How much closer was the Moon say 200,000 years ago?

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Discussion Overview

The discussion revolves around the historical distance of the Moon from Earth, specifically focusing on how much closer the Moon was approximately 200,000 years ago. Participants explore the implications of the Moon's gradual recession from Earth, the significance of this distance change, and the factors that might influence its orbital dynamics.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants mention that the Moon is receding from Earth at a rate of approximately 38 millimeters per year.
  • One participant calculates that over 200,000 years, this would amount to a distance change of about 4.7 miles (or 7 kilometers).
  • There is a question raised about whether such a small change would be noticeable from a distance of nearly 400,000 kilometers.
  • Concerns are expressed regarding the ability to prove that the Moon has been moving away at this exact rate for such a long time, considering potential influences from impacts on its surface.
  • Another participant argues that the effect of impacts on the Moon's trajectory is negligible compared to tidal forces, suggesting that the recession is a result of a constant conversion of lunar orbital momentum into tidal effects on Earth.
  • Technical calculations are presented regarding the momentum changes associated with the Moon's recession and the estimated mass of impacts, indicating that the cumulative effect of impacts is likely much smaller than the tidal losses.

Areas of Agreement / Disagreement

Participants express differing views on the significance of the Moon's recession and the impact of surface collisions on its trajectory. There is no consensus on the implications of the distance change or the factors influencing the Moon's movement.

Contextual Notes

Some assumptions about the constancy of the recession rate and the influence of impacts remain unresolved. The discussion includes complex calculations and technical reasoning that may depend on specific definitions and conditions.

stany
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much difference?
 
Astronomy news on Phys.org
[...] this causes the Moon to slowly recede from Earth at the rate of approximately 38 millimetres per year.
(Wikipedia)
 
so what would dat be?
 
You can't calculate it yourself? Make an effort. This isn't a place to have things spoon-fed to you.
 
4.7 miles

you think that would make the moon appear much closer? i mean if suddenly the moon appeared 5 miles closer would you notice?
 
how far is the moon away from the earth?

384,403 kilometers is the number i got for an average. 4.7 miles is about 7 kilometers.

would you notice a change of 7 kilometers if you were almost 400 000 kilometers away?
 
Is there any way to prove it has been moving away at this exact speed for that long? 38 millimeters a year is barely anything, so wouldn't some of the millions of impacts along the surface influence its direction?
 
dacruick said:
how far is the moon away from the earth?

384,403 kilometers is the number i got for an average. 4.7 miles is about 7 kilometers.

would you notice a change of 7 kilometers if you were almost 400 000 kilometers away?

yes.
 
you have fantastic depth perception then.
 
  • #10
Stanwyck66 said:
Is there any way to prove it has been moving away at this exact speed for that long? 38 millimeters a year is barely anything, so wouldn't some of the millions of impacts along the surface influence its direction?
The effect of the impacts is miniscule becaues they make up a tiny fraction of the mass of the moon. 200,000 years is a pretty short time, so it is unlikely that it has changed much in that time.
 
  • #11
Stanwyck66 said:
Is there any way to prove it has been moving away at this exact speed for that long? 38 millimeters a year is barely anything, so wouldn't some of the millions of impacts along the surface influence its direction?
Interesting question, even though, I think, it's based on a misconception. The recession is not an inertial but a friction effect, namely the result of a constant conversion of lunar orbital momentum into tidal effects on Earth. So, counteracting this effect by bombarding the moon with impactors would be not like changing the direction of a rolling car by throwing balls at it, which is tedious but easily doable given enough balls, but like trying to keep the car from eventually stopping due to energy loss, which is much harder in the long run.

Quantitatively, the figure means that the Moon's distance from Earth increases by one part in 10^10 per year, which roughly corresponds to a change in orbital speed by the same fraction, so the annual change in momentum is

delta p ~ lunar mass * change in lunar orbital speed ~ 10^23 kg * 10^3 m/s / 10^10 ~ 10^16 kg m/s

The typical speed of an impactor is on the order of tens of kilometres per second, so counteracting this would require an asymmetric bombardment on the order of 10^12 kg per year. I wasn't able to find a cumulative figure anywhere, but several publications gave total impact masses for certain impactor size ranges, and all of those were in the range of 10^3 to 10^6 kg per year per mass decade (i.e. impactor mass between 10^n and 10^(n+1) kg), so I'm guessing the grand total won't exceed 10^9 kg. And most of that is symmetric, so the momentum contributions will cancel each other out.

So, the answer seems to be that the effect of impacts is negligible in comparison with that of tidal losses, unless I made a major mistake somewhere.
 

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