How long would it take two planets to collide?

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Discussion Overview

The discussion revolves around the hypothetical scenario of two celestial bodies, specifically the Earth and the Moon, colliding. Participants explore the time it would take for them to impact each other under idealized conditions, focusing on gravitational interactions and the implications of such a collision. The conversation includes considerations of mathematical modeling, observational effects, and conceptual clarifications regarding the nature of the collision.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant proposes a method involving conservation of energy and momentum to calculate the time until collision, but notes that their solution is incomplete due to the complexity of the resulting function.
  • Another participant questions whether the specifics of the collision matter for determining the time to impact, indicating uncertainty about the relevance of collision dynamics.
  • Several participants discuss the perceptual aspects of the Moon's approach, suggesting that initial changes in its appearance would be subtle and not easily noticeable to casual observers.
  • One participant provides a detailed estimation of how the Moon's angular size would change over time as it approaches Earth, noting specific percentage increases over 24-hour intervals.
  • There are references to lunar laser ranging measurements that could detect changes in the Moon's position relative to Earth, emphasizing the precision of such observations.
  • Participants express interest in visualizing the dynamics of celestial collisions, such as the historical event of Theia colliding with Earth to form the Moon.

Areas of Agreement / Disagreement

Participants express a range of views on the implications of the collision and the observational effects, with no clear consensus on the specifics of the collision dynamics or the time it would take for the bodies to collide. The discussion remains unresolved regarding the exact calculations and implications of the scenario.

Contextual Notes

Some assumptions about the idealized conditions of the Earth-Moon system are not explicitly stated, and there are unresolved mathematical steps in the proposed solutions. The discussion also reflects varying degrees of understanding regarding the perceptual changes associated with the Moon's approach.

rohanlol7
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So, i was on the plane going for oxford interviews and i was thinking about what i could be asked. While i was thinking i came up with this one. Suppose the Earth and the moon were at a distance α apart at rest, how long would it take for them to crash into each other. I'm only really considering an ideal situation where the system is only comprised of the Earth and the moon. So i tried to solve it in general for two planets of mass M1 and M2 respectively.
If anyone could provide a method or a solution. I was initially going to type in my work but its going to take hours. if anyone wants to see it just pm me. ( mine involves conservation of energy and momentum and len gthy calculus. my solution is not complete as the function i obtained was so complex that i was too lazy to substitute everything in. thanks everyone
 
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End of collision is cessation of interaction? As in attractive force, but no longer permanent distortions?
 
Hmm I don't know actually. I just took them as point masses. Does it actually matter what happens at the collision when I'm trying to find the time taken for them to impact?
If I'm making no sense I probably misunderstood you
 
What I've always found interesting about this - if I remember correctly - is that for the first day you wouldn't even notice unless you were really paying attention.
 
Notice what? :D
 
rohanlol7 said:
Notice what? :D
The moon careening toward Earth.
 
russ_watters said:
The moon careening toward Earth.
Right. On the first day it would be more like "looking in that general direction" rather that "careening towards" :smile:
 
  • #10
What would be fun would be to see a real time animation of Theia colliding with Earth to form the moon.
 
  • #11
Ah i never thought of that. I would love to see one where the Earth slowly spirals towards the sun for some sort of reason
 
  • #12
russ_watters said:
What I've always found interesting about this - if I remember correctly - is that for the first day you wouldn't even notice unless you were really paying attention.
I assume that you mean that if the Moon were falling straight towards the Earth, you wouldn't see a noticeable increase in its size for the first 24 hrs. This is likely true, as in the first 24 hrs, its angular size would only increase by ~3%. And assuming that it started at it's average distance, it would not even have reached its normal perigee distance yet. In the next 24 hrs, it will increase by another 9.5% for a total increase of 12.5%, which should be noticeable (but maybe not to the casual observer. the Moon in its semi-monthly trip from apogee to perigee changes size by ~17%*, so I wonder if someone not looking for it would notice a 9.5% increase in size between two successive nights, since the Moon would still be within its normal range of viewing size.)
12 hrs later, it will have swollen another 9.5% and be 22% larger than it started, and 12 hrs later than that it will have grown to 36% larger than what it started at, and somewhere by now people will begin to notice. * as an aside, if the Moon started falling at apogee, it would take a little over 2 days to fall to its normal perigee distance.
 
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  • #13
phinds said:
Right. On the first day it would be more like "looking in that general direction" rather that "careening towards" :smile:

http://cdn2-b.examiner.com/sites/default/files/styles/image_content_width_large/hash/c1/25/c125eeaea3694b51520ec74710f6f5cc.jpg?itok=CXgs-OJv
 
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  • #14
Lunar laser ranging would note it within seconds (assuming they do a measurement at the right time):
- they would not hit the retroreflectors any more due to the lack of lateral motion.
- if the moon does not happen to be at its highest point in the sky, the radial distance would become different as well. This can be noted with the first light pulse even after fractions of a second - but this light pulse takes ~1.5 seconds to reach the station. And that is really the absolute limit on notability speed.
 
  • #15
mfb said:
Lunar laser ranging would note it within seconds (assuming they do a measurement at the right time):
- they would not hit the retroreflectors any more due to the lack of lateral motion.
- if the moon does not happen to be at its highest point in the sky, the radial distance would become different as well. This can be noted with the first light pulse even after fractions of a second - but this light pulse takes ~1.5 seconds to reach the station. And that is really the absolute limit on notability speed.

It also wouldn't take any amateur astronomer too long to note that the Moon was no longer moving relative to the background stars, since this motion is about its angular size per hour.
 

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