Discussion Overview
The discussion revolves around determining the recession speed of a galaxy based on the wavelengths of two stars, utilizing concepts such as Doppler shift and redshift. Participants explore the implications of star measurements for estimating the galaxy's recession speed and distance.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- One participant calculates the speeds of two stars using Doppler shift, yielding values of 4011 km/s and 4999 km/s.
- Another participant suggests that the recession speed of the galaxy will be close to the speeds of the stars but requires more measurements for accuracy.
- A participant notes that the spatial arrangement of the stars within the galaxy could affect the estimation of the recession speed, advocating for the use of mean speeds if the stars are positioned on opposite sides.
- One participant proposes calculating redshift and multiplying by the speed of light to estimate recession speed, arriving at a value of around 900 km/s.
- Another participant questions the discrepancy between the 900 km/s estimate and the previously calculated star speeds, suggesting averaging the redshifts instead.
- A later reply indicates that using the mean speed of the stars, given their positions, would yield a recession speed of 4505 km/s and a distance of 60.1 Mpc.
- Participants express curiosity about the published distance of the galaxy and whether the calculated distance aligns with existing data.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the best method to determine the galaxy's recession speed, with multiple approaches and estimates presented. The discussion remains unresolved regarding the most accurate calculation method and the implications of the star positions.
Contextual Notes
Participants acknowledge the need for additional information about the galaxy's structure and the positions of the stars to refine their estimates. There are also unresolved questions regarding the accuracy of the redshift calculations and the relationship between the different speed estimates.