출처: 케트론 미첼 윈, 박사, 아산타 쿠레이, 박사, 물리학 및 천문학, 물리 과학 학교, 캘리포니아 대학, 어바인, 캘리포니아
전설에 따르면 아이작 뉴턴은 나무에서 사과가 떨어지는 것을 보았다고 합니다. 그는 사과의 가속을 발견하고 사과에 작용하는 힘이 있었을 것이라고 추론했다. 그런 다음 중력이 나무 꼭대기에서 행동할 수 있다면 더 먼 거리에서 행동할 수도 있다고 추측했다. 그는 달의 움직임과 행성의 궤도를 관찰하고 결국 중력의 보편적 인 법칙을 공식화했다. 법에 따르면 우주의 모든 입자는 질량의 제품에 비례하고 그들 사이의 거리의 제곱에 반비례하는 힘으로 다른 모든 입자를 끌어 들인다고 명시되어 있습니다. 이 힘은 두 입자에 결합하는 선을 따라 작동합니다.
지구 중력으로 인해 지구 표면의 가속 물체인 중력 가속 g가 이 실험실에서 측정됩니다. 지구 표면의 물체에 중력의 크기를 설명하기 때문에 이 값을 정확하게 아는 것은 매우 중요합니다.
The value of g measured from the experimental procedure is shown in Table 1. The freefall time from step 1.4 is recorded in the first column of Table 1. The measured value of g is then calculated using Equation 6. The accuracy of this value can be checked by comparing it to the value of g calculated from Equation 3 using the following values: G = 6.67 x 10-11 m3kg-1s-2, mE = 5.98 x 1024 kg, and rE = 6.38 x 103 km. This comparison is also shown in Table 1 with a percent difference. The percent difference is calculated as:
| measured value – expected value | / expected value. (Equation 7)
A low percent difference indicates that Newton's law of universal gravitation is a very good description of gravity.
Table 1. Results.
| Free Fall Time (s) | Measured g | Calculated g | % difference |
| 0.45 | 9.88 | 9.79 | 0.9 |
The branch of mechanics that is concerned with the analysis of forces on objects that do not move is called statics. Engineers who construct building and bridges use statics to analyze the loads on the structures. The equation F = mg is used throughout this field, so an accurate measurement of g is extremely important in this case. Newton's law of universal gravitation is used by NASA to explore the solar system. When they send probes to Mars and beyond, they use the universal law of gravitation to calculate spacecraft trajectories to a very high level of accuracy. Some scientists are interested in doing experiments in zero-gravity environments. To achieve this, astronauts on the International Space Station perform experiments for them. The space station is in a stable orbit around the Earth because of our understanding of the universal law of gravitation.
In this experiment, the gravitational acceleration of an object on the surface of the Earth was measured. Using a ball with two timing gates attached to a meter stick, the time it took for the ball to travel 1 m from rest was measured. Using kinematic equations, the acceleration g was calculated and found to be very close to the accepted value of 9.8 m/s2.
The Law of Universal Gravitation was the culmination of years of effort by Isaac Newton to understand the force of attraction between masses.
According to legend, when Newton saw an apple dropping from a tree he deduced that a force must draw the apple to the Earth. If this force could act at the top of a tree, it could act at even greater distances. At the time, he was studying the orbits of the moon and planets and eventually formulated the law of universal gravitation to explain their motion.
Newton’s law of universal gravitation states that every particle in the universe attracts every other particle with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
This video will show how to experimentally measure the acceleration due to gravity and compare it to the theoretical value from the equation defining gravitational force.
Before delving into the experiment, let’s examine the principles behind the Law of Universal Gravitation. The gravitational force of the Earth on the moon is equal in magnitude and opposite in direction to the force of the moon on the Earth. This force FG acts along the line joining their centers of mass.
According to the law of gravity, FG equals G – the universal gravitational constant, times the product of the two masses, divided by the square of r, which is the distance between their centers of mass.
With this expression, it is possible to calculate the gravitational force Earth exerts on an object at any distance, including near or at its surface. In the case of the apple falling from a tree, let’s say that the apple’s mass is m, the Earth’s mass is mE and the radius is rE.
Newton’s second law of motion states that force equals mass times acceleration. If we combine this equation, applied to the apple, with the law of gravity, we can cancel the apple’s mass m from both sides. In this context, acceleration is typically denoted by the letter g
Now, the gravitational force on the apple is given by the Law of Universal Gravitation, but from the second law of motion, this force may also be expressed as mg. As we saw earlier with the Earth and moon example, the force of the Earth on the apple is the same as the force of the apple on the Earth. But why do we only see the apple fall toward the Earth? Why do we not see the Earth move toward the apple?
If we look back at Newton’s second law of motion, we can rearrange it to show that acceleration is equal to force divided by mass. That is, for a given force acceleration is inversely proportional to mass. Because the Earth is so much more massive than the apple, the acceleration of the Earth toward the apple is insignificant and essentially undetectable. And that’s why the apple falls from the tree.
Going back to the gravitation equation for g, since all the values on the right hand side – the universal gravitational constant, the mass of the earth and the radius of the earth — are known for an object close to earth’s surface, the magnitude of g is also standard value, which is 9.8 meters per second squared.
However, this value can be calculated experimentally simply by dropping a ball from a known height and applying the kinematical equations. And we will demonstrate how to do that in the following sections.
This experiment uses a metal ball, a meter stick, one sensor from which the ball will be suspended, another sensor on which the ball will land, one timer connected to both sensors, one clamp, and one rod-stand. First, use the clamp to attach the ball sensor to the rod, at least 0.5 meters above the surface of the table. Then, place the second sensor directly below the first sensor.
Next, measure the distance between the top and bottom sensors. The distance should be measured with respect to the bottom of the ball.
Now, release the ball from the sensor so it falls onto the lower sensor and record the time.
Repeat this procedure five times and then calculate the average fall time
From the kinematics video in this collection, we know that this formula describes position in one-dimensional motion of an object with constant acceleration.
Since we are dealing with Earth’s gravitation, the acceleration in this case is the acceleration due to gravity, or g. And the initial velocity is zero, since the ball was at rest before the drop. So if we move the initial position to other side of the equation, the left side becomes y minus y0, which is nothing but d – the distance between the initial and final measure point. Now we can rearrange the equation for g.
For this experiment, d was 0.72 meters and the average free fall time was 0.382 seconds. The resulting experimental gravitational acceleration is 9.9 meters per second squared. Experiment and theory differ only by about 1%, which indicates that Newton’s Law of Universal Gravitation is a very good description of gravitational attraction.
The Universal Law of Gravitation is involved in calculations performed by different branches of engineering.
The branch of mechanical engineering called statics is concerned with the forces on stationary objects, like bridges. Engineers designing bridges use statics, and especially the equation F = mg, throughout their work to analyze structural loads.
A NASA gravity-mapping mission uses two identical satellites-one leading, another trailing-orbiting Earth together. When the leading satellite passes over an ice cap or other mass concentration, it accelerates due to relatively larger force of attraction. The trailing satellite experiences similar acceleration when it passes over the same area.
A ranging system measures how and where the distance changes between them, providing information about the distribution of mass concentrations around the Earth.
You’ve just watched JoVE’s introduction to Newton’s law of universal gravitation. You should now know how to determine the gravitational force between two masses, and understand how to calculate the acceleration due to the force of gravity at the Earth’s surface. Thanks for watching!
