Register to reply 
What would happen if two Earth size planets very slowly collided? 
Share this thread: 
#1
Sep911, 08:46 PM

P: 18

Hypothetically this pseudoEarth suddenly appears and follows the same orbit as Earth, but moves slightly faster. If it eventually collides with Earth at snail pace what would the gravitational effects be like? (maybe ignore the moons)



#2
Sep911, 10:30 PM

P: 63

You mean like earth #2 chasing earth #1? well, it would be one hell of an unforgettable sight for a few weeks as the planet approaches. I assume E1 would slow down in it's orbit around the sun as E2 gains speed towards us. Can you imagine the sight as it passes the moons orbit? Scary but fascinating. I picture the planets from the movie Pitch Black, except we all die a feiry explosive death from a planet collision.



#3
Sep1011, 11:17 PM

Mentor
P: 11,621

I believe the two planets would pull each other towards themselves and eventually both would be falling towards each other at 9.8 m/s^2 right before they hit.



#4
Sep1011, 11:29 PM

PF Gold
P: 7,120

What would happen if two Earth size planets very slowly collided?



#5
Sep1111, 12:19 AM

Emeritus
Sci Advisor
PF Gold
P: 5,196

This is assuming that the planets have not only the same mass, but also the same size. EDIT: Nevermind. At this point they really can't be considered to act as point masses and you have to take into account tidal effects and all that... 


#6
Sep1111, 12:48 AM

P: 6

I had this big chart with a bunch of the stats of gravitational acceleration for both planets at certain distances and velocity changes and all that jazz took a while to do on my computer calculator. But alas I had most of it on an Excel chart and blam crashola program not responding, I was on a roll and hadn't saved in a while... My initial obsessive motivation has mostly drained out of me for now. Might pick it up again tomorrow.
I did make a few mental notes though. Two big factors came in to play: initial distance between Earth 1 and Earth 2, and time until impact. You have any idea what you want those to look like? Either one would do nicely I assume this is for a story. If not and it's just for your own curiosity I'll just throw something together saying they started like 630,729,000m apart moving at the same speed. But regardless the acceleration at point of impact isn't really what matters because you take into account the acceleration due to gravity across the vast distances of space between them and it continually builds up decelerating Earth 1 and accelerating Earth 2 until the impact and at that point it doesn't really matter how snail pace faster Earth 2 was moving or even if Earth 2 was moving slower initially. By the time they collide the impact due to their velocity differential would be quite something. This all of course depends on the initial distance between them. I was mostly using the equation g_{h}=g_{o}(r_{e}/(r_{e}+h))^{2} and the variations I derived from it would that equation be correct? Or would I have to double r_{e} because there are two Earths? g_{h}= Earth's gravitational acceleration on a object at a distance outside Earth's radius m/s^{2} g_{o}= Earth's standard gravitational acceleration of an object in m/s2 (usually 9.80665m/s^{2} but I used both 19.6133m/s^{2} and 39.2266m/s^{2} to get results due to 2 Earths being present) r_{e}= Radius of Earth in meters h= Distance in meters of object outside of Earth's radius Oh and all my work is disregarding the whole orbital part I haven't really studied orbital acceleration and orbital factors very extensively yet. Also disregarding spin and the influence of the moons. That's just a bit much for me right now. 


#8
Sep1111, 07:25 AM

Mentor
P: 11,621




#9
Sep1111, 12:03 PM

Emeritus
Sci Advisor
PF Gold
P: 2,361

Here's why. As it begins to approach the Earth from behind, the Earth's gravity starts to pull forward on it. But a forward force acting on a orbiting object pushes it into a higher orbit. higher orbits are slower orbits. Meanwhile, the planet is pulling backward on the Earth, causing it to fall into a lower faster orbit So what happens is that before the planet reaches the Earth it will be pushed into an orbit that is higher and slower and the Earth drifts into a lower faster one and will begin to pull away from the planet. Fast forward up to the point where the faster Earth is catching up to the slower planet. Now the Earth pulls back on the planet and the Planet pulls forward on the Earth. The Earth drifts into the slower orbit and the planet into the faster one. The planet pulls away until it begins to catch up with the Earth again and we are back where we started. This is called a "horseshoe" orbit, from the the fact that the path of one planet looks like a horseshoe from the perspective of the other. 


#10
Sep1111, 12:18 PM

Mentor
P: 11,621




#11
Sep1111, 02:43 PM

Emeritus
Sci Advisor
PF Gold
P: 5,196




#12
Sep1111, 02:55 PM

Sci Advisor
PF Gold
P: 1,542

How appropriate that Janus was the first to spot the horseshoe configuration! The best example of this in our solar system are Saturn's moons, Janus and Epimetheus. Here's a webpage I made describing their orbits: http://www.orbitsimulator.com/gravit...les/janus.html



#13
Sep1111, 06:56 PM

Mentor
P: 11,621




#14
Sep1311, 01:28 AM

P: 3

What happens when Earth1 and Earth2 pass within each others' Roche limits?



#15
Sep1311, 08:40 AM

PF Gold
P: 6,135

I don't know this stuff well so sure could be wrong, but my understanding is that the Roche limit has to do with loosely bound objects such as comets and would not apply to strongly bound objects such as a planet.



#16
Sep1311, 09:08 AM

P: 3

It reminds me of sciencefiction stories (Rocheworld, heh) by Dr. Robert L. Forward of two planets which were so close that ocean and atmosphere would occasionally spill back and forth. 


#17
Sep1311, 11:07 AM

Emeritus
Sci Advisor
PF Gold
P: 2,361




#18
Sep1311, 03:44 PM

PF Gold
P: 6,135

(1) It seems to me that a loosely cohesive grouping of rocks that had brought itself into more or less of a sphere would be torn apart far further out from a planet than would an object that was one solid rock (USED to be many rocks but has brought itself into a sphere then cooled off enough to no longer have a liquid core). (2) The Roche limit is based on the mass of the planet and is independent of the approaching object. If both of these were true then only one of the incoming objects could be torn apart specifically at the Roche limit, so I assume I'm wrong about one or the other, possibly both. Thanks 


Register to reply 
Related Discussions  
Calculating the size of planets from length of days.  Astronomy & Astrophysics  4  
What would happen if two black holes collided?  Astronomy & Astrophysics  2  
Why Can't Rocky Planets Exceed 14 Times Earth's Size?  Astronomy & Astrophysics  25  
What would happen if...? (imaginary earth)  Classical Physics  4  
What would happen if two black holes collided?  Astronomy & Astrophysics  2 