Motion of planets

The motion of planets can be explained by Kepler’s laws of planetary motion, which were derived by the German astronomer Johannes Kepler in the early 17th century based on observations made by the Danish astronomer Tycho Brahe. Kepler’s first law states that the orbit of a planet is an ellipse with the sun at one…

Geostationary orbits

A geostationary orbit is a circular orbit around the Earth, with an altitude of approximately 35,786 km (22,236 miles), in which a satellite appears to remain stationary with respect to a fixed point on the Earth’s surface. This means that the satellite moves at the same rate as the Earth’s rotation, completing one orbit in…

Kepler’s law

Kepler’s laws describe the motion of planets around the Sun. They were formulated by the German astronomer Johannes Kepler in the early 17th century, based on extensive observations made by the Danish astronomer Tycho Brahe. Kepler’s three laws are: Kepler’s laws were crucial in establishing the heliocentric model of the Solar System, in which the…

Acceleration due to gravity

Acceleration due to gravity is the acceleration experienced by an object in the gravitational field of a massive body, such as a planet, moon, or star. The acceleration due to gravity is denoted by the symbol “g” and is usually measured in meters per second squared (m/s²). The value of acceleration due to gravity depends…

Field

Mechanics is a branch of physics that deals with the study of motion, forces, and energy in physical systems. It is a fundamental field of science that provides the basis for understanding the behavior of a wide range of mechanical systems, from simple machines to complex structures like bridges, airplanes, and spacecraft. Mechanics is divided…

Gravitational potential

Gravitational potential is a concept in physics that describes the amount of work that must be done to move an object from one point in a gravitational field to another point. It is usually denoted by the symbol “V” and measured in units of joules per kilogram (J/kg) or meters squared per second squared (m^2/s^2).…

Law of gravitation

The law of gravitation, also known as Newton’s law of gravitation, is a fundamental principle in physics that describes the force of attraction between two objects with mass. The law states that every point mass in the universe attracts every other point mass with a force that is directly proportional to the product of their…

Young’s modulus

Young’s modulus, also known as the modulus of elasticity, is a measure of the stiffness of a material. It is defined as the ratio of stress to strain within the elastic limit of the material. In other words, it measures the amount of stress required to produce a certain amount of strain in a material.…

Hooke’s law

Hooke’s law is a principle in physics that states that the force needed to stretch or compress a spring is proportional to the distance the spring is stretched or compressed from its equilibrium position. This law is named after Robert Hooke, an English physicist who first described it in 1676. Hooke’s law can be expressed…

Angular simple harmonic motions

Angular simple harmonic motion is a type of periodic motion in which an object rotates about a fixed axis with an angular frequency that is proportional to the displacement from the equilibrium position, and the direction of rotation is opposite to the displacement. The equation of angular simple harmonic motion is given by: θ(t) =…