Insights Beyond the Tidal Bulge

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The discussion centers around the concept of tidal bulges and the validity of Newtonian versus Laplace dynamics theories in explaining ocean tides. Participants debate whether a tidal bulge exists and the implications of a perfect sphere covered with water. The Newtonian model is critiqued for being overly simplistic and not accurately representing oceanic tides on Earth, with claims that it serves more as a basic educational tool rather than a reliable scientific explanation. The dynamic theory of tides is presented as a more accurate model, particularly for understanding phenomena like the volcanic activity on Io, which is influenced by tidal forces. The conversation also touches on the limitations of the equilibrium tide model and its applicability to solid body tides versus oceanic tides. Overall, the discussion emphasizes the complexity of tidal dynamics and the need for more nuanced models to accurately describe tidal behavior.
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Is the Newtonian tidal bulge an approximation of Laplace dynamics theory of tides in some limit?

Edit: I mean if I just take the predominant mode or something like that does everything correspond with Newtonian theory?

Edit2: I felt that the article was missing a conclusion on key differences between the two models aside from Laplace's model being more realistic. Very interesting nonetheless!
 
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If the Earth were a perfect sphere covered with a uniform ocean, then would there be?
 
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bob012345 said:
If the Earth were a perfect sphere covered with a uniform ocean, then would there be?
My take on this is that "no, at least not the bulge predicted by Newton", one of the key take aways is that the ocean is not deep enough. But as you, I still wonder if there would be any other difference aside from that. Would there be a bulge?
 
pines-demon said:
Is the Newtonian tidal bulge an approximation of Laplace dynamics theory of tides in some limit?
In the limit of a water planet tidally-locked to its principal moon, whose rotational angular velocity vector aligns with the moon's orbital angular velocity vector, and the orbital eccentricity is very small, then yes, there is no need for the dynamics theory of the tides (at least not for the moon. The only thing the dynamics theory carries over from the equilibrium model is the tidal forcing function, and then only the horizontal components. The dynamics theory is a component replacement for the equilibrium theory.
pines-demon said:
Edit: I mean if I just take the predominant mode or something like that does everything correspond with Newtonian theory?
The predominant mode of the dynamics theory is the one cycle per 12.421 hours M2 tidal. The predominant mode of the equilibrium tide model is the tidal bulge moving at one cycle per 12.421 hours around the Earth. That however does not validate the Newtonian theory.
 
bob012345 said:
If the Earth were a perfect sphere covered with a uniform ocean, then would there be?
We'll perhaps have a clearer picture of a tidally-locked terrestrial object with an ocean that covers the globe beginning in April 2030. That's when the Europa Clipper will arrive in orbit around Jupiter with a strong focus on developing a clearer picture of what's happening in Europa.
 
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D H said:
The predominant mode of the dynamics theory is the one cycle per 12.421 hours M2 tidal. The predominant mode of the equilibrium tide model is the tidal bulge moving at one cycle per 12.421 hours around the Earth. That however does not validate the Newtonian theory.
Maybe does not validate Newtonian theory but makes it a good first approximation to learn (maybe with a warning "but it is more complicated due to continents"). I mean we still teach Newtonian gravitation and we do not go straight into general relativity for a reason. For many practical purposes Newtonian gravitation is enough and the same could be said about the Newtonian tide model.

Edit: the Newtonian tide model is not in the ensemble of obsolete theories that are clearly wrong, like for example the emission theory of vision.
 
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D H said:
We'll perhaps have a clearer picture of a tidally-locked terrestrial object with an ocean that covers the globe beginning in April 2030. That's when the Europa Clipper will arrive in orbit around Jupiter with a strong focus on developing a clearer picture of what's happening in Europa.
I would be surprised if this hasn’t been simulated many times. BTW, what would we call that big wave in the movie Interstellar?
 
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  • #10
pines-demon said:
Maybe does not validate Newtonian theory but makes it a good first approximation to learn (maybe with a warning "but it is more complicated due to continents").
In practice, this is exactly what is done. See for example NASA and the (US) National Oceanographic and Atmospheric Administration.
 
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bob012345 said:
BTW, what would we call that big wave in the movie Interstellar?
I don't know about you but I would call it "bollocks".
 
