What is the difference between supernovae and nova?

Definitions

- Referring to a massive explosion of a star that results in a sudden increase in brightness. - Describing a celestial event that occurs at the end of a star's life cycle. - Talking about a rare and spectacular astronomical phenomenon that can be observed from Earth.

- Describing a sudden increase in brightness of a star that lasts for a period of time. - Referring to a celestial event that occurs when a white dwarf star accumulates material from a companion star. - Talking about a relatively common astronomical phenomenon that can be observed from Earth.

List of Similarities

  • 1Both are astronomical events that involve stars.
  • 2Both result in a sudden increase in brightness that can be observed from Earth.
  • 3Both occur at the end of a star's life cycle.
  • 4Both are relatively rare and spectacular events.

What is the difference?

  • 1Magnitude: Supernovae are much brighter than novae and can outshine entire galaxies.
  • 2Cause: Novae occur when a white dwarf star accumulates material from a companion star, while supernovae occur when a star runs out of fuel and collapses.
  • 3Duration: Novae typically last for a few weeks, while supernovae can remain visible for months or even years.
  • 4Frequency: Novae are relatively common and occur several times a year, while supernovae are much rarer and occur only a few times per century.
  • 5Consequence: Supernovae can leave behind a remnant such as a neutron star or black hole, while novae do not have such a consequence.
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Remember this!

Supernovae and novae are both astronomical events that involve stars and result in a sudden increase in brightness that can be observed from Earth. However, the difference between them lies in their magnitude, cause, duration, frequency, and consequence. Supernovae are much brighter and rarer than novae, and they occur when a star runs out of fuel and collapses, leaving behind a remnant such as a neutron star or black hole. On the other hand, novae are relatively common and occur when a white dwarf star accumulates material from a companion star.

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