Miscellaneous

How do you find the value of the gravitational constant G?

How do you find the value of the gravitational constant G?

G is the universal gravitational constant, G = 6.674 x 10-11 m3 kg-1 s-2. M is the mass of the body measured using kg….The Table Below Shows the Value of g at Various Locations from Earth’s Center.

Location Distance from Earth’s Center(m) Value of g (m/s2)
50000 km above surface 5.64 x 107 m 0.13

What is G in Einstein field equation?

where Rμν is the Ricci curvature tensor, and R is the scalar curvature. This is a symmetric second-degree tensor that depends on only the metric tensor and its first and second derivatives. where G is the Newtonian constant of gravitation and c is the speed of light in vacuum.

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What is Einstein gravitational constant?

G = 6.674 30(15)·10-11m³kg-1s-2. Compared with other fundamental constants, G is known only to a comparatively low accuracy.

How is G calculated?

In SI units, G has the value 6.67 × 10-11 Newtons kg-2 m2. The acceleration g=F/m1 due to gravity on the Earth can be calculated by substituting the mass and radii of the Earth into the above equation and hence g= 9.81 m s-2. …

Why is G universal gravitational constant?

G is called the universal gravitational constant because its value is constant and doesn’t change from place to place. which is 6.673 × 10^-11 Nm^2/kg^2. this law is universal in the sense that it is applicable to all the bodies whether the bodies are big or small whether they are celestial or terrestrial.

How did Cavendish find the gravitational constant?

G is a constant that must be determined experimentally. In 1798 Cavendish measured the force between attracting lead spheres with a torsion balance. He knew the masses of the spheres and how far apart they were. He carefully measured the force between them, which allowed him to calculate G.

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What is the formula for the gravitational constant in physics?

g = GM⊕. /. r⊕2. The gravitational constant appears in the Einstein field equations of general relativity, G μ ν + Λ g μ ν = κ T μ ν , {\\displaystyle G_ {\\mu \ u }+\\Lambda g_ {\\mu \ u }=\\kappa T_ {\\mu \ u }\\,,}.

Does the Einstein equation reduce to Newton’s law of gravity?

In the last two articles, we have derived the G μν (Einstein tensor) and T μν (energy-momenum tensor) components of the Einstein equation: We have yet to determine the constant k. To achieve this, we need to show that the Einstein equation reduces to Newton’s law of gravity for weak and static gravitational fields (Newtonian limit).

What are the Einstein field equations?

The Einstein Field Equations are ten equations, contained in the tensor equation shown above, which describe gravity as a result of spacetime being curved by mass and energy. is determined by the curvature of space and time at a particular point in space and time, and is equated with the energy and momentum at that point.

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Why is the gravitational constant so difficult to measure?

Value and uncertainty The gravitational constant is a physical constant that is difficult to measure with high accuracy. This is because the gravitational force is an extremely weak force as compared to other fundamental forces.