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  • #12
It sounds to me like the Newtonian picture is really not of much value for understanding what gets called "ocean tides" (the way the ocean goes up and down a beach), quite frankly. Note that is quite a bit different from what we might call "tidal deformation", for which the Newtonian picture applies quite well for simple tidally locked systems. But a simple tidally locked system doesn't have "ocean tides" at all, so the only situation where the Newtonian picture is good is when you have nothing to understand in the first place (if you are a surfer or a boater).
 
  • #13
pines-demon said:
Maybe does not validate Newtonian theory but makes it a good first approximation to learn (maybe with a warning "but it is more complicated due to continents"). I mean we still teach Newtonian gravitation and we do not go straight into general relativity for a reason. For many practical purposes Newtonian gravitation is enough and the same could be said about the Newtonian tide model.
Not really. It is used as a "lie-to-children" as a first step in learning how the ocean tides work. The next step is to teach oceanography students that this model is indeed a "lie to children", that it doesn't describe the oceanic tides at all.
pines-demon said:
Edit: the Newtonian tide model is not in the ensemble of obsolete theories that are clearly wrong, like for example the emission theory of vision.
While the equilibrium tide model is not universally falsified, it is falsified as an explanation for oceanic tides on the Earth. The equilibrium tide model is a fairly good model for the solid body tides in the Earth and in the Moon. It is also presumably a fairly good model for tidally-locked moons.

bob012345 said:
I would be surprised if this hasn’t been simulated many times.
Not just many times, but many times over, at least from the perspectives of Europa Clipper failure detection & handling thereof, robustness against radiation, thermal control, GNC *guidance, navigation & control), and many other aspects. NASA has a very strong tendency to simulate things to death. Regarding what the Europa Clipper will observe -- that's a different question. The instruments aboard the vehicle were designed to detect phenomena based on predictions, but also detect where those predictions might be wrong. I didn't do scientific instrument design in my long aerospace career, but I suspect they too heavily rely on simulations.
bob012345 said:
BTW, what would we call that big wave in the movie Interstellar?
Something made up to make a movie more dramatic? Movies, sci-fi movies in particular, make stuff up all the time.

pbuk said:
In practice, this is exactly what is done. See for example NASA and the (US) National Oceanographic and Atmospheric Administration.
That is the "lie-to-children" (and in the case of the NASA site, also a "lie-to-adults") I mentioned earlier (and in the article) regarding the modeling of the oceanic tides. Other than frequency (1 cycle per 12.421 hours), the oceanic tides do not follow the predictions of this lie-to-children. The frequency of 1 cycle per 12.421 hours is exactly the same as that of the M2 tidal constituent. The M2 tidal constituent from the dynamic theory of the tides does a very good job of predicting the tides while the equilibrium tide model does not.

Ken G said:
It sounds to me like the Newtonian picture is really not of much value for understanding what gets called "ocean tides" (the way the ocean goes up and down a beach), quite frankly. Note that is quite a bit different from what we might call "tidal deformation", for which the Newtonian picture applies quite well for simple tidally locked systems.
I wholeheartedly agree. If one goes to the National Oceanic and Atmospheric Administration's tide prediction page and chooses a tide station locations (make sure to pick stations that are listed as "harmonic" rather than "subordinate") and looks at the harmonic constituents for those locations, one will see that the phase angle for the M2 tidal constituent takes on all values between 0° and 360°. This phase angle would be close to the same value for all sites if the equilibrium tide model was anywhere close to correct.
Ken G said:
But a simple tidally locked system doesn't have "ocean tides" at all, so the only situation where the Newtonian picture is good is when you have nothing to understand in the first place (if you are a surfer or a boater).
While not quite right, what you wrote is very close to right. None of the tidally locked moons of Jupiter have a perfectly circular orbit. Their orbits are instead very slightly elliptical. That slight ellipticity is enough to create time-varying tides. Those moons are more or less tidally locked, where "more or less" in this case means "on average". The tides on those moons can be viewed as small time-varying perturbations on top of a very large permanent tide. Those small variations are large enough to make Io the most volcanically active object in the solar system and to make Europa's supposedly thin ice layer on top of a global ocean geologically young. I wrote "supposedly" because that is the best scientific guess without actually going there. Europa Clipper is going there.
 
  • #14
D H said:
Not really. It is used as a "lie-to-children" as a first step in learning how the ocean tides work. The next step is to teach oceanography students that this model is indeed a "lie to children", that it doesn't describe the oceanic tides at all.

