The gravitational constant appears in Newton's law of universal gravitation, but it was not measured until 1798-71 years after Newton's death-by Henry Cavendish (Philosophical Transactions 1798). Cavendish measured G implicitly, using a torsion balance invented by the geologist Rev. John Michell. He used a horizontal torsion beam with lead balls whose inertia (in relation to the torsion constant) he could tell by timing the beam's oscillation. Their faint attraction to other balls placed alongside the beam was detectable by the deflection it caused. Cavendish's aim was not actually to measure the gravitational constant, but rather to measure the Earth's density relative to water, through the precise knowledge of the gravitational interaction. In retrospect, the density that Cavendish calculated implies a value for G of 6.754 × 10−11 m3/kg/s2.
The accuracy of the measured value of G has increased only modestly since the original Cavendish experiment. G is quite difficult to measure, as gravity is much weaker than other fundamental forces, and an experimental apparatus cannot be separated from the gravitational influence of other bodies. Furthermore, gravity has no established relation to other fundamental forces, so it does not appear possible to calculate it indirectly from other constants that can be measured more accurately, as is done in some other areas of physics. Published values of G have varied rather broadly, and some recent measurements of high precision are, in fact, mutually exclusive.
In the January 5, 2007 issue of Science (page 74), the report "Atom Interferometer Measurement of the Newtonian Constant of Gravity" (J. B. Fixler, G. T. Foster, J. M. McGuirk, and M. A. Kasevich) describes a new measurement of the gravitational constant. According to the abstract: "Here, we report a value of G = 6.693 × 10−11 cubic meters per kilogram second squared, with a standard error of the mean of ±0.027 × 10−11 and a systematic error of ±0.021 × 10−11 cubic meters per kilogram second squared."
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.
(simplified) Gravitational force of attraction is balanced by centripital force due to earths velocity. (G*m1*m2) / r2 = m2 * (v2 / r) m1 = sun mass m2 = earth mass r = earth - sun distance v = earths orbital velocity G = newtons gravitational constant
The gravitational field strength of a planet multiplied by an objects mass gives us the weight of that object, and that the gravitational field strength, g of Earth is equal to the acceleration of free fall at its surface, 9.81ms − 2.
g will increase when rotation is stopped because:- g depend on following thing;:- first on shape of earth second on rotation....(only Equator) not pole third one on going altitude and depth,...........
There is insufficient information in the question to answer it. You did not provide the list of "these". However, it seems obvious that the answer is the tides of the oceans are caused by the gravitational force between the Earth and the Moon, with the Sun also a significant part. Also, it is known that the Moon tends to keep the alignment of the Earth's axis with respect to the plane of the ecliptic relatively constant, stabilizing our seasons.
Gravitational constant was determined by lord Henry cavendish in 1798 using a torsion balance .....G=6.67 *10^-9
The gravitational constant, G, was first determined by Henry Cavendish in 1798 using a torsion balance experiment. This involved measuring the gravitational force between two known masses and the distance between them to calculate G. The value of G is crucial in determining the strength of the gravitational attraction between objects.
Cavendish measured the gravitational constant "G".
g, the force of the Earth's gravitational attraction, is not a constant.
In 1789 Henry Cavendish measured G
There is no evidence to suggest that the gravitational constant 'G' is not the exact same number everywhere in the universe.
G would remain the same, it's the gravitational constant which is the same everywhere in the universe. g would increase by 4 times, assuming that the radius of the earth didn't increase.
Force gravitational = (mass of the object)(the gravitational constant) F=mg "g" is the gravitational constant, it is equal to 9.8 m/s^2
The gravitational constant denoted by letter G, is an empirical physical constant involved in the calculation(s) of gravitational force between two bodies
The gravitational force between two objects is determined by their masses and the distance between them, as given by Newton's law of universal gravitation: ( F = G \frac{{m_1 m_2}}{{r^2}} ), where ( F ) is the gravitational force, ( G ) is the gravitational constant, ( m_1 ) and ( m_2 ) are the masses of the objects, and ( r ) is the distance between their centers.
An upper case (capital) G.
It is m3kg-1s-2