Editing 2070: Trig Identities

Jump to: navigation, search

Warning: You are not logged in. Your IP address will be publicly visible if you make any edits. If you log in or create an account, your edits will be attributed to your username, along with other benefits.

The edit can be undone. Please check the comparison below to verify that this is what you want to do, and then save the changes below to finish undoing the edit.
Latest revision Your text
Line 27: Line 27:
 
===From physics (and beyond)===
 
===From physics (and beyond)===
 
The formula s=1/2 a&#8203;t² gives the distance a uniform accelerating object reaches over time. The second formula belongs to astronomy and the {{w|Kepler's laws of planetary motion#Third law of Kepler|third law of Kepler}} in which ''the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit'', meaning the fraction of b<sup>3</sup> and t<sup>2</sup> is a constant (banana).
 
The formula s=1/2 a&#8203;t² gives the distance a uniform accelerating object reaches over time. The second formula belongs to astronomy and the {{w|Kepler's laws of planetary motion#Third law of Kepler|third law of Kepler}} in which ''the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit'', meaning the fraction of b<sup>3</sup> and t<sup>2</sup> is a constant (banana).
 
But using the angle ''θ'' as an argument leads to {{w|Richard Feynman}}, who did many famous ''{{w|The Feynman Lectures on Physics|Lectures on Physics}}''  and his lost lecture about the ''{{w|Feynman's Lost Lecture|Motion of Planets Around the Sun}}'' from 1964 in which he only used geometry, based on the orbital ellipse, a circle around, and matching right-angled triangles to illustrate this law from Kepler. For deeper understanding why it really does work there is a nice presentation at the "Journal of Symbolic Geometry": [http://ceadserv1.nku.edu/longa/classes/calculus_resources/docs/kep.pdf Feynman Says: “Newton implies Kepler, No Calculus Needed! (Brian Beckman, 2006)”]
 
  
 
===Proof of algebraic mistakes in the comic===
 
===Proof of algebraic mistakes in the comic===

Please note that all contributions to explain xkcd may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see explain xkcd:Copyrights for details). Do not submit copyrighted work without permission!

To protect the wiki against automated edit spam, we kindly ask you to solve the following CAPTCHA:

Cancel | Editing help (opens in new window)