While the equilibrium tide model is not universally falsified, it is falsified as an explanation for oceanic tides on the Earth. The equilibrium tide model is a fairly good model for the solid body tides in the Earth and in the Moon. It is also presumably a fairly good model for tidally-locked moons.
I am trying to figure out how to classify the Newtonian water tidal theory. In science, there seem to be theories that are obsolete and we throw them to the trash as soon as we find a better one, and less accurate ones that we keep as first approximation. If I take the dynamic tidal model and reduce some couplings or average out some features do I get the Newtonian one? It seems so. In this sense, the Newtonian tide model is to the dynamic theory of tides what the ray optics is to wave optics or to quantum optics. You get one from the other in the eikonal limit.

The question asked early seems important here, if I have a perfect sphere covered with water (circular orbit, tidally-locked if needed) what is the prediction? If the prediction is different from the Newtonian model what is the key difference?
 
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  • #15
bob012345 said:
I would be surprised if this hasn’t been simulated many times. BTW, what would we call that big wave in the movie Interstellar?
This is Kip Thorne's explanation from the book on the science of Interstellar:
What could possibly produce the two gigantic water waves, 1.2 kilometers high, that bear down on the Ranger as it rests on Miller's planet (Figure 17.5)? I searched for a while, did various calculations with the laws of physics, and found two possible answers for my science interpretation of the movie. Both answers require that the planet be not quite locked to Gargantua. Instead it must rock back and forth relative to Gargantua by a small amount [snip Thorne's explanation of how Gargantua's tidal gravity will naturally provide a sort of restoring force back to its preferred orientation, explaining why the planet would rock this way] ... The result is a simple rocking of the planet, back and forth, if the tilts are small enough that the planet's mantle isn't pulverized. When I computed the period of this rocking, how long it takes to swing from left to right and back again, I got a joyous answer. About an hour. The same as the observed time between giant waves, a time chosen by Chris without knowing my science interpretation.

The first explanation for the giant waves, in my science interpretation, is a sloshing of the planet's oceans as the planet rocks under the influence of Gargantua's tidal gravity.

A similar sloshing, called "tidal bores," happens on Earth, on nearly flat rivers that empty into the sea. When the ocean tide rises, a wall of water can go rushing up the river; usually a tiny wall, but occasionally respectably big. ... But the moon's tidal gravity that drives this tidal bore is tiny—really tiny—compared to Gargantua's huge tidal gravity!

My second explanation is tsunamis. As Miller's planet rocks, Gargantua's tidal forces may not pulverize its crust, but they do deform the crust first this way and then that, once an hour, and those deformations could easily produce gigantic earthquakes (or "millerquakes," I suppose we should call them). And those millerquakes could generate tsunamis on the planet's oceans, far larger than any tsunami ever seen on Earth
 
  • #16
D H said:
Not really. It is used as a "lie-to-children" as a first step in learning how the ocean tides work. The next step is to teach oceanography students that this model is indeed a "lie to children", that it doesn't describe the oceanic tides at all.

While the equilibrium tide model is not universally falsified, it is falsified as an explanation for oceanic tides on the Earth. The equilibrium tide model is a fairly good model for the solid body tides in the Earth and in the Moon. It is also presumably a fairly good model for tidally-locked moons.


Not just many times, but many times over, at least from the perspectives of Europa Clipper failure detection & handling thereof, robustness against radiation, thermal control, GNC *guidance, navigation & control), and many other aspects. NASA has a very strong tendency to simulate things to death. Regarding what the Europa Clipper will observe -- that's a different question. The instruments aboard the vehicle were designed to detect phenomena based on predictions, but also detect where those predictions might be wrong. I didn't do scientific instrument design in my long aerospace career, but I suspect they too heavily rely on simulations.

Something made up to make a movie more dramatic? Movies, sci-fi movies in particular, make stuff up all the time.


That is the "lie-to-children" (and in the case of the NASA site, also a "lie-to-adults") I mentioned earlier (and in the article) regarding the modeling of the oceanic tides. Other than frequency (1 cycle per 12.421 hours), the oceanic tides do not follow the predictions of this lie-to-children. The frequency of 1 cycle per 12.421 hours is exactly the same as that of the M2 tidal constituent. The M2 tidal constituent from the dynamic theory of the tides does a very good job of predicting the tides while the equilibrium tide model does not.


