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2a)Isaac Newton was able to determine the factors that give Kepler’s constant k its value. According...

2a)Isaac Newton was able to determine the factors that give Kepler’s constant k its value. According to Newton, k = 4π 2 GM , where G is the Universal Constant of Gravitation, and M is the mass of the object about which the planet or moon is orbitting. a) Using Newton’s relationship for Kepler’s constant, find the value of k for the Sun, given that its mass is 1.99 · 1030 kg. How does this value compare with the result which you obtained in problem 2, part b)? b) If Earth were orbitting a star that were 4x more massive than the Sun, what would happen to the value of k for its orbit?

b) The orbital velocity for a planet or satellite is given by vo = s GM r , where M is the mass of the object in the center of the orbit, and r is the orbital radius (assuming circular orbits). Estimate the orbital velocity of the Earth around the Sun in meters per second.

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