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  1. Kepler’s Law of Orbits – The Planets move around the sun in elliptical orbits with the sun at one of the focii. Kepler’s Law of Areas – The line joining a planet to the Sun sweeps out equal areas in equal interval of time. Kepler’s Law of Periods – The square of the time period of the planet is directly proportional to the cube of ...

  2. Importance of Newton’s Universal Law of Gravitation. It has explained us the force that binds us to the earth i.e how every object is pulled from the earth. It explains the motion of the moon around the earth. Also, the motion of the planets around the earth is explained. Suppose you are standing on the top of the building and you throw a ...

  3. Therefore, our equation will come as: Force = [gravitational constant x masses (m1 m2)] / (radius) 2. F = [ m1m2] / r 2. F refers to the force of gravity, N/kg. G is the gravitational constant, 6.67 10−11 N- m2/kg2. m1 will be the 1 st mass, kg. m2 is the 2 nd mass, kg. r refers to the distance between two masses, m.

  4. Black Holes are having very strong gravity in the entire universe. Gravity has the existence with unlimited range. Newton’s law and Kepler’s law are the two popular laws for gravitation. Gravitational force does not depend on the kind of medium. FAQs on gravity and gravitation: Q.1: How are spaceships creating artificial gravity?

  5. Newton’s Second Law of Motion states that force is equal to the change in momentum per change in time. For a constant mass, force equals mass times acceleration, i.e. F = m*a. Learn about the Acceleration in detail here. Newton’s Third Law of Motion states that for every action there is an equal and opposite reaction.

  6. The above diagram represents the motion of an object under the influence of gravity. It is an example of projectile motion (a special case of motion in a plane). The motion of a projectile is considered as a result: Few Examples of Two – Dimensional Projectiles. Throwing a ball or a cannonball. The motion of a billiard ball on the billiard table.

  7. Gravity. Gravity or gravitational force is a type of natural phenomenon. It’s a phenomenon by which all things with energy or mass— even including galaxies, stars, planets, and even light—are brought toward one another. On Earth, Gravity is the cause which gives weight to physical objects. The Moon’s gravity causes the ocean tides.

  8. Specific gravity is a dimensionless quantity. Furthermore, it is independent of the systems of units used for measurements. This is because it is a ratio of densities. Further, it varies with pressure and temperature. Substances which have an SG of 1 are neutrally buoyant in water.

  9. Gravity Academy Laws of Motion 31. A lift is moving downwards with an acceleration equal to acceleration due to gravity. A body of mass M kept on the floor of the lift is pulled horizontally. If the co-efficient of friction is , then the frictional resistance offered by the body is (a) Mg (b) Mg (c) ZuMg (d) zero co such that the block

  10. Newton used Kepler's third law of planetary motion to arrive at the inverse-square rule. He assumed that the orbits of the planets around the Sun are circular, and not elliptical, and so derived the inverse-square rule for gravitational force using the formula for centripetal force.