy, a long free-fall time does not necessarily equate to high speeds, using the example of falling to Earth from a distance to illustrate this point.
- Others contend that high temperatures in star formation should correlate with high speeds, challenging the idea that long free-fall times do not imply high velocities.
- There is a discussion about the relationship between free-fall time, density, and the velocities of particles, with some asserting that denser clouds collapse faster and lead to higher velocities.
- Participants express confusion over the implications of free-fall time and potential energy, with some reiterating that high temperatures indicate high speeds, while others argue against this assumption.
- One participant clarifies that the condition for high velocities is related to the potential energy of the particle rather than the duration of the gravitational force acting on it.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between free-fall time, density, and particle velocities. There is no consensus on whether long free-fall times necessarily lead to high speeds, and the discussion remains unresolved regarding the implications of potential energy conversion in the context of gravitational collapse.
Contextual Notes
Participants note that the density of the cloud plays a critical role in determining collapse time and particle velocities, but the discussion does not resolve how these factors interact in specific scenarios.