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 Geo Radius Given Speed of Satellite in its Circular Geo Orbit?
Geo Radius Given Speed of Satellite in its Circular Geo Orbit calculator uses Geostationary Radius = [GM.Earth]/Speed of Satellite^2 to calculate the Geostationary Radius, The Geo Radius Given Speed of Satellite in its Circular Geo Orbit formula is defined as distance from the center of the Earth to the satellite's orbital location. This distance is crucial for geostationary satellites to maintain a synchronized position with the Earth's rotation, allowing them to stay fixed relative to a specific point on the Earth's surface. Geostationary Radius is denoted by Rgso symbol.
How to calculate Geo Radius Given Speed of Satellite in its Circular Geo Orbit using this online calculator? To use this online calculator for Geo Radius Given Speed of Satellite in its Circular Geo Orbit, enter Speed of Satellite (v) and hit the calculate button. Here is how the Geo Radius Given Speed of Satellite in its Circular Geo Orbit calculation can be explained with given input values -> 6.484935 = [GM.Earth]/3070^2.