I wholeheartedly agree. If one goes to the National Oceanic and Atmospheric Administration's tide prediction page and chooses a tide station locations (make sure to pick stations that are listed as "harmonic" rather than "subordinate") and looks at the harmonic constituents for those locations, one will see that the phase angle for the M2 tidal constituent takes on all values between 0° and 360°. This phase angle would be close to the same value for all sites if the equilibrium tide model was anywhere close to correct.
It certainly looks like this is not a "lie to children," it's just a "lie." I'm not a big fan of lying to students, it smacks of "truthiness," and science is supposed to be pretty close to the opposite of that.
D H said:
While not quite right, what you wrote is very close to right. None of the tidally locked moons of Jupiter have a perfectly circular orbit.
That's what I meant by "simple" tidal locking. But then, if it's not simple, then the Newtonian picture suffers its own problems. So again, it really looks like we should just bite the bullet and either take on the Laplace approach, or steer clear of ocean tides altogether. One can do the Newtonian approach to tidal deformation if you want to understand Hill spheres and Lagrange points, and if you want to understand the two-a-day frequency of ocean tides, you can use Newton to get a concept of "tidal forcing", as you say, but stop short of talking about the response to tidal forcing as being like the ocean getting "rotated through the bulges" twice each day (that's the part that's clearly as wrong as wrong gets, given that phase information you mention).

But this raises two deeper questions. It is often said that the Moon is getting farther from the Earth because the closest "point of the football" is rotated (by the lag in moving the oceans around) so it leads the Moon a little. In the Laplace approach, there must be a similar kind of effect, so should we use the Newtonian tidal deformation argument to understand why the Moon is gaining orbital angular momentum, or is that just as wrong as the phase information you mention?

Another question I have wondered about is, I recall hearing that Io is volcanic because it is "kneaded like bread" by the changing tidal deformation of its (very slightly) elliptical orbit. But there are deeper issues here, because Io's orbit is less than 2 days, yet the orbit itself evolves on timescales longer than a year. So immediately we must wonder if the "kneading" is the 2-day effect of its eccentricity, or much longer timescale changes in the eccentricity. The reason the latter is relevant is that if we are dealing with longer variations than one orbit, how do we know the real heating that matter happens during much larger changes in its eccentricity over time, such that the current eccentricity plays almost no role at all in keeping Io volcanically active? (This paper: https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2019GL082691 suggests that volcanic eruptions do vary on the ~480 day period of orbital changes, but it leaves open the question of whether there are much longer period changes that are more important for keeping the moon's interior molten in the first place.)
 
  • #17
pines-demon said:
I am trying to figure out how to classify the Newtonian water tidal theory.
Aside: It's called the equilibrium tide model rather than Newtonian water tidal theory. There is at least one aspect that Newton did get right and is still used, which is the tidal forcing function. That said, it is best to discard the vertical component of that forcing function, as Laplace did. The response of the Earth's oceans to that forcing, the equilibrium tide: Newton got that completely wrong. So, falsified. It is nowhere close to being universally true, even in a Newtonian sense. Moreover, it has been falsified on the one planet in the entire universe that matters most to humankind, which is of course the Earth.

If you're looking for an analogy, I would classify it somewhere between the phlogiston and caloric theories of heat, both of which have been tossed onto the big pile of discarded scientific theories. Phlogiston theory is completely off. Caloric theory has some truth to it. For example, Carnot's heat engine concepts are deeply rooted in caloric theory. Modern thermodynamics has very little in common with caloric theory. Just because a model is wrong does not mean some aspects of that model are not useful.
 
  • #18
D H said:
Aside: It's called the equilibrium tide model rather than Newtonian water tidal theory. There is at least one aspect that Newton did get right and is still used, which is the tidal forcing function. That said, it is best to discard the vertical component of that forcing function, as Laplace did. The response of the Earth's oceans to that forcing, the equilibrium tide: Newton got that completely wrong. So, falsified. It is nowhere close to being universally true, even in a Newtonian sense. Moreover, it has been falsified on the one planet in the entire universe that matters most to humankind, which is of course the Earth.

If you're looking for an analogy, I would classify it somewhere between the phlogiston and caloric theories of heat, both of which have been tossed onto the big pile of discarded scientific theories. Phlogiston theory is completely off. Caloric theory has some truth to it. For example, Carnot's heat engine concepts are deeply rooted in caloric theory. Modern thermodynamics has very little in common with caloric theory. Just because a model is wrong does not mean some aspects of that model are not useful.
Ken G said:
It certainly looks like this is not a "lie to children," it's just a "lie." I'm not a big fan of lying to students, it smacks of "truthiness," and science is supposed to be pretty close to the opposite of that.
Ok let's say that the whole equilibrium tide model is FALSE. What does the dynamic theory of tides predicts for perfect sphere covered with water, circular orbit, tidally-locked, and how does that compare to the equilibrium theory?
 
