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  2. Escape velocity - Wikipedia

    en.wikipedia.org/wiki/Escape_velocity

    For example, as the Earth's rotational velocity is 465 m/s at the equator, a rocket launched tangentially from the Earth's equator to the east requires an initial velocity of about 10.735 km/s relative to the moving surface at the point of launch to escape whereas a rocket launched tangentially from the Earth's equator to the west requires an ...

  3. Longevity escape velocity - Wikipedia

    en.wikipedia.org/wiki/Longevity_escape_velocity

    "The first 1000-year-old is probably only ~10 years younger than the first 150-year-old."–Aubrey de Grey, 2005 [1]. In the life extension movement, longevity escape velocity (LEV), actuarial escape velocity [2] or biological escape velocity [3] is a hypothetical situation in which one's remaining life expectancy (not life expectancy at birth) is extended longer than the time that is passing.

  4. Event horizon - Wikipedia

    en.wikipedia.org/wiki/Event_horizon

    One of the best-known examples of an event horizon derives from general relativity's description of a black hole, a celestial object so dense that no nearby matter or radiation can escape its gravitational field. Often, this is described as the boundary within which the black hole's escape velocity is greater than the speed of light.

  5. Parabolic trajectory - Wikipedia

    en.wikipedia.org/wiki/Parabolic_trajectory

    A radial parabolic trajectory is a non-periodic trajectory on a straight line where the relative velocity of the two objects is always the escape velocity. There are two cases: the bodies move away from each other or towards each other. There is a rather simple expression for the position as function of time:

  6. Specific orbital energy - Wikipedia

    en.wikipedia.org/wiki/Specific_orbital_energy

    It is related to the hyperbolic excess velocity (the orbital velocity at infinity) by = =. It is relevant for interplanetary missions. Thus, if orbital position vector ( r {\displaystyle \mathbf {r} } ) and orbital velocity vector ( v {\displaystyle \mathbf {v} } ) are known at one position, and μ {\displaystyle \mu } is known, then the energy ...

  7. Oberth effect - Wikipedia

    en.wikipedia.org/wiki/Oberth_effect

    For example, as a vehicle falls toward periapsis in any orbit (closed or escape orbits) the velocity relative to the central body increases. Briefly burning the engine (an "impulsive burn") prograde at periapsis increases the velocity by the same increment as at any other time ( Δ v {\displaystyle \Delta v} ).

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  9. Newton's cannonball - Wikipedia

    en.wikipedia.org/wiki/Newton's_cannonball

    Beyond the escape velocity, it will leave the Earth without returning (E). Newton's cannonball was a thought experiment Isaac Newton used to hypothesize that the force of gravity was universal, and it was the key force for planetary motion.