Astronomy - Measuring Distance, Size, and Luminosity (8 of 30) Distance to Our Planets

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In this video I will use Keppler's 3rd law to find the distances to our planets.
  1. Michel van Biezen
  2. lectureonline
  3. ilectureonline.com
  4. Mike
  5. Mike van Biezen
  6. van Biezen
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Комментарии
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The best history field is certainly the history of astronomy. Thanks Sir that you cover these underrated topics.

-ne
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The BEST series on you tube concise and informative

gowdsake
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Your lectures are very helpful for astronomy olympiad. Thank you sir.

gauravsinha
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Where did the equation D3 = p2 come from?

dajavuja
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I guess this could be one opponent idea for excluding Pluto as a planet. am i right? does it work for Pluto now or maybe a long time ago even Pluto was in proper rotation and worked in the equation but not now.

-ne
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It looks like circular argument. How can Newton state his 3. law when he don't know any distance of one planet to the sun.
In the past videos you showed only distance of earth between moon. And the distance of sun between earth (very inaccurate). To state the law he need at least 2 distances but you showed only one. Even with 2 distances this would only be a guess.

Stefan
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Suryasiddhanta was written in India thousands of years before Kepler. It is an extensive work on Solar system in Sanskrit. But somehow only western scholars get all the credit. Look how blatantly they lied about calculus being developed by Newton.

AbhinavChauhan