  • #19
pines-demon said:
Ok let's say that the whole equilibrium tide model is FALSE. What does the dynamic theory of tides predicts for perfect sphere covered with water, circular orbit, tidally-locked, and how does that compare to the equilibrium theory?
If we have only circular orbits and tidally locked bodies, then there are no ocean tides at all to understand, and also no dynamical tide model because there are no dynamics. That was my point, the Newtonian model works perfectly in that situation, but it explains nothing but the shape of the object. The situation where Newton's equilibrium tide model is correct, is also the situation where it has no explanatory value toward understanding ocean tides, because there are none to explain, and the dynamical model also has no usefulness there. It's just an irrelevant test, the idealization has removed the purpose of the explanation.
 
  • #20
Ken G said:
It certainly looks like this is not a "lie to children," it's just a "lie." I'm not a big fan of lying to students, it smacks of "truthiness," and science is supposed to be pretty close to the opposite of that.
The equilibrium tide theory (I'm using theory here in the mathematical sense: a body of knowledge, as in string theory or knot theory) has some validity for some tides, but not in the Earth's oceans, where it has no validity. Educators consider it to be too big of a jump to go from the tidal forcing functions directly to the dynamic theory of the tides. Many students do not comprehend how there can be two bulges, one centered on the zenith point and the other on the antipodal (nadir) point. Those instructors tend to follow Newton's derivation, calling the outer bulge due to a centrifugal force that is constant all across the world. (That is not a centrifugal force. Also, it is not needed. I did not invoke that concept in the article.)

There are bodies where the equilibrium tide model is approximately correct. The solid body tides are one example. Tidally-locked bodies with a liquid covering are another. These are bodies where the perturbations on top of the zero frequency tides are small. Most frequency analyses will inevitably yield a zero frequency response. The zero frequency response in the Earth's oceanic tides is ridiculously small. It is considerably larger in the Earth's solid body tides, and is presumably ridiculously large in Europa's world spanning ocean that lies under the ice.

However, as used for Earth's oceans, the equilibrium tide theory simply does not apply.

Ken G said:
But this raises two deeper questions. It is often said that the Moon is getting farther from the Earth because the closest "point of the football" is rotated (by the lag in moving the oceans around) so it leads the Moon a little. In the Laplace approach, there must be a similar kind of effect, so should we use the Newtonian tidal deformation argument to understand why the Moon is gaining orbital angular momentum, or is that just as wrong as the phase information you mention?
No. We should use the observed tidal energy dissipation that represents a transfer of angular momentum between the solid Earth and the oceans. These are quite observable and stand in as a proxy for the transfer of angular momentum between the oceans and the Moon. Or one can calculate the gravitational effects of all of the various amphidromic systems on the Moon. I don't know whether this has been done.

One thing that has been done is to look at tidal rhythmites, ancient tidal patterns now locked in rock. These tidal rhythmites provide yet another death by a million cuts for the equilibrium tide theory. The Moon's current recession rate extrapolated over the last billion years or so would result in a Moon much younger than the solar system. Tidal rhythmites show that this is not the case' the Moon's current recession rate is considerably higher than it has been on average over the last two billion years. The North Atlantic exhibits considerable resonances with regard to the tidal driving forces. These resonances are nicely explained by the dynamic theory of the tides -- but not by the equilibrium tides.

Ken G said:
Another question I have wondered about is, I recall hearing that Io is volcanic because it is "kneaded like bread" by the changing tidal deformation of its (very slightly) elliptical orbit.
Io allegedly undergoes an interesting hysteresis loop; I'll try to find the seminal paper that describes this. The tidal forces and responses to it tend to make Io's orbit less eccentric. The resonant forces due to Io's orbital resonances with Ganymede and Europa tend to make Io's orbit more eccentric. Which predominates varies over time. the responses to the tidal forcing from Jupiter, or the response to the resonant forces? The answer is, it depends. When its eccentricity is very low, Io's inner core becomes more solid, thereby reducing the tidal energy losses, which are already low due to the low eccentricity. This enables Ganymede and Europa to dominate, making Io's orbit become more elliptic. At this point, the tidal forces start "kneading Io like bread", making the interior more liquid. Now the tidal forces dominate, making Io's orbit less eccentric and eventually making Io less active. Rinse and repeat. It's a very interesting hysteresis.

