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Ch 13: Gravitation
Chapter 13, Problem 13

The mass of Venus is 81.5% that of the earth, and its radius is 94.9% that of the earth. (b) If a rock weighs 75.0 N on earth, what would it weigh at the surface of Venus?

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Calculate the mass of Venus by multiplying the mass of Earth by 81.5%. Use the formula: \( M_{Venus} = 0.815 \times M_{Earth} \).
Calculate the radius of Venus by multiplying the radius of Earth by 94.9%. Use the formula: \( R_{Venus} = 0.949 \times R_{Earth} \).
Use the gravitational force formula to find the weight on Venus. The formula is \( F = G \frac{M_{Venus} \times m}{R_{Venus}^2} \), where \( G \) is the gravitational constant, \( M_{Venus} \) is the mass of Venus, \( m \) is the mass of the object, and \( R_{Venus} \) is the radius of Venus.
Calculate the mass of the rock from its weight on Earth using the formula \( m = \frac{W_{Earth}}{g_{Earth}} \), where \( W_{Earth} \) is the weight of the rock on Earth and \( g_{Earth} \) is the acceleration due to gravity on Earth.
Substitute the values of \( M_{Venus} \), \( R_{Venus} \), and \( m \) into the gravitational force formula to find the weight of the rock on Venus.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Weight and Gravitational Force

Weight is the force exerted by gravity on an object, calculated as the product of mass and gravitational acceleration (W = mg). On different celestial bodies, the gravitational acceleration varies due to differences in mass and radius, affecting the weight of objects. Understanding how to calculate weight in different gravitational fields is essential for solving problems involving weight on other planets.
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Gravitational Acceleration

Gravitational acceleration (g) is the acceleration experienced by an object due to the gravitational pull of a planet. It can be calculated using the formula g = G(M/r²), where G is the gravitational constant, M is the mass of the planet, and r is its radius. For Venus, knowing its mass and radius relative to Earth allows us to determine its gravitational acceleration and subsequently the weight of objects on its surface.
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Proportional Relationships

Proportional relationships are used to compare quantities that change in relation to one another. In this context, the weight of an object on Venus can be determined by establishing a ratio based on the gravitational accelerations of Earth and Venus. By understanding how the mass and radius of Venus affect its gravity, we can apply these ratios to find the new weight of the rock when transferred from Earth to Venus.
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Related Practice
Textbook Question
You decide to visit Santa Claus at the north pole to put in a good word about your splendid behavior throughout the year. While there, you notice that the elf Sneezy, when hanging from a rope, produces a tension of 395.0 N in the rope. If Sneezy hangs from a similar rope while delivering presents at the earth's equator, what will the tension in it be? (Recall that the earth is rotating about an axis through its north and south poles.)
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Textbook Question
At what distance above the surface of the earth is the acceleration due to the earth's gravity 0.980 m/s^2 if the acceleration due to gravity at the surface has magnitude 9.80 m/s^2 ?
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Textbook Question
The mass of Venus is 81.5% that of the earth, and its radius is 94.9% that of the earth. (a) Compute the acceleration due to gravity on the surface of Venus from these data.
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Textbook Question
Titania, the largest moon of the planet Uranus, has 1/8 the radius of the earth and 1/1700 the mass of the earth. (a) What is the acceleration due to gravity at the surface of Titania?
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Textbook Question
Titania, the largest moon of the planet Uranus, has 1/8 the radius of the earth and 1/1700 the mass of the earth. (b) What is the average density of Titania? (This is less than the density of rock, which is one piece of evidence that Titania is made primarily of ice.)
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Textbook Question
Ten days after it was launched toward Mars in December 1998, the Mars Climate Orbiter spacecraft (mass 629 kg) was 2.87 * 10^6 km from the earth and traveling at 1.20 * 10^4 km/h relative to the earth. At this time, what were (a) the spacecraft's kinetic energy relative to the earth and (b) the potential energy of the earth–spacecraft system?
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