Home
Class 12
PHYSICS
In Newton's inverse square law of gravit...

In Newton's inverse square law of gravitation had some dependence of radial distance other than `r^(-2)` which on of kepler's three laws of planetary motion would unchanged ?

A

First law on nature of orbits

B

Second law on constant areal velocity

C

Third law on dependence of orbital time period on orbit's semi major axis

D

None of the above

Text Solution

AI Generated Solution

The correct Answer is:
To solve the question regarding which of Kepler's three laws of planetary motion would remain unchanged if Newton's inverse square law of gravitation had some dependence on radial distance other than \( r^{-2} \), we can analyze each of Kepler's laws: ### Step 1: Understand Kepler's Laws Kepler's three laws of planetary motion are: 1. **Kepler's First Law**: The orbit of a planet is an ellipse with the Sun at one of the foci. 2. **Kepler's Second Law**: A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time (law of areas). 3. **Kepler's Third Law**: The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. ### Step 2: Analyze the Effect of Changing the Gravitational Law If we change the gravitational force from being inversely proportional to the square of the distance (\( r^{-2} \)) to some other form, we need to consider how this affects each of Kepler's laws. - **Kepler's First Law**: The shape of the orbit (ellipse) is determined by the gravitational force. If the force changes, the orbits could also change from ellipses to other shapes, thus this law may not remain unchanged. - **Kepler's Second Law**: This law states that the area swept out by a planet in a given time is constant. This law is based on the conservation of angular momentum. Angular momentum depends on the radial distance and the tangential velocity of the planet. If the gravitational force changes, it may affect the velocities and distances, potentially altering the area swept out. Therefore, this law might not remain unchanged. - **Kepler's Third Law**: This law relates the orbital period to the semi-major axis of the orbit. If the gravitational force changes, the relationship between the period and the radius will also change. Hence, this law is likely to be affected. ### Step 3: Conclusion The only law that is fundamentally based on the area swept out over time and not directly dependent on the specific form of the gravitational force is **Kepler's Second Law**. Therefore, even if the gravitational force has a different dependence on distance, the law of areas (Kepler's Second Law) would remain unchanged. ### Final Answer **Kepler's Second Law (Law of Areas) would remain unchanged.** ---
Promotional Banner

Topper's Solved these Questions

  • GRAVITATION

    RESONANCE ENGLISH|Exercise EXERCISE-2 PART-2|10 Videos
  • GRAVITATION

    RESONANCE ENGLISH|Exercise EXERCISE-2 PART-3|12 Videos
  • GRAVITATION

    RESONANCE ENGLISH|Exercise EXERCISE-1 PART-3|2 Videos
  • GEOMATRICAL OPTICS

    RESONANCE ENGLISH|Exercise Advance level Problems|35 Videos
  • NUCLEAR PHYSICS

    RESONANCE ENGLISH|Exercise Advanced level solutions|16 Videos

Similar Questions

Explore conceptually related problems

Deduce the law of gravitation from Kepler’s laws of planetary motion

The inverse square law of intensity (i.e., the intensity prop1/r^2) is valid for a

Statement I: The smaller the orbit of a planet around the Sun, the shorter is the time it takes to complete. Statement II: According to Kepler's third law of planetary motion, square of time period is proportional to cube of mean distance from Sun.

Coulomb's law for electrostatic force between two point charges and Newton's law for gravitational force between two stationary point masses, both have inverse square dependence on the distance between the charges // masees (a) compare the strength of these forces by determining the ratio of their maagnitudes (i) for an electron and as proton (ii) for two protons (b) estimate the accelerations for election and proton due to electrical force of their mutal attraction when they are 1 A apart.

According to Kepler's law of planetary motion, if T represents time period and r is orbital radius, then for two planets these are related as

Kepler's third law states that square of period revolution (T) of a planet around the sun is proportional to third power of average distance i between sun and planet i.e. T^(2)=Kr^(3) here K is constant if the mass of sun and planet are M and m respectively then as per Newton's law of gravitational the force of alteaction between them is F=(GMm)/(r^(2)) , here G is gravitational constant. The relation between G and K is described as

This question contains Statement -1 and Stantement -2 Of the four choices given after the statements, choose the one that best desctibes the two statemesnts. Statement -1: For a mass M kept at the center of a cube of side 'a', the flux of gravitational field passing through its sides 4piGM. Statement -2: If the direction of a field due to a point source is radial and its dependence on the distance 'r' from the source is given as (1)/(r^2) , its flux through a closed surface depends only on the strength of the source enclosed by the surface and not on the size or shape of the surface.

(A) : Newton's third law of motion is applicable only when bodies are in motion. (R) : Newton's third law is not applicable to all types of forces. Like gravitational, electric or magnetic forces etc.

The formula above is Newton's law of universal gratitation, where F is the attractive force, gamma is the gravitational constnat, m_(1)and m_(2) are the masses of the particles, and r is the distnace between their centres of mass. Which of the following givers r in terms of F, gamma , m_(1),and m _(2) ?

When a liquid flows in a tube, there is relative motion between adjacent layers of the liquid. This force is called the viscous force which tends to oppose the relative motion between the layers of the liquid. Newton was the first person to study the factors that govern the viscous force in a liquid. According to Newton’s law of viscous flow, the magnitude of the viscous force on a certain layer of a liquid is given by F = - eta A (dv)/(dx) where A is the area of the layer (dv)/(dx) is the velocity gradient at the layer and eta is the coefficient of viscosity of the liquid. A river is 5 m deep. The velocity of water on its surface is 2 ms^(-1) If the coefficient of viscosity of water is 10 ^(-3 ) Nsm ^(-2) , the viscous force per unit area is :