Ken G said:
But there are deeper issues here, because Io's orbit is less than 2 days, yet the orbit itself evolves on timescales longer than a year. So immediately we must wonder if the "kneading" is the 2-day effect of its eccentricity, or much longer timescale changes in the eccentricity. The reason the latter is relevant is that if we are dealing with longer variations than one orbit, how do we know the real heating that matter happens during much larger changes in its eccentricity over time, such that the current eccentricity plays almost no role at all in keeping Io volcanically active? (This paper: https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2019GL082691 suggests that volcanic eruptions do vary on the ~480 day period of orbital changes, but it leaves open the question of whether there are much longer period changes that are more important for keeping the moon's interior molten in the first place.)
 
  • #21
I have been wondering if it were possible for a practical student project to be constructed that might give some more insight on the problem. The idea is to take a smooth wooden ball of about 4 cm diameter. This is then turned into model Earth using “Plasticine” to roughly make the Earth’s main land-masses. A spindle is fitted into the Antarctic region so that the ball can be spun at a very slow rate to imitate the Earth’s rotation. A 1 cm. diameter neodymium powerful magnetic sphere is then used to represent the moon. Using an almost saturated solution of manganese chloride I have checked that if a blob of this solution is smeared over a surface that has been made quite hydrophilic, then by holding the magnet no more than about 3 or 4 mm above the smear one can see a small bulge of the very paramagnetic solution occurring at the point nearest to the magnet. ( I did also check out the effect of using a “ferrofluid” instead, but that turned out to be useless because it forms spikes of colloidal ferrite particles and therefore could not represent gravitational effects). So if the magnetic sphere is now fixed about 3 to 4 mm from the wooden ball’s surface and with the oceans marked out as smears of concentrated MnCl2 solution, then it would be interesting to witness the bulge changing as the ball is rotated. Getting the high natural surface tension of MnCl2 solution on the ball to be as low as possible will require surfactant to be added and the wooden ball to be treated with a thin film of hydrophilic polymer such as hardened gelatin or polyacrylamide, before the continents are added. Yes it is a bit of a mad idea but maybe worth a thought or two.
 
  • #22
I was just wondering about this and was thinking about the fact that gravity itself is not distributed equally around the globe. I wonder how much this would influence the sea level.
 
  • #23
Laroxe said:
I was just wondering about this and was thinking about the fact that gravity itself is not distributed equally around the globe. I wonder how much this would influence the sea level.
See https://en.wikipedia.org/wiki/Geoid.
 
  • #24
Unfortunately this Insight perpetuates two commonly repeated myths about Newton's work on tides, namely
  1. Newton believed that the time and height of tides at any particular location is determined by a 'tidal bulge'; and
  2. Newton was ignorant of, or ignored, observations of actual tidal variations.
Taking the second myth first, nothing could be further from the truth. In Book III of Principia he writes1:

"The force of the moon to move the sea is to be deduced from its proportion to the force of the sun, and this proportion is to be collected from the proportion of the motions of the sea, which are the effects of those forces. Before the mouth of the river Avon, three miles below Bristol, the height of the ascent of the water in the vernal and autumnal syzygies of the luminaries (by the observations of Samuel Sturmy) amounts to about 45 feet, but in the quadratures to 25 only. The former of those heights arises from the sum of the aforesaid forces, the latter from their difference. If, therefore, S and L are supposed to represent respectively the forces of the sun and moon while they are in the equator, as well as in their mean distances from the earth, we shall have L + S to L - S as 45 to 25, or as 9 to 5.​

At Plymouth (by the observations of Samuel Colepress) the tide in its mean height rises to about 16 feet, and in the spring and autumn the height thereof in the syzygies may exceed that in the quadratures by more than 7 or 8 feet. Suppose the greatest difference of those heights to be 9 feet, and L + S will be to L - S as 20½ to 11½, or as 41 to 23; a proportion that agrees well enough with the former. But because of the great tide at Bristol, we are rather to depend upon the observations of Sturmy; and, therefore, till we procure something that is more certain, we shall use the proportion of 9 to 5."​

