Nova
id:
nova-181-5836218
title:
Nova
text:
A nova is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star that slowly fades over weeks or months. All observed novae involve white dwarfs in close binary systems, but causes of the dramatic appearance of a nova vary, depending on the circumstances of the two progenitor stars. The main sub-classes of novae are classical novae, recurrent novae (RNe), and dwarf novae. They are all considered to be cataclysmic variable stars. Classical nova eruptio
brand slug:
wiki
category slug:
encyclopedia
description:
Nuclear explosion in a white dwarf star
original url:
https://en.wikipedia.org/wiki/Nova
date created:
2001-10-16T00:30:10Z
date modified:
2024-09-05T22:00:56Z
main entity:
{"identifier":"Q6458","url":"https://www.wikidata.org/entity/Q6458"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/5/5d/Making_a_Nova.jpg","width":250,"height":169}
fields total:
13
integrity:
16