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Encyclopedia :
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DEL :
Delta-v |
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Delta-vIn general physics, delta-v is simply the change in velocity.Depending on the situation delta-v can be referred to as a spatial vector () or scalar (). In both cases it is equal to the acceleration (vector or scalar) integrated over time:
Without gravity delta-v is, in the case of thrust in the direction of the velocity, simply the change in speed. However, in a gravitational field, orbits which are not circular involve changes in speed without requiring any delta-v, while gravity drag can cause the change of speed to be less than delta-v. When applying delta-v in the direction of the velocity and against gravity the specific orbital energy gained per unit delta-v is equal to the instantaneous speed. For a burst of thrust during which both the acceleration produced by the thrust, and the gravity, are constant, the specific orbital energy gained per unit delta-v is the mean value of the speed before and the speed after the burst. The rocket equation shows that the required amount of propellant can dramatically increase, and that the possible payload can dramatically decrease, with increasing delta-v. Therefore in modern spacecraft propulsion systems considerable study is put into reducing the total delta-v needed for a given spaceflight, as well as designing spacecraft that is capable of producing a large delta-v. For the first, see e.g. Hohmann transfer orbit, gravitational slingshot; also, a large thrust reduces gravity drag. For the second some possiblities are: Delta-v is also required to keep satellites in orbit and is expended in orbital stationkeeping maneuvers. See alsoExternal link
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