Skip to main content
12 events
when toggle format what by license comment
Apr 13, 2017 at 12:40 history edited CommunityBot
replaced http://physics.stackexchange.com/ with https://physics.stackexchange.com/
Jan 23, 2012 at 10:14 comment added voix Look at The Time That 2 Massess Will Collide Due To Gravity. The resulting formula is pretty nice, for $M>>m$, $\large \bf{T= \frac{\pi}{2} \frac{h}{v_e}}$, where $\large v_e$ - escape velocity, $\large v_e = \sqrt{\frac{2GM}{h}}$
Jan 23, 2012 at 9:13 history edited CommunityBot
insert duplicate link
Jan 23, 2012 at 9:13 history closed Qmechanic
David Z
exact duplicate
Jan 23, 2012 at 9:03 answer added twistor59 timeline score: 1
Jan 23, 2012 at 8:52 answer added Maksim Zholudev timeline score: 1
Jan 23, 2012 at 8:34 comment added John Rennie Have a look at physics.stackexchange.com/questions/19813/… as this describes a similar calculation.
Jan 23, 2012 at 8:18 comment added Green Noob @Bernhard I just took 10 km as an example. What I really wanted to know was how to solve the problem considering the variation in distance.
Jan 23, 2012 at 8:15 comment added Green Noob @LubošMotl Can you give a more detailed answer? I'm familiar with differential equations (though I don't claim to be an expert) I'll try to grasp whatever I can.
Jan 23, 2012 at 8:14 comment added Bernhard @LubošMotl If you want to calculate the time at which they meet, an approximation with constant r will get you close enough. Since the radius of the earth plus 10km will not change too much here.
Jan 23, 2012 at 8:00 comment added Luboš Motl The time needed for two balls to collide by the action of gravity: It's an analytically solvable problem but too mathematically contrived one for a beginner. The resulting formula is pretty messy. One has to find the solution to the Kepler problem (differential equations) etc. Yes, the acceleration is accelerated because the force (and therefore acceleration) itself is increasing as the particles get closer to each other.
Jan 23, 2012 at 6:32 history asked Green Noob CC BY-SA 3.0