Views : 1,536,806
Genre: Education
Date of upload: Apr 16, 2015 ^^
Rating : 4.932 (321/18,652 LTDR)
RYD date created : 2022-04-03T17:21:09.5322Z
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Top Comments of this video!! :3
It took me a while to understand from 5:08 to 5:30. I'll break it up for the one's who are facing the same problem as I did.
1) At Aphelion, Mercury's angular rotational speed is faster than it's angular orbital speed, so the Sun moves rapidly to the west side in the sky.
2) Four days before Perihelion, the angular orbital velocity of Mercury is equal to the angular rotational velocity, so the Sun appears to stop in the sky.
3) While now at Perihelion, the angular orbital velocity of Mercury is more than the angular rotational velocity, so the Sun appears to move eastwards.
4) Now as the Mercury is pulled away from the Sun i.e. it leaves it Perihelion position, again it moves westwards as the angular rotational velocity dominates over the angular orbital velocity.
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This video actually corrected a misconception that I had about Mercury. I remember reading that Mercury was tidally locked in the same way that the Moon was so that its year was the same as its day. I always believed that Mercury had a permanent light side and dark side, and that the light side was always really hot and the dark side was extremely cold. I think I got this impression from a children's book I had while growing up which might have been using out of date information.
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Little bonus fact, even though it is the closest planet to the sun, Venus is hotter, this is because the atmosphere on Venus keeps the heat in.
Because Mercury has almost no atmosphere to retain heat, Mercury's surface experiences the greatest temperature variation of the planets in the Solar System, ranging from 100 K (−173 °C; −280 °F) at night to 700 K (427 °C; 800 °F) during the day at some equatorial regions.
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This video told me a lot about Mercury that I didn't know, but it didn't answer the question I had - about the anomaly of Mercury's orbit that had to be explained through Relativity. I have looked in other places, where the anomaly seems to be its precession - but I don't think relativity is needed to explain that. I'm guessing that when precession is taken into account, the orbit is still not exactly what it is expected to be. The answer must be out there somewhere - but the Internet is a big place!
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@Zerepzerreitug
9 years ago
Also, I say we adopt the phrase "I had a Mercury's day" to describe a day when it feels as if everything was chaotic and the end of your day never seemed to arrive.
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