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Ch 13: Gravitation
Young & Freedman Calc - University Physics 14th Edition
Young & Freedman Calc14th EditionUniversity PhysicsISBN: 9780321973610당신이 사용하는 게 아니라요?교과서 변경
13장, 문제 18

Ten days after it was launched toward Mars in December 1998, the Mars Climate Orbiter spacecraft (mass 629 kg) was 2.87 × 106 km from the earth and traveling at 1.20 × 104 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?

검증된 단계별 안내
1
To find the spacecraft's kinetic energy relative to the Earth, use the kinetic energy formula: \( KE = \frac{1}{2}mv^2 \), where \( m \) is the mass of the spacecraft and \( v \) is its velocity. First, convert the velocity from km/h to m/s by multiplying by \( \frac{1000}{3600} \).
Substitute the mass of the spacecraft (629 kg) and the converted velocity into the kinetic energy formula to calculate the kinetic energy.
For the potential energy of the Earth-spacecraft system, use the gravitational potential energy formula: \( U = -\frac{G M m}{r} \), where \( G \) is the gravitational constant \( 6.674 \times 10^{-11} \text{Nm}^2/\text{kg}^2 \), \( M \) is the mass of the Earth \( 5.972 \times 10^{24} \text{kg} \), \( m \) is the mass of the spacecraft, and \( r \) is the distance between the Earth and the spacecraft.
Convert the distance from km to meters by multiplying by 1000. Substitute the values of \( G \), \( M \), \( m \), and \( r \) into the potential energy formula to calculate the potential energy.
Ensure all units are consistent (mass in kg, distance in meters, velocity in m/s) and perform the calculations to find the kinetic and potential energies.

비슷한 문제에 대한 검증된 영상 답변:

이 영상 해법은 위 문제에 도움이 된다고 튜터들이 추천한 것입니다.
영상 길이:
10m
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주요 개념

질문에 올바르게 답하기 위해 반드시 이해해야 하는 핵심 개념들은 다음과 같습니다.

Kinetic Energy

Kinetic energy is the energy an object possesses due to its motion, calculated using the formula KE = 0.5 * m * v^2, where m is the mass and v is the velocity of the object. For the Mars Climate Orbiter, this involves converting its velocity from km/h to m/s and using its mass to find the kinetic energy relative to Earth.
추천 영상:
가이드 코스
06:07
Intro to Rotational Kinetic Energy

Gravitational Potential Energy

Gravitational potential energy in a two-body system, like the Earth and the spacecraft, is given by U = -G * (m1 * m2) / r, where G is the gravitational constant, m1 and m2 are the masses of the two bodies, and r is the distance between their centers. This concept helps determine the potential energy of the Earth-spacecraft system based on their separation.
추천 영상:
가이드 코스
06:35
Gravitational Potential Energy

Relative Motion

Relative motion refers to the calculation of an object's motion as observed from a particular frame of reference. In this problem, the spacecraft's velocity and energy are considered relative to Earth, meaning calculations must account for the spacecraft's speed and position as observed from Earth, not an absolute frame.
추천 영상:
가이드 코스
04:27
Intro to Relative Motion (Relative Velocity)
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