To approximate the distance from the Earth to stars relatively close by, astronomers often use the method of parallax. Parallax is the apparent displacement of an object caused by a change in the observer's point of view. As the Earth orbits the Sun, a nearby star will appear to move against the more distant background stars. Astronomers measure a star's position at times exactlv 6 months apart when the Earth is at opposite points in its orbit around the Sun. The Sun, Earth, and star form the vertices of a right triangle with LPSE=90°. The length of side SE is the distance between the Earth and Sun, approximately 92,900,000 mi. The parallax angle (or simply parallax) is denoted by p. Earth Sun Star Exampl P Parallax angle Background stars Earth Part: 0/ 2 Part 1 of 2 (a) Find the distance between the Earth and Ruchbah if the parallax angle is 0.033" (arcseconds). Round your answer to the nearest hundred billion miles. mi . The distance between the Earth and Ruchbah is approximately

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Chapter9: The Famliy Of Stars
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To approximate the distance from the Earth to stars relatively close by, astronomers often use the method of parallax. Parallax is the apparent displacement of
an object caused by a change in the observer's point of view. As the Earth orbits the Sun, a nearby star will appear to move against the more distant
background stars. Astronomers measure a star's position at times exactly 6 months apart when the Earth is at opposite points in its orbit around the Sun. The
Sun, Earth, and star form the vertices of a right triangle with LPSE=90°. The length of side SE is the distance between the Earth and Sun, approximately
92,900,000 mi. The parallax angle (or simply parallax) is denoted by p.
Earth
Star
Example
Sun
P
Parallax angle
E
Earth
Background stars
Part: 0/ 2
Part 1 of 2
(a) Find the distance between the Earth and Ruchbah if the parallax angle is 0.033" (arcseconds). Round your answer to the nearest hundred billion miles.
mi .
The distance between the Earth and Ruchbah is approximately
x10
Transcribed Image Text:Est To approximate the distance from the Earth to stars relatively close by, astronomers often use the method of parallax. Parallax is the apparent displacement of an object caused by a change in the observer's point of view. As the Earth orbits the Sun, a nearby star will appear to move against the more distant background stars. Astronomers measure a star's position at times exactly 6 months apart when the Earth is at opposite points in its orbit around the Sun. The Sun, Earth, and star form the vertices of a right triangle with LPSE=90°. The length of side SE is the distance between the Earth and Sun, approximately 92,900,000 mi. The parallax angle (or simply parallax) is denoted by p. Earth Star Example Sun P Parallax angle E Earth Background stars Part: 0/ 2 Part 1 of 2 (a) Find the distance between the Earth and Ruchbah if the parallax angle is 0.033" (arcseconds). Round your answer to the nearest hundred billion miles. mi . The distance between the Earth and Ruchbah is approximately x10
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