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  2. Gravitational time dilation - Wikipedia

    en.wikipedia.org/wiki/Gravitational_time_dilation

    Gravitational time dilation is a form of time dilation, an actual difference of elapsed time between two events, as measured by observers situated at varying distances from a gravitating mass. The lower the gravitational potential (the closer the clock is to the source of gravitation), the slower time passes, speeding up as the gravitational ...

  3. Time dilation - Wikipedia

    en.wikipedia.org/wiki/Time_dilation

    It has also been calculated that due to time dilation, the core of the Earth is 2.5 years younger than the crust. [34] "A clock used to time a full rotation of the Earth will measure the day to be approximately an extra 10 ns/day longer for every km of altitude above the reference geoid."

  4. Gravitational redshift - Wikipedia

    en.wikipedia.org/wiki/Gravitational_redshift

    The effect of gravity on light was then explored by Johann Georg von Soldner (1801), who calculated the amount of deflection of a light ray by the Sun, arriving at the Newtonian answer which is half the value predicted by general relativity. All of this early work assumed that light could slow down and fall, which is inconsistent with the ...

  5. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    For example, the Schwarzschild radius r s of the Earth is roughly 9 mm (3 ⁄ 8 inch); at the surface of the Earth, the corrections to Newtonian gravity are only one part in a billion. The Schwarzschild radius of the Sun is much larger, roughly 2953 meters, but at its surface, the ratio r s / r is roughly 4 parts in a million.

  6. General relativity - Wikipedia

    en.wikipedia.org/wiki/General_relativity

    For the Moon–Earth system, this effect has been measured with the help of lunar laser ranging. [102] More recently, it has been measured for test masses aboard the satellite Gravity Probe B to a precision of better than 0.3%. [103] [104] Near a rotating mass, there are gravitomagnetic or frame-dragging effects. A distant observer will ...

  7. 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.

  8. Introduction to general relativity - Wikipedia

    en.wikipedia.org/wiki/Introduction_to_general...

    Objects are falling to the floor because the room is aboard a rocket in space, which is accelerating at 9.81 m/s 2, the standard gravity on Earth, and is far from any source of gravity. The objects are being pulled towards the floor by the same "inertial force" that presses the driver of an accelerating car into the back of their seat.

  9. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    The tropical year is the length of time that the Sun, as viewed from the Earth, takes to return to the same position along the ecliptic (its path among the stars on the celestial sphere). The sidereal year is the length of time that the Sun takes to return to the same position with respect to the stars of the celestial sphere. Precession causes ...