Planet A 2.01 AU AU Semi-major Axis R 2.01 Eccentricity Mass Distance from star ww R 0.00002 6 x 1024 kg 250,000,000 km or 2.5 x 108 km Planet B 4.01 AUR 0.5 2 x 1025 kg 590,000,000 km or 5.9 x 108 km Calculate how long it takes each planet to orbit its star, given the formula T² = R³/(Where T is the orbit time (period), and R is semimajor axis) Explain why the values are different for each planet. (show work) 3 Planet B: Planet A: 2014-8.12 2/5 4₁015 =64,49 64.49² = 4158.97 64.49 = T² 64.49²=4,01 3 8.12²= 65.93 8₁12²2² = 2₁01 A4²³ T=? 8.12=T² Explain: The values are different for both of the planets because they have differe R values. With smaller R value, the Agreater force of gravity. tamamil de Atomim

Planet A 2.01 AU AU Semi-major Axis R 2.01 Eccentricity Mass Distance from star ww R 0.00002 6 x 1024 kg 250,000,000 km or 2.5 x 108 km Planet B 4.01 AUR 0.5 2 x 1025 kg 590,000,000 km or 5.9 x 108 km Calculate how long it takes each planet to orbit its star, given the formula T² = R³/(Where T is the orbit time (period), and R is semimajor axis) Explain why the values are different for each planet. (show work) 3 Planet B: Planet A: 2014-8.12 2/5 4₁015 =64,49 64.49² = 4158.97 64.49 = T² 64.49²=4,01 3 8.12²= 65.93 8₁12²2² = 2₁01 A4²³ T=? 8.12=T² Explain: The values are different for both of the planets because they have differe R values. With smaller R value, the Agreater force of gravity. tamamil de Atomim

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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