Nova (astronomy)/Related Articles: Difference between revisions
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==Other related topics== | ==Other related topics== | ||
* [[Supernova]] | * [[Supernova]]e are exhibiting similar brightness increases but are much brighter. They are also triggered by an unrelated physical mechanism. | ||
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Revision as of 04:21, 19 July 2010
- See also changes related to Nova (astronomy), or pages that link to Nova (astronomy) or to this page or whose text contains "Nova (astronomy)".
Parent topics
- Cataclysmic variable, novae belong to the class of cataclysmic variable stars.
Subtopics
- Supernovae are exhibiting similar brightness increases but are much brighter. They are also triggered by an unrelated physical mechanism.
Bot-suggested topics
Auto-populated based on Special:WhatLinksHere/Nova (astronomy). Needs checking by a human.
- Helium [r]: A chemical element, having the chemical symbol He, and atomic number (the number of protons) 2. [e]
- Iron [r]: An important transition metal and chemical element with the symbol Fe (Latin: ferrum) and atomic number 26. [e]
- Star [r]: A massive, luminous ball of plasma that is held together by gravity. [e]
- Sun [r]: The star that defines our solar system. [e]