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(astrophysics) The minimum velocity needed to escape the gravitational field of a planet or other body.
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Escape velocity is the minimum speed a ballistic object needs to escape from a massive body such as Earth.
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Escape orbit: A parabolic orbit where the object has escape velocity and is moving directly away from the planet.
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The escape velocity from Earth's surface is about 11 200 m/s, and is irrespective of the direction of the object.
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At a specific horizontal firing speed called escape velocity, dependent on the mass of the planet, an open orbit (E) is achieved that has a parabolic path.
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Many open clusters are inherently unstable, with a small enough mass that the escape velocity of the system is lower than the average velocity of the constituent stars.
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In other words, if given escape velocity, the object will move away from the other body, continually slowing, and will asymptotically approach zero speed as the object's distance approaches infinity, never to come back.
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Originating at the extremely hot surface of the corona, solar wind particles reach escape velocity, streaming outwards at 300 to 800 km/s (671 thousand to 1.79 million mph or 1 to 2.9 million km/h).
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For a mass equal to a Saturn V rocket, the escape velocity relative to the launch pad is 253.5 am/s (8 nanometers per year) faster than the escape velocity relative to the mutual center of mass.
Во основа на оваа идеја, која беше мистериозно оквалификувана од Адам Смит со неговата религиозна објава на ’ Невидливата рака ' е дека ограничената, себична потрага по оваа фиктивна стока некако магично ќе манифестира човечка и социјална благосостојба и напредокWikiMatrix WikiMatrix
Defined a little more formally, "escape velocity" is the initial speed required to go from an initial point in a gravitational potential field to infinity and end at infinity with a residual speed of zero, without any additional acceleration.
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For a given gravitational potential energy at a given position, the escape velocity is the minimum speed an object without propulsion needs to be able to "escape" from the gravity (i.e. so that gravity will never manage to pull it back).
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On the surface of the Earth, the escape velocity is about 11.2 km/s, which is approximately 33 times the speed of sound (Mach 33) and several times the muzzle velocity of a rifle bullet (up to 1.7 km/s).
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Assuming that gravity is the only significant force in the system, this object's speed at any point in the trajectory will be equal to the escape velocity at that point due to the conservation of energy, its total energy must always be 0, which implies that it always has escape velocity; see the derivation above.
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The solar wind then supplies energy that gives some of these ions sufficient velocity to escape Venus's gravity field.
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It has been argued that to conserve energy and momentum, any black holes created in a collision between an UHECR and local matter would necessarily be produced moving at relativistic speed with respect to the Earth, and should escape into space, as their accretion and growth rate should be very slow, while black holes produced in colliders (with components of equal mass) would have some chance of having a velocity less than Earth escape velocity, 11.2 km per sec, and would be liable to capture and subsequent growth.
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14 sinne gevind in 5 ms. Hulle kom uit baie bronne en word nie nagegaan nie.