The effect is noticeable even here on Earth, and in fact it has been used to measure the mean density of the Earth in experiments such as the Schiehallion experiment. The principle is simple: take a pendulum. If there is no large-mass object nearby (such as a mountain), it will hang straight downward, pointing to the center of the planet. But if there is a large-mass object nearby it will pull the pendulum out of true.  In fact, with a sensitive enough instrument, it is possible to measure the gravitational pull of much smaller objects. In 1798 Henry Cavendish used a torsion balance to measured the gravitational attraction between balls of lead. In space, the effect would of course be much greater because the predominant gravitational field of Earth wouldn't be there. Update: clarification I was quite sloppy with my last sentence, as CuriousOne correctly pointed out. Here's what I meant: If you were able to detach the whole mountain from the surface of the planet and take it far from the planet itself, as it seems you are suggesting when you talk about "lifting" the mountain, the effect -the deflection of the pendulum- would indeed be greater. In fact, the gravitational pull exerted by the planet is proportional to $r^{-2}$, where $r$ is the distance from the planet's center. Since the deflection of the pendulum is (see here) $$\theta = \arctan \left(\frac {F_M} {F_E}\right)$$ where $F_M$ is the force exerted by the mountain and ${F_E}$ the force exerted by the Earth, you can see that in this case the deflection would be greater. If you took the mountain an infinite distance away from the planet (into deep space), the deflection would be entirely due to the mountain and you would of course have $\theta = \pi/2$ (the pendulum would point towards the mountain's center of gravity).
In order to continue enjoying our site, we ask that you confirm your identity as a human. Thank you very much for your cooperation. All objects having mass attract each other with a force known as the gravitational force. It is quite noticeable in astronomical objects such as Sun, Earth, and Moon that have enormous masses. The reason is that the force is proportional to the products of the objects’ masses. It is responsible for keeping the planets in motion around the Sun and the Moon around the Earth. Even human beings exert a force on each other, but it is quite insignificant because of relatively low masses. Gravitational force is non-contact since there is no contact between the objects. It is centripetal since it is directed towards the center of the orbit around which the object moves. It is responsible for keeping the body in orbit. The revolving body feels a tug that is directed away from the center. This tug is called the centrifugal force. The gravitational force is the weakest of all fundamental forces.
Many famous scientists have made significant contributions to the field of gravitation. Italian astronomer Galileo Galilei, in the early 17th century, found that all objects accelerate equally towards the center of the Earth. English mathematician Isaac Newton was the first to discover the laws of gravitation in his 1687 seminal work.
Also known as Newton’s Law of Universal Gravitation, the law states that all objects with a mass in the universe attract each other with a force that is
These are the two factors that affect the gravitational force. The value is high for massive objects and when the bodies are closer to one another.
General Formula for Gravitational Force Suppose M1 and M2 be the masses of the two bodies, and R be the distance of separation between their centers. The following equation gives the gravitational force between the two objects. \[ F = \frac{GM_1M_2}{d^2} \hspace{2 cm} (1) \] Unit of Gravitational Force: N or Newton Here, G is called the universal gravitational constant. It is an empirical physical constant, which has a value of 6.67 X 10-11N.m2/kg2. Its dimensional formula is M-1L-3T-2. By knowing the masses M1 and M2 and their distance of separation d, it is possible to calculate the magnitude of F.
Here are some facts and characteristics of gravitational force.
An example of gravitation force in our daily lives is that when an object is thrown in the air, it comes back to the surface due to Earth’s gravitation. Below are some more examples.
