Kepler's Laws and Gravitational Attraction
Johannes Kepler's laws of planetary motion, developed in the 17th century, provided significant insights into the relationship between celestial bodies and gravity. Kepler's laws describe the elliptical orbits of planets and other objects in the solar system, all of which are governed by the gravitational pull of the central body, such as the Sun. These laws laid the foundation for understanding how gravity affects the motion of objects in space, paving the way for Sir Isaac Newton's formulation of the law of universal gravitation.
How to Calculate Speed of Satellite in its Circular GEO of Radius?
Speed of Satellite in its Circular GEO of Radius calculator uses Speed of Satellite = sqrt([GM.Earth]/(Geostationary Radius)) to calculate the Speed of Satellite, The Speed of Satellite in its Circular GEO of Radius formula is defined as velocity at which a satellite orbits the Earth in a geostationary orbit. Speed of Satellite is denoted by v symbol.
How to calculate Speed of Satellite in its Circular GEO of Radius using this online calculator? To use this online calculator for Speed of Satellite in its Circular GEO of Radius, enter Geostationary Radius (Rgso) and hit the calculate button. Here is how the Speed of Satellite in its Circular GEO of Radius calculation can be explained with given input values -> 0.003075 = sqrt([GM.Earth]/(42164170)).