Timeline for Integrating acceleration + escape velocity over distance [closed]
Current License: CC BY-SA 4.0
11 events
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Jun 20 at 11:34 | history | closed |
John Rennie anna v naturallyInconsistent |
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Jun 20 at 10:25 | answer | added | Ralf Kleberhoff | timeline score: 1 | |
Jun 20 at 9:31 | comment | added | PM 2Ring | Your object can escape Earth, but it doesn't have enough orbital energy to escape the Sun. | |
Jun 20 at 9:22 | comment | added | PM 2Ring | This may be helpful: en.wikipedia.org/wiki/Hyperbolic_trajectory | |
Jun 20 at 9:16 | review | Close votes | |||
Jun 20 at 11:37 | |||||
Jun 20 at 8:53 | history | edited | John Rennie |
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Jun 20 at 8:52 | comment | added | John Rennie | Use conservation of energy i.e. KE + PE = constant | |
Jun 20 at 8:31 | history | edited | uggupuggu | CC BY-SA 4.0 |
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Jun 20 at 8:30 | comment | added | Y Z | I don't think there is a "ds" in the expression of acceleration. | |
Jun 20 at 8:29 | history | edited | Qmechanic♦ |
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Jun 20 at 8:18 | history | asked | uggupuggu | CC BY-SA 4.0 |