Gravitational acceleration

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In

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At a fixed point on the surface, the magnitude of Earth's gravity results from combined effect of gravitation and the centrifugal force from Earth's rotation.^[2][3] At different points on Earth's surface, the free fall acceleration ranges from 9.764 to 9.834 m/s² (32.03 to 32.26 ft/s²),^[4] depending on altitude, latitude, and longitude. A conventional standard value is defined exactly as 9.80665 m/s² (about 32.1740 ft/s²). Locations of significant variation from this value are known as gravity anomalies. This does not take into account other effects, such as buoyancy or drag.

Relation to the Universal Law

Newton's law of universal gravitation states that there is a gravitational force between any two masses that is equal in magnitude for each mass, and is aligned to draw the two masses toward each other. The formula is:

${\displaystyle F=G{\frac {m_{1}m_{2}}{r^{2}}}\ }$

where ${\displaystyle m_{1}}$ and ${\displaystyle m_{2}}$ are any two masses, ${\displaystyle G}$ is the gravitational constant, and ${\displaystyle r}$ is the distance between the two point-like masses.

Using the integral form of

of each pair rather than the direct total distance between planet centers.)

If one mass is much larger than the other, it is convenient to take it as observational reference and define it as source of a gravitational field of magnitude and orientation given by:[5]

${\displaystyle \mathbf {g} =-{GM \over r^{2}}\mathbf {\hat {r}} }$

where ${\displaystyle M}$ is the mass of the field source (larger), and ${\displaystyle \mathbf {\hat {r}} }$ is a unit vector directed from the field source to the sample (smaller) mass. The negative sign indicates that the force is attractive (points backward, toward the source).

Then the attraction force ${\displaystyle \mathbf {F} }$ vector onto a sample mass ${\displaystyle m}$ can be expressed as:

${\displaystyle \mathbf {F} =m\mathbf {g} }$

Here ${\displaystyle \mathbf {g} }$ is the frictionless, free-fall acceleration sustained by the sampling mass ${\displaystyle m}$ under the attraction of the gravitational source. It is a vector oriented toward the field source, of magnitude measured in acceleration units. The gravitational acceleration vector depends only on how massive the field source ${\displaystyle M}$ is and on the distance 'r' to the sample mass ${\displaystyle m}$. It does not depend on the magnitude of the small sample mass.

This model represents the "far-field" gravitational acceleration associated with a massive body. When the dimensions of a body are not trivial compared to the distances of interest, the principle of superposition can be used for differential masses for an assumed density distribution throughout the body in order to get a more detailed model of the "near-field" gravitational acceleration. For satellites in orbit, the far-field model is sufficient for rough calculations of altitude versus period, but not for precision estimation of future location after multiple orbits.

The more detailed models include (among other things) the

mission from 2011 to 2012 consisted of two probes ("Ebb" and "Flow") in polar orbit around the Moon to more precisely determine the gravitational field for future navigational purposes, and to infer information about the Moon's physical makeup.

Comparative gravities of the Earth, Sun, Moon, and planets

The table below shows comparative gravitational accelerations at the surface of the Sun, the Earth's moon, each of the planets in the Solar System and their major moons, Ceres, Pluto, and Eris. For gaseous bodies, the "surface" is taken to mean visible surface: the cloud tops of the

. The values in the table have not been de-rated for the centrifugal force effect of planet rotation (and cloud-top wind speeds for the gas giants) and therefore, generally speaking, are similar to the actual gravity that would be experienced near the poles. For reference the time it would take an object to fall 100 meters, the height of a skyscraper, is shown, along with the maximum speed reached. Air resistance is neglected.

Body	Multiple of Earth gravity	m/s2	ft/s2	Notes	Time to fall 100 m and maximum speed reached
Sun	27.90	274.1	899		0.85 s	843 km/h (524 mph)
Mercury	0.3770	3.703	12.15		7.4 s	98 km/h (61 mph)
Venus	0.9032	8.872	29.11		4.8 s	152 km/h (94 mph)
Earth	1	9.8067	32.174	[a]	4.5 s	159 km/h (99 mph)
Moon	0.1655	1.625	5.33		11.1 s	65 km/h (40 mph)
Mars	0.3895	3.728	12.23		7.3 s	98 km/h (61 mph)
Ceres	0.029	0.28	0.92		26.7 s	27 km/h (17 mph)
Jupiter	2.640	25.93	85.1		2.8 s	259 km/h (161 mph)
Io	0.182	1.789	5.87		10.6 s	68 km/h (42 mph)
Europa	0.134	1.314	4.31		12.3 s	58 km/h (36 mph)
Ganymede	0.145	1.426	4.68		11.8 s	61 km/h (38 mph)
Callisto	0.126	1.24	4.1		12.7 s	57 km/h (35 mph)
Saturn	1.139	11.19	36.7		4.2 s	170 km/h (110 mph)
Titan	0.138	1.3455	4.414		12.2 s	59 km/h (37 mph)
Uranus	0.917	9.01	29.6		4.7 s	153 km/h (95 mph)
Titania	0.039	0.379	1.24		23.0 s	31 km/h (19 mph)
Oberon	0.035	0.347	1.14		24.0 s	30 km/h (19 mph)
Neptune	1.148	11.28	37.0		4.2 s	171 km/h (106 mph)
Triton	0.079	0.779	2.56		16.0 s	45 km/h (28 mph)
Pluto	0.0621	0.610	2.00		18.1 s	40 km/h (25 mph)
Eris	0.0814	0.8	2.6	(approx.)	15.8 s	46 km/h (29 mph)

General relativity

In Einstein's theory of

) on the curved spacetime.

Gravitational field

See also

Notes

References