Star 4 ly Earth Sun Diameter of orbit Figure 34.26 Distances to nearby stars are measured using triangulation, also called the parallax method. The angle of line of sight to the star is measured at intervals six months apart, and the distance is calculated by using the known
Star 4 ly Earth Sun Diameter of orbit Figure 34.26 Distances to nearby stars are measured using triangulation, also called the parallax method. The angle of line of sight to the star is measured at intervals six months apart, and the distance is calculated by using the known
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Distances to the nearest stars (up to 500 ly away) can be measured by a technique called parallax, as shown in Figure 34.26. What are the angles θ and θ relative to the plane of the Earth’s orbit for a star 4.0 ly directly
above the Sun?
![Star
4 ly
Earth
Sun
Diameter of orbit
Figure 34.26 Distances to nearby stars are measured using
triangulation, also called the parallax method. The angle of
line of sight to the star is measured at intervals six months
apart, and the distance is calculated by using the known](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F2b4dfa94-c589-4cb9-9d6a-c32b423816c8%2F8d76ad17-540c-4263-856a-410941be60b1%2Frjprbza_processed.png&w=3840&q=75)
Transcribed Image Text:Star
4 ly
Earth
Sun
Diameter of orbit
Figure 34.26 Distances to nearby stars are measured using
triangulation, also called the parallax method. The angle of
line of sight to the star is measured at intervals six months
apart, and the distance is calculated by using the known
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