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・ Orbital (comics)
・ Orbital (metro)
・ Orbital (The Culture)
・ Orbital 20
・ Orbital angular momentum
・ Orbital angular momentum multiplexing
・ Orbital angular momentum of light
・ Orbital apex syndrome
・ Orbital arc
・ Orbital artery
・ Orbital ATK
・ Orbital blowout fracture
・ Orbital cellulitis
・ Orbital Corporation
・ Orbital Debris Co-ordination Working Group
Orbital decay
・ Orbital discography
・ Orbital eccentricity
・ Orbital Education
・ Orbital effects on climate
・ Orbital elements
・ Orbital engine
・ Orbital Express
・ Orbital fascia
・ Orbital fissure
・ Orbital foramen
・ Orbital forcing
・ Orbital gyri
・ Orbital hybridisation
・ Orbital inclination


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Orbital decay : ウィキペディア英語版
Orbital decay

In orbital mechanics, decay is a process that leads to gradual decrease of the distance between two orbiting bodies at their closest approach (the periapsis) over many orbital periods. These orbiting bodies can be a planet and its satellite, a star and any object orbiting it, or components of any binary system. The orbital decay can be caused by a multitude of mechanical, gravitational, and electromagnetic effects. For bodies in a low Earth orbit, the most significant effect is the atmospheric drag.
If left unchecked, the decay eventually results in termination of the orbit where the smaller object strikes the surface of the primary; or for objects where the primary has an atmosphere, it burns, explodes, or otherwise breaks up in its atmosphere; or for objects where the primary is a star, ends with incineration by the star's radiation (such as for comets), and so on.
Collisions and mergers of two stellar-mass objects usually produce cataclysmic effects; see stellar collision and gamma-ray burst.
==Causes==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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