Novae are more closely related to Type II than to Type I supernovae.

Name: Novae are more closely related to Type II than to Type I supernovae.
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Novae involve a white dwarf in a binary system accreting material from its companion star, leading to a thermonuclear explosion on its surface, whereas Type I and Type II supernovae are both catastrophic explosions of stars, with Type I lacking hydrogen lines and Type II showing them, indicating different progenitor systems and mechanisms.

Novae Are More Closely Related to Type II Than to Type