The basic equtiion is g=(GM)/(r squared). Where G is the gravitational constant, M is the mass of the object, and r is the radius of the object. There are a lot of other factors to include to get a more accurate number, but this equation will get you in the same ballpark.
... the masses of the bodies involved and the distance between them.
To answer this question we need to know either the height of the Earth station above the Earth or the gravitational acceleration of gravity present at the Earth station initially.Solving without these values:(1/2)Gm/R2 = Gm/r2whereG is the Gravitational Constantm is the mass of the EarthR is the radius of the Earth Station from the center of the Earth.r is the radius of the satellite where gr=1/2ge2R2 = r2SQRT(2)R=r
He didn't. It was first measured by Henry Cavendish in 1798. He used a torsion balance invented by John Mitchel. Google "Cavendish Experiment" for precise details.
The scales have differing uses and so which scale is more useful depends on exactly what the scientist is interested in. The Richter scale is a magnitude scale. This is an estimate of the amount of energy released by an earthquake. The Mercalli scale is an intensity scale. This is an estimate of the perceived severity of ground shaking in differing areas caused by an earthquake. The Richter value is derived based on the amplitude of seismic waves measured on a seismometer and a single value is calculated for a given earthquake. This allows an earthquake to be compared to other earthquakes. The Mercalli intensity value is derived based on the damage caused to buildings and other structures and also based on the measured ground acceleration at a given location. This value can vary depending for a given earthquake on the local ground conditions, the distance from the earthquakes epicentre and the earthquake resistance of buildings. As such, the Richter value is most useful for comparing one earthquake with another, the Mercalli value is most useful for comparing the severity of ground shaking and damage caused by a single earthquake in different locations.
3.14159 26535 89793 23846 26433 83279 50288 41971 69399 37510 3.14159 26535 89793 23846 26433 83279 50288 41971 69399 37510 the "absolute" value of pi cannot be expressed using real numbers since it is and infinite value. The numbers/answers above are only approximations.
The acceleration of gravity due to a single object is(Universal gravitational constant) x (Mass of the object)/(distance from the object's center of mass)2
The acceleration of gravity ... and therefor the weight of any object ... on thesurface of Mercury is 37.698% of its value on the surface of Earth. (rounded)
9.81
9.98
It depends on what planet you are in. If you are talking about the 100 Newton weight on Earth, then the mass is 100 / 9.81 = 10.19 kgThe formula isWeight(N) = Mass(kg) / acceleration due to gravity(m s-2)The value of the acceleration dude to gravity depends on the planet you are in, and that obviously affects the weight. Mass is constant anywhere. On Earth, the acceleration is 9.81 m s-2.
No effect. All masses experience the same acceleration due to gravity.
Acceleration due to gravity on Saturn = 11.171 m/s2 (9.807 m/s2 on Earth)
Newton.
9.8
Yes. That is because the acceleration due to gravity (ag) is larger on Neptune than on Mars. Ag on Neptune is 14.07 m/s2, while ag on Mars is 3.77 m/s2. (For comparison, ag on earth is 9.8 m/s2.)Gravity can be described using this equation:Fg = magwhere m is the mass of an object on a planet, and a is the acceleration due to gravity on a planet.If the mass is constant (the same object on each planet), the value of the force of gravity will be larger on Neptune because the acceleration is larger.
Gravity is about 9.8 meters/second2. This refers to planet Earth, near the surface. The value varies a bit from one place to another. For example, it varies with latitude.
The magnitude of acceleration due to gravity depends on the mass of the object toward which you're attracted by gravity, and on your distance from it. There are trillions of different possibilities in space.