Definitions for halley's cometˈhæl iz or, often, ˈheɪ liz; ˈhæl i; ˈheɪ li

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Random House Webster's College Dictionary

Hal′ley's com′et*ˈhæl iz or, often, ˈheɪ liz; ˈhæl i; ˈheɪ li(n.)

  1. a comet with a period averaging 76 years: most recently visible in 1986.

    Category: Astronomy

* Pron: The common pronunciation for both the comet and the astronomer Edmund Halley, and the one usu. recommended by astronomers, isHowever, several spellings of the name, including Hailey and Hawley, were in use during the astronomer's own time, when spellings were not yet fixed, and corresponding pronunciations have survived. The pronunciationin particular remains associated with Halley'scomet ; it is less likely to be heard as a pronunciation of Edmund Halley .

Origin of Halley's comet:

after Edmund Halley , who first predicted its return

Freebase

  1. Halley's Comet

    Halley's Comet or Comet Halley, officially designated 1P/Halley, is the best-known of the short-period comets and is visible from Earth every 75–76 years. Halley is the only short-period comet that is clearly visible to the naked eye from Earth, and thus the only naked-eye comet that might appear twice in a human lifetime. Other naked-eye comets may be brighter and more spectacular, but will appear only once in thousands of years. Halley's returns to the inner Solar System have been observed and recorded by astronomers since at least 240 BCE. Clear records of the comet's appearances were made by Chinese, Babylonian, and medieval European chroniclers, but were not recognized as reappearances of the same object at the time. The comet's periodicity was first determined in 1705 by English astronomer Edmond Halley, after whom it is now named. Halley's Comet last appeared in the inner Solar System in 1986 and will next appear in mid-2061. During its 1986 apparition, Halley became the first comet to be observed in detail by spacecraft, providing the first observational data on the structure of a comet nucleus and the mechanism of coma and tail formation. These observations supported a number of longstanding hypotheses about comet construction, particularly Fred Whipple's "dirty snowball" model, which correctly predicted that Halley would be composed of a mixture of volatile ices – such as water, carbon dioxide and ammonia – and dust. The missions also provided data which substantially reformed and reconfigured these ideas; for instance it is now understood that Halley's surface is largely composed of dusty, non-volatile materials, and that only a small portion of it is icy.

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