How Did Scientists Calculate the Orbital Radius of Jupiter's Moons?

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    Moon Orbital Radius
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SUMMARY

The calculation of the orbital radius of Jupiter's moons involves using the formula D = θ d / 206,265, where D represents the linear size of the moon's orbit, θ is the angular size in arcseconds, and d is the distance to Jupiter. Observations can be made using telescopes, particularly during opposition, to measure the angular distance of the moons. Historical context includes Römer's 1676 measurement of the speed of light, which, despite being inaccurate, provided a basis for estimating distances in the solar system. The discussion emphasizes the importance of repeated measurements over multiple orbits for accurate calculations.

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  • Understanding of angular measurements in astronomy
  • Familiarity with the concept of opposition in celestial observations
  • Knowledge of basic astronomical formulas, specifically D = θ d / 206,265
  • Awareness of historical methods for measuring astronomical distances
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  • Research the methods used by Römer for measuring the speed of light
  • Explore the concept of celestial opposition and its significance in astronomy
  • Learn about modern techniques for measuring distances in the solar system
  • Investigate the historical context of Galilei's and Römer's astronomical findings
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Astronomers, physics students, and anyone interested in the historical and practical methods of calculating celestial distances and orbital mechanics.

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TL;DR
How did the first scientists figure out the orbital radius of a moon of Jupiter? How can observations lead to a calculation of the orbital radius of a moon of another planet?
How did the first scientists figure out the orbital radius of a moon of Jupiter? How can observations lead to a calculation of the orbital radius of a moon of another planet?
 
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Thank you.

So would you find the orbital radius of a Jovian moon by using a telescope to view Jupiter at opposition during a time when the moon is farthest from Jupiter? Then you could find the arcseconds of angle from the center of Jupiter to the center of the moon? Then you could use the equation D = θ d / 206,265? Then D would be the orbital radius of the moon?
 
Yeah, although:
1. it doesn't really have to be at opposition
2. you'd need to measure the angular distance of the moon over several/many orbits to get a good estimate of the maximum orbital radius.
 
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How did the scientists figure out distance to Jupiter back in 17th century? Römer measured speed of light by 1676, but he got the speed about 30% too slow. How much of it was the error in travel time, how much the error in distance to Jupiter?
How much was Römer´s distance in 1676 better than Galilei´s distance, if any, in 1610?
 

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