In this video, the stars in globular cluster Omega Centauri are rearranged according to their intrinsic brightness (vertical axis) and their temperature (horizontal axis). The temperature of a star dictates its apparent colour, with cooler stars being red and hotter ones being blue. The majority of stars at any given time fall into a wide band known as the main sequence, which passes from the top left (hot, bright stars) to the bottom right (cool, dim stars). However this is just a snapshot in time — as stars evolve they do not stay fixed to one point on the diagram for the whole of their lives.
Credit:
NASA, ESA, J. Anderson and R. van der Marel (STScI)
very pretty :)
andreirocks1992 1 month ago
so cool
CaptainplanetPHD 4 months ago
perfetto
Ilgulliverblue 6 months ago
this is great for science class
bobwasherenotthere 1 year ago