The value of orbital period using Newton’s version of Kepler’s Third Law: When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

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Answer 1

Question

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

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3.63 • Leaping the River II. A physics professor did daredevil stunts in his spare time. His last stunt was an attempt to jump across a river on a motorcycle (Fig. P3.63). The takeoff ramp was inclined at 53.0°, the river was 40.0 m wide, and the far bank was 15.0 m lower than the top of the ramp. The river itself was 100 m below the ramp. Ignore air resistance. (a) What should his speed have been at the top of the ramp to have just made it to the edge of the far bank? (b) If his speed was only half the value found in part (a), where did he land? Figure P3.63 53.0° 100 m 40.0 m→ 15.0 m

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Answer 2

Question

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

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Answer 3

Question

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

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Answer 4

Question

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Expert Solution & Answer

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Answer 5

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Answer 6

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

Answer 7

Chapter 4, Problem 45EAP

(a)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

Answer 8

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Answer 9

(b)

To determine

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Answer 10

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Answer 11

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Answer 12

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Answer 13

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The value of orbital period using Newton’s version of Kepler’s Third Law: When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

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The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Want to see the full answer?

Chapter 4 Solutions

The value of orbital period using Newton’s version of Kepler’s Third Law: When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

Videos

The value of orbital period using Newton’s version of Kepler’s Third Law: When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

The value of orbital period using Newton’s version of Kepler’s Third Law: When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.

Want to see the full answer?

Chapter 4 Solutions

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having mass twice the mass of the earth is orbiting around a star having the same mass as that of the sun at a distance of 1 AU

The value of orbital period using Newton’s version of Kepler’s Third Law:

When the planet having a mass same as that the mass of the earth is orbiting around a star having a mass four times as that of the sun at a distance of 1 AU.