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  2. Relative velocity - Wikipedia

    en.wikipedia.org/wiki/Relative_velocity

    Relative velocities between two particles in classical mechanics. The figure shows two objects A and B moving at constant velocity. The equations of motion are: = +, = +, where the subscript i refers to the initial displacement (at time t equal to zero).

  3. List of equations in classical mechanics - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    Classical mechanics is the branch of physics used to describe the motion of macroscopic objects. [1] It is the most familiar of the theories of physics. The concepts it covers, such as mass, acceleration, and force, are commonly used and known. [2]

  4. Faster-than-light - Wikipedia

    en.wikipedia.org/wiki/Faster-than-light

    That is, special relativity gives the correct velocity-addition formula for computing such relative velocity. It is instructive to compute the relative velocity of particles moving at v and −v in accelerator frame, which corresponds to the closing speed of 2v > c. Expressing the speeds in units of c, β = v/c:

  5. List of relativistic equations - Wikipedia

    en.wikipedia.org/wiki/List_of_relativistic_equations

    In other words, the laws of physics will be the same whether you are testing them in a frame 'at rest', or a frame moving with a constant velocity relative to the 'rest' frame. The speed of light in a perfect classical vacuum ( c 0 {\displaystyle c_{0}} ) is measured to be the same by all observers in inertial frames and is, moreover, finite ...

  6. Relativistic mechanics - Wikipedia

    en.wikipedia.org/wiki/Relativistic_mechanics

    Looking at the above formula for invariant mass of a system, one sees that, when a single massive object is at rest (v = 0, p = 0), there is a non-zero mass remaining: m 0 = E/c 2. The corresponding energy, which is also the total energy when a single particle is at rest, is referred to as "rest energy".

  7. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    A proper motion of 1 arcsec per year 1 light-year away corresponds to a relative transverse speed of 1.45 km/s. Barnard's Star's transverse speed is 90 km/s and its radial velocity is 111 km/s (perpendicular (at a right, 90° angle), which gives a true or "space" motion of 142 km/s.

  8. Corpus Christi ISD science fair promotes STEM - AOL

    www.aol.com/corpus-christi-isd-science-fair...

    Brittany Flores speaks to first grade son Rey Flores Jr. about his science fair project at Miller High School on Friday, Jan. 19, 2024, in Corpus Christi, Texas. Father Rey Flores stands in the ...

  9. Michelson–Morley experiment - Wikipedia

    en.wikipedia.org/wiki/Michelson–Morley_experiment

    Alternatively, consider the rearrangement of the speed of light formula =. If the relation v 2 / c 2 << 1 {\displaystyle {v^{2}}/{c^{2}}<<1} is true (if the velocity of the aether is small relative to the speed of light), then the expression can be simplified using a first order binomial expansion;