You realize you are using the right document editor when such a simple task as Diagram age bulletin does not take more time than it should. Editing files is now a part of a lot of working operations in different professional fields, which is the reason accessibility and straightforwardness are crucial for editing instruments. If you find yourself researching manuals or looking for tips about how to Diagram age bulletin, you might want to find a more intuitive solution to save your time on theoretical learning. And this is where DocHub shines. No training is needed. Simply open the editor, which will guide you through its principal functions and features.
A workflow gets smoother with DocHub. Make use of this instrument to complete the documents you need in short time and get your productivity to a higher level!
so the sun starts helium burning as it starts the helium burning process it settles down becomes a horizontal branch star its not really stable at this point its still evolving its still moving across the hr diagram back towards the main sequence and so its still heading back towards the main sequence but the thing is we also know the lifetime of a star on the main sequence depends on the mass of the star so wed already given this equation earlier saying that the main sequence lifetime can be approximated by that equation at least for stars that are within a reasonable range for super high mass stars this equation doesnt work and for really low mass stars this equation doesnt work but for in between this equation works pretty good and so its a pretty good approximation lets so we can look at a star cluster and this is the hr diagram of a very old star cluster and remember the main sequence would look something kind of like that okay so whats happened is that the stars that w
