Views : 6,394,449
Genre: Education
Date of upload: Nov 15, 2022 ^^
Rating : 4.958 (2,140/199,845 LTDR)
RYD date created : 2024-05-03T09:30:42.642928Z
See in json
Top Comments of this video!! :3
I was surprised a few years ago to learn that gold and heavier elements are unlikely to be created in a standard supernova but require a more extreme ultranova or similar event such as star collisions to produce special elements like gold. That just adds to how lucky we are to have such abundance of uranium, gold, etc on our planet.
337 |
i’m extremely proud of the way my dad explained supernovae to me when i was about 5. he told me to put my hands out, facing each other, and then he put his hands on mine. he then told me to push outwards, as hard as i can, while he pushed inwards, which made my hands collapse. he said that when a star wasn’t strong enough anymore then gravity won.
now that i’m older, i’m really enjoying this more comprehensive explanation
2.7K |
Whenever I watch an almost 20 minute long Veritasium video, I never lose interest throughout the video and it's consistently gets my attention. The pacing of him talking quickly and pausing to make a transition makes it easier to retain the information. Also his voice is very clear and comprehensible. As always amazing stuff Veritasium, you never fail to get my attention.
1.2K |
I'm an undergraduate student majoring in Astrophysics and Planetary Geology. Thank you SO much for this video and your sources, one of my professors was looking into an extinction event and I was curious as well. This has given me a starting place on research to piece things together! While I was pondering on possibilities I remembered this video. Veritasium, you are doing an amazing job with your channel. I have sent many of your videos to friends to help explain concepts, they always love your content too!
4 |
Last year, I almost joined the Brian fields research group after listening to his presentation on this topic. He talked about how they had to look through sediment samples to find traces of Fe-60. I thought it was so cool that we could learn so much about the history of our cosmic neighbourhood just by observing earth. It's amazing to see this topic explained so well.
719 |
It took me a moment to fully understand just how much of a difference the density changed when going from an iron core with a diameter of 3000km down to a neutron star with a diameter of 30km. At first I thought "hmm, 100x smaller is quite a bit smaller, but doesn't seem like enough for how insanely dense a neutron star is". Then I remembered that volume is affected by a square compared to the diameter. So, even though the core "only" goes from 3000km to 30km, the volume is about 1,000,000x smaller. Thats some DENSE matter. Especially when you consider the fact that iron is already relatively dense, that's absolutely insane.
20 |
Small addendum regarding the name Supernova that you mention (1:20):
Kepler's teacher and mentor, Tycho Brahe, was the first to publish a book concerning a new star (stella nova), namely SN1572 or "Tycho's Supernova", which appeared 32 years earlier (TWO visible supernovae in a lifetime and NONE since!)
Brahe's book was "De nova et nullius aevi memoria prius visa stella", ("Concerning the Star, new and never before seen in the life or memory of anyone").
190 |
@brunosimoes6405
1 year ago
I've already seen dozens of videos on Youtube about how a Supernova works, but this is another level. A complete and very well illustrated lesson in under 20 minutes. Veritasium never disappoints.
11K |