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  2. Gravity of Earth - Wikipedia

    en.wikipedia.org/wiki/Gravity_of_Earth

    The gravity g′ at depth d is given by g′ = g(1 − d/R) where g is acceleration due to gravity on the surface of the Earth, d is depth and R is the radius of the Earth. If the density decreased linearly with increasing radius from a density ρ 0 at the center to ρ 1 at the surface, then ρ(r) = ρ 0 − (ρ 0 − ρ 1) r / R, and the ...

  3. Theoretical gravity - Wikipedia

    en.wikipedia.org/wiki/Theoretical_gravity

    The component due to the Earth's rotation can then be included, if appropriate, based on a sidereal day relative to the stars (≈366.24 days/year) rather than on a solar day (≈365.24 days/year). That component is perpendicular to the axis of rotation rather than to the surface of the Earth.

  4. Gamma (eclipse) - Wikipedia

    en.wikipedia.org/wiki/Gamma_(eclipse)

    The sign of gamma defines, for a solar eclipse, if the axis of the shadow passes north or south of the center of the Earth; a positive value means north.The Earth is defined as that half which is exposed to the Sun (this changes with the seasons and is not related directly to the Earth's poles or equator; thus, the Earth's center is wherever the Sun is directly overhead).

  5. Gravitational constant - Wikipedia

    en.wikipedia.org/wiki/Gravitational_constant

    The constant of proportionality, G, in this non-relativistic formulation is the gravitational constant. Colloquially, the gravitational constant is also called "Big G", distinct from "small g" (g), which is the local gravitational field of Earth (also referred to as free-fall acceleration).

  6. Curved spacetime - Wikipedia

    en.wikipedia.org/wiki/Curved_spacetime

    It is the cumulative total effect of many local manifestations of curvature that result in the appearance of a gravitational force acting at a long range from Earth. [ 1 ] : 175–190 Different observers viewing the scenarios presented in this figure interpret the scenarios differently depending on their knowledge of the situation.

  7. Mathematics of general relativity - Wikipedia

    en.wikipedia.org/wiki/Mathematics_of_general...

    A principal feature of general relativity is to determine the paths of particles and radiation in gravitational fields. This is accomplished by solving the geodesic equations. The EFE relate the total matter (energy) distribution to the curvature of spacetime. Their nonlinearity leads to a problem in determining the precise motion of matter in ...

  8. Inside the totality -- or how I learned to stop worrying and ...

    www.aol.com/inside-totality-learned-stop...

    Apr. 8—LEAKEY, Texas — The emergency weather and road condition signs along Interstate 10 proclaim: Find a spot and stay put. So we did. But the clouds, the sun and the moon didn't listen. As ...

  9. Gravitational lens - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lens

    A light source passes behind a gravitational lens (invisible point mass placed in the center of the image). The aqua circle is the light source as it would be seen if there were no lens, while white spots are the multiple images of the source (see Einstein ring).