PokeVideoPlayer v23.9-app.js-020924_
0143ab93_videojs8_1563605 licensed under gpl3-or-later
Views : 94,985
Genre: Education
Uploaded At Feb 3, 2023 ^^
warning: returnyoutubedislikes may not be accurate, this is just an estiment ehe :3
Rating : 4.848 (184/4,666 LTDR)
96.21% of the users lieked the video!!
3.79% of the users dislieked the video!!
User score: 94.31- Overwhelmingly Positive
RYD date created : 2024-07-01T16:37:39.955951Z
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Top Comments of this video!! :3
If we take the centripetal force mv^2/r and equal it to GMm/r^2 approximately (assuming all other forces are negligible) you will see that GM/r=v^2, where G is the universal gravitational constant, and M is the mass of the Sun, which is basically constant. As you get closer to the Sun, your radius (r) gets smaller. Since r is on the denominator, decreasing r increases the value of the fraction. Therefore v^2 is greater if r is reduced, so v is greater when r is reduced. There’s your explanation that I think is correct, feel free to correct me if I’m wrong :) I would also like to add that if the Sun were to disappear, gravitational waves would only travel at the speed of light. So it would take 8 and a half minutes before the Earth gets catapulted whereas Neptune, for example, would take around 4 hours before it becomes ejected.
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@kayzeaza
1 year ago
“Alright gang, let’s split up!”
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