Earth exerts a gravitational force on every object, a phenomenon known as gravity. Gravity holds us on the surface and does not let us float freely in the air. We exert the same force on Earth that the Earth exerts on us. However, the Earth is so massive that it is unperturbed. An object suspended in air, if released, will fall freely towards the center of the Earth. The difference between gravitational force and gravity is that the former is applied to any two objects in the universe. Gravity is the force between Earth and any other object close to Earth, including on its surface. The force of gravity is given by, \[ F = \frac{G\hspace{0.1 cm}M_E\hspace{0.1 cm} m}{R_{E}^2} \hspace{2 cm} (2)\] Where ME is the mass of the Earth, m is the mass of an object, and RE is the Earth’s radius. If the object is at an altitude h above the surface of the Earth, then the equation modifies to \[ F = \frac{G\hspace{0.1 cm}M_E\hspace{0.1 cm} m}{(R_{E}+h)^2} \hspace{2 cm} (3)\] From the above equation, it is quite clear that the Earth’s gravitational force vanishes when h →∞, or at large distances from the surface. According to Newton’s second law of motion, force is given by mass m multiplied by acceleration a. Therefore, \[ F = ma \hspace{2 cm} (4) \] Comparing equations (2) and (4), \[ a = \frac{G\hspace{0.1 cm}M_E\hspace{0.1 cm}}{R_{E}^2} \hspace{2 cm} (5) \] The above term is called acceleration due to gravity. It has a value of 9.81 m/s2 on the surface of the Earth. Multiplying g by the mass of a person gives the weight W of the person. \[ W = mg \hspace{2 cm} (6) \] The acceleration due to gravity in space is zero, which is why astronauts feel weightless and float freely. The following expression gives the work done by Earth’s gravitational force when an object of mass m falls from a height h above the Earth’s surface. \[ \text{Work done} = mgh \hspace{2 cm} (7) \] This work is the change in the object’s potential energy as the object falls through the air. Satellites orbit around the Earth in fixed orbits due to the gravitational pull. Had there been no gravity, the satellites would have been flung away into space. The gravity in the polar region is higher than that at the equator. The reason is that the poles are closer to the center of the Earth than the equator. Gravitational Force Between Earth and MoonThe Moon revolves around the Earth because gravitational forces hold them together. We put their masses and the distance between their two centers in equation (1) to calculate this force. Mass of the Earth: ME = 6.0 x 1024 kg Mass of the Moon: MM = 7.35 x 1022 kg The average distance between the Earth and Moon, REM = 3.844 x 108 m Universal gravitational constant, G = 6.67 x 10-11 Nm2/kg2 From equation (1), \[ F = \frac{G M_E M_M}{R_{EM}^2} \\ \Rightarrow F = \frac{6.67 \times 10^{-11} \hspace{0.1 cm} N \cdot m^{2} \cdot kg^{-2} \times 6.0 \times 10^{24} \hspace{0.1 cm} kg \times 7.35 \times 10^{22} \hspace{0.1 cm} kg}{ (3.844 \times 10^{8} \hspace{0.1 cm} m)^2} \\ \Rightarrow F = 2 \times 10^{20} \hspace{0.1 cm} N \] Thus, the gravitational force between the Earth and Moon is 2 x 1020 N. 2. Gravitational Force of the SunThe Sun has a gravitational force due to its mass, which is so large that its influence extends vastly. All planets revolve around the Sun in elliptical orbits due to this attractive force. The gravitational force between the Sun and Earth can be calculated using equation (1). Mass of the Sun: Ms = 2.0 x 1030 kg Mass of the Earth: ME = 6.0 x 1024 kg The average distance between the Sun and Earth, RSE = 1.5 x 1011 m Universal gravitational constant, G = 6.67 x 10-11 Nm2/kg2 From equation (1), \[ F = \frac{G M_S M_E}{R_{SE}^2} \\ \Rightarrow F = \frac{6.67 \times 10^{-11} \hspace{0.1 cm} N \cdot m^{2} \cdot kg^{-2} \times 2.0 \times 10^{30} \hspace{0.1 cm} kg \times 6.0 \times 10^{24} \hspace{0.1 cm} kg}{ (1.5 \times 10^{11} \hspace{0.1 cm} m)^2} \\ \Rightarrow F = 3.5 \times 10^{22} \hspace{0.1 cm} N \] Thus, the gravitational force between the Sun and Earth is 3.5 x 1022 N. Likewise, the gravitational force between the Sun and other planets will depend upon their masses and distances.
All planets of the solar system have their gravitational force. The values of the acceleration due to gravity are given below.
Besides, the gravity of the Moon is 1.62 m/s2. When compared to Earth, it is about 1/6th.
The gravitational force has significant importance that has impacted our daily lives. Here are some of its benefits.
Here are some of its disadvantages.
Q.1. Is gravitational force conservative? Ans. Yes. The gravitational force is conservative since the work done by it around a close path is zero. Q.2. Is there gravitational force in a vacuum? Ans. Yes. There can be a gravitational force in a vacuum. Q.3. What is the range of gravitational force? Ans. The range of the gravitational force is infinite, although it becomes weaker as the distance between objects increases. Q.4. Which measurement changes based on the strength of gravitational force? Ans. Weight. A person’s weight on Earth is not the same on the Moon due to the difference in gravitational forces. Q.5. Which force is stronger? Gravitational or electrical? Ans. The electrical force is stronger than the gravitational force.
Problem 1. What is the gravitational force between two solid objects whose masses are 110 and 130 kgs, and their distance of separation is 80 cms.? Given, G = 6.67 x 10-11 Nm2/kg2. Solution: Given M1 = 110 kg M2 = 130 kg d = 80 cm or 0.8 m F = G M1 M2 / d2 = 6.67 x 10-11 N.m2/kg2 x 110 kg x 130 kg / (0.8)2 = 1.5 X 10-6 N
Article was last reviewed on Sunday, September 4, 2022 |
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