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单词 nova
释义

nova

[ noh-vuh ]
/ ˈnoʊ və /
SEE SYNONYMS FOR nova ON THESAURUS.COM

noun, plural no·vas, no·vae [noh-vee]. /ˈnoʊ vi/. Astronomy.

a star that suddenly becomes thousands of times brighter and then gradually fades to its original intensity.
Compare supernova.

Origin of nova

1680–90; <New Latin: noun use of feminine of Latin novusnew

OTHER WORDS FROM nova

no·va·like, adjective

Words nearby nova

Nouvelle-Calédonie, nouvelle cuisine, nouvelles, nouvelle vague, nov., nova, Novachord, novaculite, Nova Iguaçu, Novalis, Nova Lisboa

Definition for nova (2 of 2)

Nova
[ noh-vuh ]
/ ˈnoʊ və /

noun

Also called Nova Salmon. a Pacific salmon cured in the style of Nova Scotia salmon.
(lowercase) (loosely) any smoked salmon.
Compare Nova Scotia salmon.
Dictionary.com UnabridgedBased on the Random House Unabridged Dictionary, © Random House, Inc. 2020

Example sentences from the Web for nova

British Dictionary definitions for nova

nova
/ (ˈnəʊvə) /

noun plural -vae (-viː) or -vas

a variable star that undergoes a cataclysmic eruption, observed as a sudden large increase in brightness with a subsequent decline over months or years; it is a close binary system with one component a white dwarfCompare supernova

Word Origin for nova

C19: New Latin nova (stella) new (star), from Latin novus new
Collins English Dictionary - Complete & Unabridged 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

Cultural definitions for nova

nova
[ (noh-vuh) ]

In astronomy, the appearance of a new star in the sky (nova is Latin for “new”). Novae are usually associated with the last stages in the life of a star. (See supernova.)

The New Dictionary of Cultural Literacy, Third Edition Copyright © 2005 by Houghton Mifflin Harcourt Publishing Company. Published by Houghton Mifflin Harcourt Publishing Company. All rights reserved.

Scientific definitions for nova

nova
[ nōvə ]

Plural novae () novas

A white dwarf star that suddenly and temporarily becomes extremely bright as a result of the explosion at its surface of material accreted from an expanding companion star. The material, mostly hydrogen and helium, is attracted by the white dwarf's gravity and accumulates under growing pressure and heat until nuclear fusion is ignited. Unlike a supernova, a nova is not blown apart by the explosion and gradually returns to its original brightness over a period of weeks to years. Because of their sudden appearance where no star had been previously visible, novae were long thought to be new stars. Since 1925, novae have been classified as variable stars. Compare supernova.
The American Heritage® Science Dictionary Copyright © 2011. Published by Houghton Mifflin Harcourt Publishing Company. All rights reserved.
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更新时间:2024/11/14 6:32:04