The table below illustrates data on Kepler's 3rd Law for the first six planets.Use it to estimate the semi-major axis of the object Hathor 2340 which has an orbital period of 0.77 yearsp (years) p2a3 a (AU)Mercury0.240.058 0.0580.39Venus0.620.380.380.72Earth1.001.001.001.00Mars1.883.543.541.52Jupiter11.91411415.20Saturn29.58688689.54А. 13.7 AUO B. 0.84 AUОС. 1.41 AUD. 2.55 AUO E. 1.05 AU

According to Kepler's third law, The ratio of square of time period to the cube of semimajor axis of…

The table below illustrates data on Kepler's 3rd Law for the first six planets. Use it to estimate the semi-major axis of the object Hathor 2340 which has an orbital period of 0.77 years p (years) p2 a (AU) Mercury 0.24 0.058 0.058 0.39 Venus 0.62 0.38 0.38 0.72 Earth 1.00 1.00 1.00 1.00 Mars 1.88 3.54 3.54 1.52 Jupiter 11.9 141 141 5.20 Saturn 29.5 868 868 9.54 A. 13.7 AU B. 0.84 AU O C. 1.41 AU D. 2.55 AU O E. 1.05 AU

The table below illustrates data on Kepler's 3rd Law for the first six planets. Use it to estimate the semi-major axis of the object Hathor 2340 which has an orbital period of 0.77 years p (years) p2 a (AU) Mercury 0.24 0.058 0.058 0.39 Venus 0.62 0.38 0.38 0.72 Earth 1.00 1.00 1.00 1.00 Mars 1.88 3.54 3.54 1.52 Jupiter 11.9 141 141 5.20 Saturn 29.5 868 868 9.54 A. 13.7 AU B. 0.84 AU O C. 1.41 AU D. 2.55 AU O E. 1.05 AU

Glencoe Physics: Principles and Problems, Student Edition

1st Edition

ISBN:9780078807213

Author:Paul W. Zitzewitz

Publisher:Paul W. Zitzewitz

Chapter7: Gravitation

Section7.1: Planetary Motion And Gravitation

Problem 5PP

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