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Cosmology - The End of the Universe OPENING QUESTIONS: *Without* checking your notes: Work with your team to make a quick list of item/instances/questions/interesting bits that are still kicking around in your brain from yesterday's reading! OBJECTIVE: I will be able to relate three "Big Freeze" timeline milestones of the very distant future after today's class. OBJECTIVE: The team says Yay WORDS FOR TODAY:
WORK O' THE DAY: Let's review our (Revised) Big Bang timeline -- there are 6 items now instead of 7 ═══════════════════════════ Here are a couple of new terms that will help before we watch this video: Red Dwarf stars: We talked about them yesterday. Those are very small stars (roughly 5 - 10 times the size of the Earth) that can (and will!) live for trillions of years!!! White Dwarf stars: Aren't stars at all. They are the core of stars like the sun. They don't 'mash' atoms anymore. They just sit there like coals in a barbeque-- slowing giving off heat for dozens or maybe even hundreds of billions of years! Black Dwarf stars: A white dwarf star that has given off ALL of it's heat. Just a chunk of iron floating in space Neutron stars: Wannabe black holes that that were born from exploded stars that just never got big and bad enough to become black holes. ═══════════════════════════ One of my student's last year shared THIS absolutely incredible video that helps visualize some of what that article discusses. It's a bit long but well worth the time. What we don't finish now we'll view tomorrow. |