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A meteor or shooting star [8] is the visible passage of a meteoroid, comet, or asteroid entering Earth's atmosphere. At a speed typically in excess of 20 km/s (72,000 km/h; 45,000 mph), aerodynamic heating of that object produces a streak of light, both from the glowing object and the trail of glowing particles that it leaves in its wake.
Aristotelian physics is the form of natural philosophy described in the works of the Greek philosopher Aristotle (384–322 BC). In his work Physics, Aristotle intended to establish general principles of change that govern all natural bodies, both living and inanimate, celestial and terrestrial – including all motion (change with respect to place), quantitative change (change with respect to ...
Would You Catch a Falling Star. " Would You Catch a Falling Star " is a song written by Bobby Braddock, and recorded by American country music artist John Anderson. It was released in April 1982 as the second single from the album I Just Came Home to Count the Memories. The song reached number 6 on the Billboard Hot Country Singles & Tracks chart.
Classical mechanics. In classical physics and special relativity, an inertial frame of reference (also called an inertial space or a Galilean reference frame) is a frame of reference in which objects exhibit inertia: they remain at rest or in uniform motion relative to the frame until acted upon by external forces.
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In astronomy, a syzygy (/ ˈsɪzədʒi / SIZ-ə-jee; from Ancient Greek συζυγία (suzugía) 'union, yoking', expressing the sense of σύν (syn- "together") and ζυγ- (zug- "a yoke") [1][2]) is a roughly straight-line configuration of three or more celestial bodies in a gravitational system. [3]
The Song: Go and Catch a Falling Star, also known simply as Song, is a poem by John Donne, one of the leading English metaphysical poets.Probably first passed round in manuscript during the final decade of the 16th century, it was not published until the first edition of Donne's collected poems in 1633 - two years after the poet's death. [2]
Stellar rotation is the angular motion of a star about its axis. The rate of rotation can be measured from the spectrum of the star, or by timing the movements of active features on the surface. The rotation of a star produces an equatorial bulge due to centrifugal force. As stars are not solid bodies, they can also undergo differential rotation.