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  2. Cavendish experiment - Wikipedia

    en.wikipedia.org/wiki/Cavendish_experiment

    Since there are two balls, each experiencing force F at a distance ⁠ L / 2 ⁠ from the axis of the balance, the torque due to gravitational force is LF. At equilibrium (when the balance has been stabilized at an angle θ {\displaystyle \theta } ), the total amount of torque must be zero as these two sources of torque balance out.

  3. Coriolis frequency - Wikipedia

    en.wikipedia.org/wiki/Coriolis_frequency

    Replacing =, where is the magnitude of the spin rate of the Earth, to obtain f = ω = 2 Ω sin ⁡ φ . {\displaystyle f=\omega =2\Omega \sin \varphi .} Thus the Coriolis parameter, f {\displaystyle f} , is the angular velocity or frequency required to maintain a body at a fixed circle of latitude or zonal region.

  4. Geopotential spherical harmonic model - Wikipedia

    en.wikipedia.org/wiki/Geopotential_spherical...

    As P 0 n (x) = −P 0 n (−x) non-zero coefficients J n for odd n correspond to a lack of symmetry "north–south" relative the equatorial plane for the mass distribution of Earth. Non-zero coefficients C n m, S n m correspond to a lack of rotational symmetry around the polar axis for the mass distribution of Earth, i.e. to a "tri-axiality" of ...

  5. Gravitational wave - Wikipedia

    en.wikipedia.org/wiki/Gravitational_wave

    This type of instrument was the first type of gravitational wave detector. Strains in space due to an incident gravitational wave excite the bar's resonant frequency and could thus be amplified to detectable levels. Conceivably, a nearby supernova might be strong enough to be seen without resonant amplification.

  6. Schwarzschild geodesics - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild_geodesics

    The basic idea is that, due to gravitational slowing of time, parts of a wave-front closer to a gravitating mass move more slowly than those further away, thus bending the direction of the wave-front's propagation. Using general covariance, the Hamilton–Jacobi equation for a single particle of unit mass can be expressed in arbitrary ...

  7. Projectile motion - Wikipedia

    en.wikipedia.org/wiki/Projectile_motion

    The only force of mathematical significance that is actively exerted on the object is gravity, which acts downward, thus imparting to the object a downward acceleration towards Earth's center of mass. Due to the object's inertia, no external force is needed to maintain the horizontal velocity component of the object's motion.

  8. Theta wave - Wikipedia

    en.wikipedia.org/wiki/Theta_wave

    Theta waves generate the theta rhythm, a neural oscillation in the brain that underlies various aspects of cognition and behavior, including learning, memory, and spatial navigation in many animals. [ 1 ] [ 2 ] It can be recorded using various electrophysiological methods, such as electroencephalogram (EEG), recorded either from inside the ...

  9. Newton's law of universal gravitation - Wikipedia

    en.wikipedia.org/wiki/Newton's_law_of_universal...

    The theorem tells us how different parts of the mass distribution affect the gravitational force measured at a point located a distance r 0 from the center of the mass distribution: [13] The portion of the mass that is located at radii r < r 0 causes the same force at the radius r 0 as if all of the mass enclosed within a sphere of radius r 0 ...