E.5.2 State the effect of a star's mass on the end product of nuclear fusion.
{"Image DocumentName": "E.5.2 State the effect of a star\u2019s mass on the end product of nuclear fusion.", "Image ImageDescription": "At the end of a star\u2019s lifetime as a main sequence star all the H in its core has been used up. How long this takes and a star\u2019s ultimate fate depends upon its initial mass. The Sun will convert H into He for 5x109 years but a star of mass 25M\uf0a4 will take only about 106 years to use up all its H.", "Image XResolution": "37", "Image YResolution": "37", "Image ResolutionUnit": "Pixels/Centimeter", "Image Software": "SlidePlayer", "Image YCbCrPositioning": "Centered"}