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hey guys miss Gosling here in this video were going to talk about the main sequence by the end of the video youll be able to quantify the relationship between mass and Luminosity for main sequence Stars so lets go ahead and get started so lets go ahead and start by taking a look at your IB understandings applications and skills so you need to understand the massive monocity relationship for main sequence stars and you need to be able to apply the mass Luminosity relation for main sequence Stars so lets go ahead and get started so as youll remember in the main sequence is this stripe of stars that are going from the top left corner of the HR diagram down diagonally to the bottom right corner this is where my stars that are young so my stars that are still fusing hydrogen into helium are located on my HR diagram so the way that the mass Luminosity relationship is typically written is that the Luminosity of a given star divided by the Luminosity of the sun is equal to the mass of th