Alright here’s the next question:
Explain the effectiveness of the Morgan-Keenan system in stellar classification. (4 marks)
This question seems a bit difficult to answer, but I will give it my best shot (Im assuming Morgan-Keenan refers to stellar spectral classes divided by temperature?) I would assume that you say:
-The Morgan Keenan system is extremely effective at separating stars into spectral classes based off of temperature. It allows for a separation by the colour for the star as well, since Wien's Law states that the peak wavelength is inverselvely proportional to the temperature of the star.
-When plotted on the HR diagram, the relative position of a star in the main sequence can also be determined. This allows for a determination of its absolute magnitude, which is related to luminosity and surface area, as well as the expected lifetime of the star and the predominant nuclear fusion reactions (p-p chain in smaller main sequence stars as opposed to CNO in larger main sequence). The position of a star in the main sequence can also be used to predict the formation of a black hole or neutron star in the stars future.
-Post main sequence stars can also be classified based on their colour and temperature, i.e. the position of red giants and white dwarfs. The sub classes help determine whether stars in these red and white regions are either main sequence stars or red giants/white dwarf due to their relative sizes. These also allow for a comparison of luminosities of stars, usually compared to the luminosity of our sun in practice.
Thats what i did but i didnt get 701.9 nm, rather 707.1 i believe
Yeah theres also a typo in the marking guidelines (This is fron the TEC exam). Instead of saying d*sin45 they say d+sin45. Really badly designed question lol.