During a solar eclipse, the Moon is positioned directly between Earth and the Sun.The masses of the Sun, Earth, and the Moon are 1.99 x 1030 kg, 5.98 × 1024 kg, and 7.36 x 1022 kg, respectively. The Moon'smean distance from Earth is 3.84 × 10 m, and Earth's mean distance from the Sun is 1.50 × 10'"is G = 6.67 x 10-1' N•m²/kg².m. The gravitational constantFind the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun.2.6 x1045F =NIncorrect

Given Data Mass of the Sun is Msun=1.99×1030 kg Mass of the Earth is Mearth=5.98×1024 kg Mass of the…

During a solar eclipse, the Moon is positioned directly between Earth and the Sun. The masses of the Sun, Earth, and the Moon are 1.99 × 1030 'kg, 5.98 x 1024 kg, and 7.36 x 102 kg, respectively. The Moon's mean distance from Earth is 3.84 x 10° m, and Earth's mean distance from the Sun is 1.50 × 10'' m. The gravitational constant is G = 6.67 x 10-1" N•m²/kg². Find the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun.

During a solar eclipse, the Moon is positioned directly between Earth and the Sun. The masses of the Sun, Earth, and the Moon are 1.99 × 1030 'kg, 5.98 x 1024 kg, and 7.36 x 102 kg, respectively. The Moon's mean distance from Earth is 3.84 x 10° m, and Earth's mean distance from the Sun is 1.50 × 10'' m. The gravitational constant is G = 6.67 x 10-1" N•m²/kg². Find the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun.

Glencoe Physics: Principles and Problems, Student Edition

1st Edition

ISBN:9780078807213

Author:Paul W. Zitzewitz

Publisher:Paul W. Zitzewitz

Chapter7: Gravitation

Section: Chapter Questions

Problem 5STP

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During a solar eclipse, the Moon is positioned directly between Earth and the Sun. The masses of the Sun, Earth, and the Moon are 1.99 × 1030 kg, 5.98 × 1024 kg, and 7.36 × 10²² kg, respectively. The Moon's mean distance from Earth is 3.84 × 108 m, and Earth's mean distance from the Sun is 1.50 × 10¹¹ m. The gravitational constant is G = 6.67 × 10¯¹¹ N-m²/kg². Find the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun. What is the direction of this force? toward the Sun elsewhere toward Venus toward Earth F = N
During a solar eclipse, the Moon is positioned directly between Earth and the Sun. The masses of the Sun, Earth, and the Moon are 1.99 x 1030 kg, 5.98 × 1024 kg, and 7.36 × 1022 kg, respectively. The Moon's mean distance from Earth is 3.84 × 10% m, and Earth's mean distance from the Sun is 1.50 x 10" m. The gravitational constant is G = 6.67 x 10-11 N-m²/kg². Find the magnitude F of the net gravitational force acting on the Moon during the solar eclipse due to both Earth and the Sun. F = N