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What is the magnitude of the orbital angular momentum L of Earth about the Sun? Use data from the astropendix to answer this question. L = kg m² s-1 Earth

What is the magnitude of the orbital angular momentum L of Earth about the Sun? Use data from the astropendix to answer this question. L = kg m² s-1 Earth

College Physics
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
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**Question:** What is the magnitude of the orbital angular momentum \( L \) of Earth about the Sun? Use data from the astroappendix to answer this question. \( L = \) [________] kg m\(^2\) s\(^{-1}\) **Image Description:** On the right side, there is an image of Earth as seen from space, showcasing cloud patterns, oceans, and landmasses. The image is labeled "Earth." **Explanation:** To find the magnitude of Earth’s orbital angular momentum about the Sun, you would use relevant astrophysical data, typically found in an appendix or database. The quantity is calculated using the formula: \[ L = mvr \] where \( m \) is the mass of Earth, \( v \) is the orbital velocity, and \( r \) is the average distance from the Sun. The answer should be inserted into the provided blank space with the correct unit: kg m\(^2\) s\(^{-1}\).
Transcribed Image Text:**Question:** What is the magnitude of the orbital angular momentum \( L \) of Earth about the Sun? Use data from the astroappendix to answer this question. \( L = \) [________] kg m\(^2\) s\(^{-1}\) **Image Description:** On the right side, there is an image of Earth as seen from space, showcasing cloud patterns, oceans, and landmasses. The image is labeled "Earth." **Explanation:** To find the magnitude of Earth’s orbital angular momentum about the Sun, you would use relevant astrophysical data, typically found in an appendix or database. The quantity is calculated using the formula: \[ L = mvr \] where \( m \) is the mass of Earth, \( v \) is the orbital velocity, and \( r \) is the average distance from the Sun. The answer should be inserted into the provided blank space with the correct unit: kg m\(^2\) s\(^{-1}\).
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