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O Class stars have the following characteristics.

  • Temperature: > 30,000 Kelvin
  • Colour: Blue
  • Mass: > 16 Solar masses
  • Radius: >6.6 Solar radius
  • Luminosity: > 30,000 Solar luminosities.
  • Rarity: 0.00003% of all main sequence stars.
Example: Zeta Orionis

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How hot are O stars?

Class O stars are the hottest of stars with temperatures greater than 30,000oK


What does the spectral class letters mean?

The spectral class letters in astronomy represent the temperature and color of stars. The sequence starts with O (hottest and bluest stars) and ends with M (coolest and reddest stars). The spectral class letters are O, B, A, F, G, K, and M.


Of the spectral classes the highest temperature class is designated as what?

The O spectral class is the highest temperature class. Stars in this class are extremely hot and blue in color, with surface temperatures exceeding 30,000 K.


What class of stars are the largest?

The largest class of stars are known as hypergiants. These massive stars have very high luminosities and can be hundreds of times bigger than the Sun. Examples include stars like UY Scuti and Betelgeuse.


What spectral class is the hottest star under?

O. This is the class of the blue/white giants.


What is spectral class?

Spectral class is a classification system for stars based on their temperature and spectral characteristics. It categorizes stars into different groups, such as O, B, A, F, G, K, and M, with O being the hottest and M being the coolest. Spectral class is indicated by a letter, with additional subtype information denoted by a number.


What are B class stars?

B Class stars have the following characteristics.Temperature: 10,000 -> 30,000 KelvinColour: Blue -> Blue-whiteMass: 2.1 -> 16 Solar massesRadius: 1.8 -> 6.6 Solar radiusLuminosity: 25 -> 30,000 Solar luminosities.Rarity: 0.13% of all main sequence stars.Examples: RigelSee related link for more information.


What are F class stars?

F Class stars have the following characteristics.Temperature: 6,000 -> 7,500 KelvinColour: Yellow-white -> WhiteMass: 1.04 -> 1.4 Solar massesRadius: 1.15 -> 1.4 Solar radiusLuminosity: 1.5 -> 5 Solar luminosities.Rarity: 3% of all main sequence stars.Examples: CanopusSee related link for more information.


What spectral class of stars are the hotteset?

Type-O are the hottest but there are very few. Then type-B, there are more of them but still not a lot. Then you have type-A, which are very common, then F, then G like the Sun, then K and then the coolest common ones, type M which are the red stars like Betelgeuse.


How are stars classified description?

There are several ways that Stars get classified. The first is by spectrum, this was used early on in astronomy as astronomers did not have the equipment we have today. Basically they measure the visual spectrum of light that the stars give off to Earth. The second method is using the letter system O B A F G K M. O being the hottest and M the coolest. O class stars contain helium, B class stars have hydrogen and helium, A class stars hydrogen and ionized metals, F class Stars hydrogen, ionized calcium, and iron, G class Stars (like our sun) calcium and ionized metals, k class stars neutral metals and sodium and M class Stars sodium and titanium oxide. The third method is by is by temperature. They measure the heat it gives off and the amount that is absorbed by the materials around the star these are called absorption lines. This helps to determine what letter to give a Star. The fourth is by colour. The the visual colour the star appears in the sky is not enough to just say its red or blue so they other measurements like infrared and other kinds of invisible light spectrum's. And finally the elements that surround a star also differentiates what light is reflected back to earth. You combine all these methods together and you get how stars a classified.


Why are there no massive O and B stars?

Massive O and B stars have shorter lifespans due to their high rate of fusion and energy output, leading to a faster depletion of their nuclear fuel. As a result, they are relatively short-lived compared to lower mass stars. Additionally, massive stars have strong stellar winds and are more prone to exploding as supernovae, further limiting their presence in the universe.


Why are o and b main sequence stars rare?

O and B main sequence stars are rare because they are massive stars with short lifespans compared to smaller stars like the Sun. Their high mass causes them to burn through their nuclear fuel at a faster rate, leading to a shorter main sequence lifetime. This means that O and B stars are less common in the overall population of stars because they exist for a shorter period of time.