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the claim
The mass of the Earth is determined using gravitational physics constants
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SUPPORTED
the evidence backs this
refutedsupported
the weight of evidence
8 sources for · 0 against

Retrieved physical and geodetic literature demonstrates that determinations of the Earth's mass and geocentric gravitational parameter rely on gravitational physics equations and satellite orbital data.

Evidence for · 8
1992 · cited by 101
In most of the recent determinations of the geocentric gravitational coefficient (GM) of the Earth, the laser ranging data to the Lageos satellite have had the greatest influence on the solution. These data, however, have generally been processed with a small but significant error in one of the range corrections. In a new determination of GM using the corrected center‐of‐mass offset, a value of 398600.4415 km3/sec2 (including the mass of the atmosphere) has been obtained, with an estimated uncertainty (1 σ) of 0.0008 km3/sec2.
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rails:sufficiency:supported:for=2+6p:against=0+0p | v55:sufficiency

More for · 7
cited by 0
Another way gravitational potential energy helps us is by keeping earth and the other planets in orbit in our solar system around the Sun. Formula and example The mathematical formula for the gravitational potential energy: Gravitational potential energy = Where: - m is the mass of the object , - g is the gravitational acceleration of the object , and - h is the height above a chosen point. Most scientists and students use these measurement unit: - The value m is in kilograms. - The value h is in metres. - The value g is a physical constant with the value of 9.81 metres per second squared. This is known as the gravitational constant. - The value of the gravitational potential energy that is calculated using values in the above units is called the Joule (J). For example, an object with a mass of 1.5 kilograms that is 2.5 metres above the ground would have a gravitational potential energy value of: joules.
2024 · cited by 0
Physical properties of the Sun (orientation of rotation axis, oblateness coefficient J 2 ⊙ , and change rate of the gravitational parameter μ ˙ ⊙ ) are determined using a dynamical model describing the motion of the Sun, planets, the Moon, asteroids, and Trans-Neptunian objects (TNOs). Among the many kinds of observations used to determine the orbits and physical properties of the bodies, the most important for our study are precise interplanetary ranging data: Earth–Mercury ranges from MESSENGER spacecraft and Earth–Mars ranges from Odyssey and MRO. The findings allow us to improve the model of the Sun in modern planetary ephemerides. First, the dynamically determined direction of the Sun’s pole is ≈2° off the visible axis of rotation of the Sun’s surface, which is corroborated by present knowledge of the Sun’s interior. Second, the change rate of the Sun’s gravitational parameter is found to be smaller (in absolute value) than the nominal value derived from the estimate of mass loss through radiation and solar wind. Possible interpretations are discussed.
1952 · cited by 0
Publisher Summary This chapter discusses the ways in which gravitational attraction is utilized. It also summarizes the fundamental facts concerning the Earth's gravity field. Any measured value of gravity is a composite of many mass effects that includes the shape and size of the earth as a whole, the rotation of the earth, changes in elevation, horizontal mass discontinuities, and changes in topographic configuration. The largest and most easily measured changes in gravity are related to the change in shape of the earth. Therefore, these gravity measurements are an integral part of the geodetic program. Other geologic uses of gravity data include earth crystal studies, geological exploration, and gravity studies of the strength of the earth. With regard to national gravity base values, the principal difficulty in using gravity work, particularly for the study of the geoid, lies in getting all data on absolute datum. To eliminate confusion about the absolute gravity datum, the value determined at the Geodetic Institute at Potsdam is adopted by international agreement as a base value and all values are referred to it.
1976 · cited by 0
times round the Earth in one second, so that the cir¬ cumference of the earth is about ‘one-seventh … mass - is also the mass which determines the magnitude of the gravitational force acting on … hope, contribute to the revival of the old idea that physics should be, above all, ‘natural
2018 · cited by 0
Fossil fuels are intensively extracted from around the world faster than they are renewed. Regardless of direct and indirect effects of such extractions on climate change and biosphere, another issue relating to Earth's internal structure and Earth mass should receive at least some interest. According to the Energy Information Administration (EIA), about 34 billion barrels of oil (~4.7 trillion metric tons) and 9 billion tons of coal have been extracted in 2014 worldwide. Converting the amounts of oil and coal extracted over the last 3 decades and their respective reserves, intended to be extracted in the future, into mass values suggests that about 355 trillion tons, or ~5.86∗10(-9) (~0.0000000058)% of the Earth mass, would be 'lost'. Although this is a tiny percentage, modeling the potential loss of Earth mass may help figuring out a critical threshold of mass loss that should not be exceeded. Here, I briefly discuss whether such loss would have any potential consequences on the Earth's internal structure and on its gravitational force based on the Newton's law of gravitation that links the attraction force between planets to their respective masses and the distance that separate them.
cited by 0
net force is applied. In physics, mass is not the same as weight, even though mass is often determined by measuring the object's weight using a spring In physics, mass is an intrinsic positive physical quantity of a body, which measures its resistance to acceleration. In modern physics, it is generally defined as the strength of an object's gravitational attraction to other bodies — as measured by an observer moving along at the same speed. The unit of mass in the International System of Units (SI) is the kilogram (kg). Since 1905, mass can also In physics, mass is an intrinsic positive physical quantity of a body, which measures its resistance to acceleration. In modern physics, it is generally defined as the strength of an object's gravitational attraction to other bodies — as measured by an observer moving along at the same speed. The unit of mass in the International System of Units (SI) is the kilogram (kg). Since 1905, mass can also be understood as a measure of the energy content of a body (see E=mc²). Mass can be experimentally defined as a measure of the body's inertia, meaning the resistance to acceleration (change of velocity) when a net force is applied. In physics, mass is not the same as weight, even though mass is often determined by measuring the object's weight using a spring scale, rather than balance scale comparing it directly with known masses. An object on the Moon would weigh less than it does on Earth because of the lower gravity, but it would still have the same mass. This is because weight is a force, while mass is the property that (along with gravity) determines the strength of this force. In… w…
cited by 0
that the total gravitation of the earth , assumed as spherical, on external bodies, would be the same as if the earth’s mass were concentrated in the centre
Everything we examined (8) — 7 independent sources
This check searched the claim as stated. It did not run a separate search for evidence against it.
  1. Simple English Wikipedia: Gravitational energyreferencesame source L3no side taken
  2. Studying the Properties of Spacetime with an Improved Dynamical Model of the Inner Solar Systempeer-reviewedno side taken
  3. The Earth's Gravitational Field and Its Exploitationpeer-reviewedno side taken
  4. Principles of cosmology and gravitationreferenceno side taken
  5. Oil, Earth mass and gravitational forcepeer-reviewedno side taken
  6. Massreferencesame source L3no side taken
  7. Progress in the determination of the gravitational coefficient of the Earthreferenceno side taken
  8. 1911 Encyclopædia Britannica/Gravitationreferenceno side taken
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first checked02 Aug 2026
judged → COMMON KNOWLEDGE · 9502 Aug 2026
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