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awesome vid as always 👍👍 i like how the systems looking, though when it comes to gas giants, refer to the sudarsky gas giant classification system its basically a system which predicts the colour and albedo of gas giants from their temperature, and these are the 5 classes: class 1: these have ammonia clouds, and temperatures below about -120 celsius, basically like jupiter and saturn. the predicted albedos are about the same as jupiter and saturn, so ~0.5. class 2: these have water clouds, and are above -23 celsius. they appear grey and white, and have high albedos of between 0.6 and 0.7. if you have a superjupiter however, pressures are high enough to turn them into a class 2, even if they should be a class 1. class 3: these are cloudless, and appear azure blue in a similar fashion to uranus or neptune. they also appear at above 80 celsius. low albedos of about ~0.12 class 4: these are dominated by alkali metals, and appear dark blue. they appear at temperatures above 630 celsius. these have low albedos, about ~0.03. class 5: these have silicate clouds, with temperatures above 1100 celsius. even though you wouldnt see their colour at this point, theyd probably have black and maybe white or grey bands. these have high albedos, about ~0.55 hope this helps for future reference
Imagine what happens when Eta Carinae goes supernova 😅 Those humongous stars are at center of galaxy area, and have a lifetime of a few million years or less, compared to our sun at 12+ billion years, so life wouldn’t even have a CHANCE to develop 😭
