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Hot, blue stars appear brighter through the blue filter, while the opposite is true for cooler, red stars.
For starters, a planet orbiting a hot blue-white star will not have the same reflectance characteristics as a planet orbiting a cooler red dwarf.
As new star formation has declined and the population of aging, cooler red stars is proportionally much larger, the universe has moved into a middle green period.
Eventually, when all of the free gas is turned into stars, after many generations, only stars that can live for really long periods of time will survive, and so galaxies with lots of young, hot, blue stars will eventually turn into galaxies with lots of old, cooler, red stars.
The cooler red will be more pulled together, the alcohol subdued, the flavors miraculously zoomed into focus.
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The Chandra image shows the outer blast wave produced by the supernova (blue), and an inner ring of cooler (red-orange) material.
The Chandra data shows an outer blast wave produced by the supernova (blue) and an inner ring of cooler (red-orange) material.
The plants don't need it, preferring cooler reds and blues.
By the time tens of billions of additional years have gone by, only the cooler, redder stars will remain.
Without new stars forming, the more massive, bluer ones simply end their lives when they run out of fuel, leaving the cooler, redder stars as the only survivors.
TRAPPIST-1, named for the telescope that was used to discover the three exoplanets, is a star that is much cooler, redder, and smaller than the Sun.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com