4.3 • 1.4K Ratings
🗓️ 16 June 2023
⏱️ 5 minutes
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0:00.0 | Hi, and welcome to Cosmos Quickly. |
0:07.8 | This is Lee Billings. |
0:08.8 | And this is Karen Leone. |
0:13.0 | Karen, thanks so much for being here. |
0:15.5 | A quick question for you. |
0:17.1 | What's super duper bright and hundreds, or even thousands of times heavier than our |
0:21.2 | entire solar system, yet it's so hard to find that it has yet to be directly seen? |
0:28.0 | Hmm. |
0:29.0 | It's not a good riddle. |
0:30.5 | The answer, though, is a population-three star. |
0:33.5 | That's a astronomer-lingo for the very first stars in the universe, which formed from |
0:37.6 | dense clouds of pristine hydrogen and helium that filled the cosmos in the first few hundred |
0:41.9 | million years after the Big Bang. |
0:44.1 | Those conditions should have allowed population-three stars to bulk up to proportions impossible |
0:48.7 | for more chemically enriched modern-day stars to achieve. |
0:52.0 | Great. |
0:53.0 | Okay. |
0:54.0 | And these massive stars were also foundational for everything else we see in the |
0:57.1 | universe today, right? |
0:58.3 | So they were important cosmic ingredients that set the table for the evolution of things |
1:03.5 | like galaxies and black holes, other types of stars, planets, and of course us. |
1:09.4 | Right. |
... |
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