Discussion Overview
The discussion revolves around proving the equation for the duration of transit, specifically ΔT = PR*/πα, where P is the period of a planet around a star, R* is the radius of the star, and α is the orbital radius of the planet. Participants explore the derivation of this equation, addressing various steps and potential errors in earlier calculations.
Discussion Character
- Technical explanation
- Mathematical reasoning
- Debate/contested
Main Points Raised
- One participant presents the equation ΔT = PR*/πα and discusses their progress in deriving it, mentioning the relationship between orbital speed, linear velocity, and the radius of the star.
- Another participant questions the derivation of ΔT = 2R*/α, suggesting it may be incorrect and emphasizing the need to clarify what has been given and what needs to be shown.
- Some participants express confusion over the transition from v = 2R*/ΔT to ΔT = 2R*/α, with suggestions that the original notes may have been miswritten or misunderstood.
- There is a discussion about the dimensional correctness of the equations, with one participant asserting that ΔT = 2R*/α is dimensionally wrong.
- Eventually, a participant outlines a series of steps to eliminate v from the equations, leading to the conclusion that ΔT = PR*/πα, which is confirmed by another participant.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the initial steps leading to the equation. There is disagreement regarding the correctness of certain equations and the clarity of the derivation process. However, there is agreement on the final form of the equation ΔT = PR*/πα.
Contextual Notes
Participants express uncertainty about the definitions and roles of variables, particularly α, which is noted to typically represent an angle or angular acceleration rather than a distance in this context. There are also unresolved questions about the accuracy of the initial notes provided by the lecturer.