This is a supernova from hundreds of years ago |
Monday, 19 August 2013
Star classification
So yesterday, we went a bit into star classification but there is more to it.
So the smallest star is a red colour and goes as low as 2,500 kelvin and is M class. Next is K and it is a orange colour star and goes up to 5,200 kelvin, then G, which is what our sun is. G stars are yellow and temperatures can go as high as 6000 kelvin, then F stars which are a white-yellow colour and temperatures can be as hot as 7,500 kelvin, following that are the A class stars which are white in colour. They can be extremely hot at 10,000 kelvin. Second to last is B, they are white-blue and can reach 33,000 kelvin in temperatures. Finally is class O which is blue and can go over 60,000 kelvin.
So they're the main classes, but there are sub- classes as well. They contain numbers ranging from 0-9 and roman numerals from I to V. The numbers are in tenths to the next star class. The Roman Numerals measure the size of the star which shows how much light it gives out.
So the smallest star is a red colour and goes as low as 2,500 kelvin and is M class. Next is K and it is a orange colour star and goes up to 5,200 kelvin, then G, which is what our sun is. G stars are yellow and temperatures can go as high as 6000 kelvin, then F stars which are a white-yellow colour and temperatures can be as hot as 7,500 kelvin, following that are the A class stars which are white in colour. They can be extremely hot at 10,000 kelvin. Second to last is B, they are white-blue and can reach 33,000 kelvin in temperatures. Finally is class O which is blue and can go over 60,000 kelvin.
So they're the main classes, but there are sub- classes as well. They contain numbers ranging from 0-9 and roman numerals from I to V. The numbers are in tenths to the next star class. The Roman Numerals measure the size of the star which shows how much light it gives out.
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