Standard gravitational parameter

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SUMMARY

The standard gravitational parameter (G*M) is measured with greater accuracy than the gravitational constant (G). Observations of planetary orbits around the Sun have established the Sun's standard gravitational parameter to 11 significant digits, while Earth's parameter is known to 9 or 10 significant digits. The challenge lies in isolating G from G*M, as G is only known to 4 or 5 significant digits, primarily due to limitations in measuring the Earth's mass accurately. Remote sensing projects, such as those conducted by NASA's GRACE mission, provide insights into the Earth's dimensions and composition but are limited to measuring G*Me.

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  • Understanding of gravitational parameters and constants
  • Familiarity with celestial mechanics and orbital dynamics
  • Knowledge of remote sensing techniques in geophysics
  • Basic principles of mass measurement and uncertainty analysis
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  • Research the methods used in remote sensing projects like NASA's GRACE mission
  • Study the implications of gravitational constant measurements on astrophysics
  • Explore the relationship between G, M, and the standard gravitational parameter in detail
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Sanjay87
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Hi,

Is it true that the standard gravitational parameter of an object (G*M) is more accurately known than the the gravitational constant (G)? If so, why? Any references would be much appreciated.

Thanks,
San
 
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Yes, its true. We can measure the standard gravitational parameter of some object by observing other objects orbits about the object in question. With hundreds of years of observing planets in orbit about the Sun, we have the standard gravitational parameter for the Sun nailed down extremely well (11 significant digits). We know the standard gravitational parameter for the Earth to 9 or 10 significant digits. While we can measure G*M very precisely, untangling G (or M) from G*M is a much harder task. We only know G to 4 or 5 significant digits.
 
i think what this also means (and i don't know which is cause and effect) is that we don't know the mass of the Earth precisely. i know it's true that G*M is known to 10 digits and that G only to 5 (by measurement with a Cavendish-like experiment) but i find it unexpected that knowing the dimensions and composition of the Earth well, of the mutual orbit of these (unequal) twin planets around their common center of gravity, that with years of astronomical observation of the Moon, that we wouldn't have gotten that more precisely.
 
Why do you think we know the composition of the Earth well? (Better than 10 parts per million, which is what 5 digits of accuracy means) Most of it is underground. :)
 
rbj said:
i think what this also means (and i don't know which is cause and effect) is that we don't know the mass of the Earth precisely.
That is exactly right. The uncertainty in the Earth's mass is for, all practical purposes, entirely due to the uncertainty in G.
but i find it unexpected that knowing the dimensions and composition of the Earth well
Vanadium 50 already asked the key question here. Piling on, one of the key sources of insight into the dimensions and composition of the Earth comes from remote sensing projects such as http://grace.jpl.nasa.gov/" . The problem here is that these remote sensing experiments are sensitive only to the product G*Me.
... of the mutual orbit of these (unequal) twin planets around their common center of gravity, that with years of astronomical observation of the Moon, that we wouldn't have gotten that more precisely.
What these observations give us insight into is the Earth's standard gravitational parameter, the Earth/Moon mass ratio, and the Sun/(Earth+Moon) mass ratio. They do not give direct insight to the Earth's mass unencumbered with G.
 
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