Astronomy
As I said before a Nova is a completely different process compared with a Supernova. A Nova is actually a sudden brightness that spreads across the surface of a White dwarf--kind of a star. The brightness is the result of a fusion reaction that happens on the surface of the White dwarf, and that fusion reaction is initiated by the matter that was gravitated towards and got accumulated across the surface of the White dwarf from a nearby binary neighbor.
This doesn't cause any sort of huge impact on the White dwarf's dimensions or properties, and hence can happen again and again as long as its neighbor stays close enough, and the matter gets accumulated on its surface.
Supernova on the other hand is a complete destruction of a star that which can't able to withstand its own gravity, when it happens to reach a certain mass at the end of its fuel consumption. The limit being found as 1.4 solar masses by Chandrashekar and was popular as Chandrashekar Limit.
Obviously it happens just once for a star that supposedly reaches above or equals Chandrashekar Limit, after burning away its complete fuel, unlike Nova.
Supernova got classified in to two types depending up on the way it reaches the Chandrashekar Limit.
Earlier it was thought that the Supernova is a kind of bigger and brighter Nova and hence the name. And now, the name stayed but not the definition. A Supernova is in noway related to Nova where the former is caused by the gravitational collapse and the later by the fusion reaction.
The only thing that appears common for the both at times is White dwarf.
- New Candidate For Coldest Known Star May Help Blur The Distinction Between A Star And A Planet
An artist?s impression of the CFBDSIR 1458+10 star system. The star in the background is the candidate for the coldest known star. Image: ESO/L. CalçadaThere may be a new candidate for the coldest known star, an object classified as a brown dwarf with...
- White Dwarfs As Pulsars
A little more than two years ago, in early 2008, there was a shocking discovery from the Suzaku team. Suzaku is an orbiting X-ray observatory, operated jointly by JAXA and NASA. It had detected a white dwarf star, AE Aquarii, emit high-energy X-ray pulses....
- Supernova Smashed Into A Nearby Star
A team of astronomers has witnessed a supernova smashing into a nearby star, shocking it and creating an ultraviolet glow that reveals the size of the companion. In a type "Ia" supernova, a white dwarf star explodes after it gains matter from a companion...
- What Is A White Dwarf?
A white dwarf is a dwarf star and the 'white' that was added to its name was just because, the few dwarfs that were found during their discovery appeared white--I'm not kidding, that's true. Do you know how dense a typical white dwarf...
- What Is A Nova?
A Nova is not a new star that appears all of a sudden in the sky, as its name suggests. It's actually a sudden brightness that appears on the surface of an existing white dwarf star in a binary system with another star. The White dwarf star's...
Astronomy
Difference between Nova and Supernova
As I said before a Nova is a completely different process compared with a Supernova. A Nova is actually a sudden brightness that spreads across the surface of a White dwarf--kind of a star. The brightness is the result of a fusion reaction that happens on the surface of the White dwarf, and that fusion reaction is initiated by the matter that was gravitated towards and got accumulated across the surface of the White dwarf from a nearby binary neighbor.
This doesn't cause any sort of huge impact on the White dwarf's dimensions or properties, and hence can happen again and again as long as its neighbor stays close enough, and the matter gets accumulated on its surface.
Supernova on the other hand is a complete destruction of a star that which can't able to withstand its own gravity, when it happens to reach a certain mass at the end of its fuel consumption. The limit being found as 1.4 solar masses by Chandrashekar and was popular as Chandrashekar Limit.
Obviously it happens just once for a star that supposedly reaches above or equals Chandrashekar Limit, after burning away its complete fuel, unlike Nova.
Supernova got classified in to two types depending up on the way it reaches the Chandrashekar Limit.
- The first one, as I mentioned earlier happens when a star can't burn anymore and endup above or across Chandrashekar Limit. This is more natural as it seems.
- The second one happens for a White dwarf, where its resultant mass reaches the 'Limit' through accretion of mass from its nearby binary neighbor. It might look like Nova in the beginning but is more powerful and more devastating, as there will be no star left over--other than some Supernova Remnant--at the end of the process that lasts ranging from several weeks to months.
Earlier it was thought that the Supernova is a kind of bigger and brighter Nova and hence the name. And now, the name stayed but not the definition. A Supernova is in noway related to Nova where the former is caused by the gravitational collapse and the later by the fusion reaction.
The only thing that appears common for the both at times is White dwarf.
- New Candidate For Coldest Known Star May Help Blur The Distinction Between A Star And A Planet
An artist?s impression of the CFBDSIR 1458+10 star system. The star in the background is the candidate for the coldest known star. Image: ESO/L. CalçadaThere may be a new candidate for the coldest known star, an object classified as a brown dwarf with...
- White Dwarfs As Pulsars
A little more than two years ago, in early 2008, there was a shocking discovery from the Suzaku team. Suzaku is an orbiting X-ray observatory, operated jointly by JAXA and NASA. It had detected a white dwarf star, AE Aquarii, emit high-energy X-ray pulses....
- Supernova Smashed Into A Nearby Star
A team of astronomers has witnessed a supernova smashing into a nearby star, shocking it and creating an ultraviolet glow that reveals the size of the companion. In a type "Ia" supernova, a white dwarf star explodes after it gains matter from a companion...
- What Is A White Dwarf?
A white dwarf is a dwarf star and the 'white' that was added to its name was just because, the few dwarfs that were found during their discovery appeared white--I'm not kidding, that's true. Do you know how dense a typical white dwarf...
- What Is A Nova?
A Nova is not a new star that appears all of a sudden in the sky, as its name suggests. It's actually a sudden brightness that appears on the surface of an existing white dwarf star in a binary system with another star. The White dwarf star's...