Tides due to the moon vs. the sun?

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Discussion Overview

The discussion centers on the comparative effects of the moon and the sun on Earth's tides, exploring the reasons why tides are predominantly influenced by the moon despite the sun's greater gravitational pull. The scope includes theoretical explanations, mathematical reasoning, and conceptual clarifications regarding tidal forces.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • Some participants assert that the moon's proximity to Earth results in a significantly larger tidal effect compared to the sun, despite the sun's greater mass.
  • Others explain that tides are caused by the difference in gravitational force between the near and far sides of Earth, with the sun's distance diminishing its tidal influence.
  • A participant calculates that the tidal force from the sun is approximately half that of the moon, based on the differences in gravitational pull across Earth.
  • Some participants challenge earlier calculations and emphasize the importance of considering the differences in gravitational force rather than just the absolute values of gravitational pull.
  • There is a discussion about the mathematical relationship between gravitational force and tidal effects, including the effects of distance on these forces.
  • One participant raises a question about why tides are determined by the difference in forces rather than the total gravitational forces acting on Earth.

Areas of Agreement / Disagreement

Participants express differing views on the relative contributions of the moon and sun to tidal forces, with no consensus reached on the exact nature of these contributions or the calculations involved. The discussion remains unresolved regarding the implications of the differences in gravitational forces.

Contextual Notes

Some calculations presented rely on specific assumptions about distances and masses, and there are unresolved mathematical steps regarding how these relate to tidal effects. The discussion also touches on the conceptual understanding of forces acting on Earth.

Who May Find This Useful

This discussion may be of interest to those studying astrophysics, oceanography, or anyone curious about the mechanics of tidal forces and gravitational interactions between celestial bodies.

  • #31


selfAdjoint said:

Yes, the bulges are the same height. On the near side to the moon the water is closer to the moon than the Earth and is more strongly pulled, hence it is pulled up into a bulge. On the far side the Earth is closer to the moon than the water, so it is pulled away from the water, making a water bulge. Tidal forces are all about differential effects of gravitation at different distances.


Yeah, I know it's an old topic, but something bugged me about this answer. I have never heard this explanation for the second water bulge. I thought the second one was created due to the centrifugal force that arises from the Earth and moon revolving around their centre of mass?
 
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  • #32


Shukie said:
Yeah, I know it's an old topic, but something bugged me about this answer. I have never heard this explanation for the second water bulge. I thought the second one was created due to the centrifugal force that arises from the Earth and moon revolving around their centre of mass?

It's not centrifugal force; that has nothing to do with it.

The answer you have quoted is correct and it explains the bulges on both sides and why they are about equal. Read it again. It says: Tidal forces are all about differential effects of gravitation at different distances. It stretches out a fluid sphere into an ellipsoid shape. Relevant to the center of the sphere, you get bulges on each side. There's a difference between the Moon's gravity at the center of the Earth and the nearside bulge, and there's about the same difference between the Moon's gravity at the center of the Earth and the far side bulge.
 
  • #33


I found this to be a very insightful and interesting undergraduate thesis on tides by a world-class student (currently I think a PhD student at Caltech).

http://www.gps.caltech.edu/~carltape/research/pubs/thesis/tides_CHT_thesis.pdf" (6.7 MB)
 
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  • #34


Shukie said:
Yeah, I know it's an old topic, but something bugged me about this answer. I have never heard this explanation for the second water bulge. I thought the second one was created due to the centrifugal force that arises from the Earth and moon revolving around their centre of mass?
That is a common but completely erroneous explanation. First off, what centrifugal force?

Secondly, and more importantly, suppose an object of the Moon's mass is falling straight toward the Earth with zero tangential velocity. There is no centrifugal force in this case; the object is falling straight into the Earth. At the point in time that this object reaches the Moon's orbital distance the tidal forces will be exactly equal to those exerted by the Moon. The tidal forces exerted by the Moon has nothing per se to do with Moon's orbit. It is solely a function of where the Moon is.

So, how to explain that there are two bulges? The answer is simple. The Earth as a whole is accelerating gravitationally toward the Moon:

a_e = \frac {GM_m}{{R_m}^2}

where ae is the acceleration of the Earth toward the Moon, Mm is the mass of the Moon, and Rm is the distance between the centers of the Earth and the Moon.

The distances between the center of the Moon and the points on the surface of the Earth directly opposite the Moon and directly between the Earth and Moon are Rm+re and Rm-re, respectively. Here re[/i] is the radius of the Earth

Because these points are a bit further from/closer to the Moon than the center of the Earth, the acceleration toward the Moon at these points will be slightly different than that of the Earth as a whole. In particular,

a_p = \frac {GM_m}{(R_m\pm r_e)^2}

It is the difference in acceleration that is important here. Calculating this,

a_{p,\text{rel}} = \frac {GM_m}{(R_m\pm r_e)^2} - \frac {GM_m}{{R_m}^2}<br /> \approx \mp\, 2\,\frac{GM_mr_e}{R_m^3}

The point on the surface of the Earth directly between the centers of the Earth and the Moon experiences a bit more acceleration toward the Moon that does the Earth as a whole, so this differential acceleration is directed toward the Moon -- that is, away from the center of the Earth. The point on the surface of the Earth directly opposite the Moon experiences a bit less acceleration toward the Moon that does the Earth as a whole, so this differential acceleration is directed away from the Moon -- which is, once more, away from the center of the Earth. The Moon pulls the submoon point and its antipode apart, like a piece of taffy. For the points on the surface of the Earth where the Moon is at the horizon, the action is to squeeze those points inward a tiny bit.

For the Moon these tidal forces are very, very small. For a neutron star or black hole they are not. There is a cool technical term for how black holes pull the extremes of some object apart and squeeze in at the middle: http://en.wikipedia.org/wiki/Spaghettification" .
 
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  • #35


Shukie said:
Yeah, I know it's an old topic, but something bugged me about this answer. I have never heard this explanation for the second water bulge. I thought the second one was created due to the centrifugal force that arises from the Earth and moon revolving around their centre of mass?
The easiest way to deal with this is to get rid of the rotational motion altogether. Without the moon being in orbit and the Earth rotating, the tides would still be there (for a little while, anyway - until the moon crashed into the earth!).
 
  • #36


russ_watters said:
The easiest way to deal with this is to get rid of the rotational motion altogether. Without the moon being in orbit and the Earth rotating, the tides would still be there (for a little while, anyway - until the moon crashed into the earth!).

Exactly! The only thing necessary condition for tides (or differential acceleration) is that the object be in free fall. The effect of rotation enables us to "see" the tides by standing in one place, and the effect of orbital free fall keeps the whole experience going on and on.
 
  • #37


billiards said:
Exactly! The only thing necessary condition for tides (or differential acceleration) is that the object be in free fall.
The only necessary condition for tides to exist is that the object be where it is. It does not have to be in free fall. Outfit the Moon with some BIG honking rocket engines that are capable of making the Moon hover 384,399 km away from the center of the Earth without orbiting and the tides will still exist.
 
  • #38


Alright, so this topic is old. But there is one thing I've been puzzling over for the past half day.

Say we ignore the sun's effect on the tides and just went with the moon-earth system. I understand why the tides happen, but I don't understand why, in an idealized model of the Earth (sphere covered completely with water , no variation in water depth), the tides on either side of the Earth are equal.
 
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