Newton's access to data was not limited to observations around the coast of England: again in In Book III of Principia he addresses the anomalous tides in the Qiongzhou Strait separating the island of Hainan from the mainland of what is now China2:

"Again it can come about that the tide will be propagated from the ocean through different channels to the same port, and it may pass faster by one channel than by another: in which case the same tide, divided into two or more arriving successively, may consist of new motions of different kinds... An example of all of which has been revealed from the observations of Halley's sailors at the port of Batsham in the kingdom of Tunquin, at the northern latitude of 20° 50'."​

Other unusual tides Newton mentions include what are now Khambhat, India (Cambaia), the Gulf of Martaban, Myanmar (Pegu), Mont Saint Michel and Avranches, France, and the Straits of Magellan, Chile. Newton did not make these observations himself of course: they were reported in meticulous detail by ships of the English navies.

From this it is clear that it was well understood by Newton (as it had been for many centuries) that tides at any particular location are determined by lateral flows of bodies of water, constrained as they are by the sides and floor of the channels and basins in which they flow, and he repeatedly pointed this out in his treatise, for example1 (my emphases):

...Moreover the force LM pulls the water down at the quadratures, and will make that descend as far as the syzygies; and the force KL draws the same water up at the syzygies, and stop the descent of this, and will make that ascend as far as the quadratures: unless in so far as the motion of flux and reflux of the water may be directed by the channel, and may be retarded a little by friction. (Book 1 Section XI Corollary 19)
...And hence the maximum height of the water can come about in the octants after the syzygies, and the minima in the octants after the quadrutures approximately; unless as it were the motion of rising or falling impressed by these forces, for the water to persist with a little daily motion, either by a force in place or by the hindrance of some channel it might have stopped a little quicker. (Book 1 Section XI Corollary 20)
... on all the shores of which the tide comes in for around two, three or four hours, except where the
motion propagated from the ocean depths may be retarded by shallow places as much as
five, six, or seven hours or more... Also all the motions are retarded by passing through channels, thus so that the maximum of all the tides, in certain straits and estuaries of rivers, shall be even as the fourth or fifth day after the syzygies... (Book 3 Section II PROPOSITION XXIV THEOREM XIX)

What was not understood before Newton was the underlying cause of these lateral flows. Most civilizations from the beginning of history, and probably before, had observed that it must have something to do with the Moon (although Kepler advanced the theory that it was the breathing of fish, and Galileo similarly ignored the evidence and argued that it was simply the rotation of the Earth), but without Newton's theory of gravity exactly how the Moon caused the tides was an impossible mystery.

In particular, the fact that (in most places) there are two complete high-low cycles for every Ed: orbit of the Moon 24 hour 50 minute rotation of the Earth underneath the Moon, defied explanation.

It was only through understanding, and quantifying, the differential gravitational force of the Moon according to its distance, that Newton was able to explain that the Moon's gravity pulls the ocean up from its floor when it is overhead, and at the same time pulls the ocean floor down from its surface on the opposite side of the Earth, tending to create a 'tidal bulge' towards which the body of the ocean must flow. But as shown above, he repeatedly stated that whilst this is the driving force causing tidal flows, the timing, height and direction of that flow at any particular location is determined by the topography of the ocean floor and land masses, the Coriolis force, and other factors..

References
  1. https://en.wikisource.org/wiki/Page:Newton's_Principia_(1846).djvu/456
  2. https://www.17centurymaths.com/contents/newton/book3s2.pdf

Further reading - free access subject to NERC free access policies

Further reading - non-free access
 
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  • #25
pines-demon said:
Is the Newtonian tidal bulge an approximation of Laplace dynamics theory of tides in some limit?

Edit: I mean if I just take the predominant mode or something like that does everything correspond with Newtonian theory?

Edit2: I felt that the article was missing a conclusion on key differences between the two models aside from Laplace's model being more realistic. Very interesting nonetheless!
The Newtonian tidal bulge can be seen as an approximation of Laplace's dynamic theory of tides in certain limits. When considering the predominant mode, the Newtonian theory aligns with the basic tidal forces described by Laplace. However, Laplace's model incorporates additional factors like the Coriolis effect and ocean basin resonances, making it more realistic and comprehensive. The key difference is that Laplace's model accounts for the dynamic response of the ocean to tidal forces, while the Newtonian model is a simpler, static approximation2.

1.Beyond the Tidal Bulge 2. Laplace’s dynamic theory of tides 3. Tide Dynamics
 
  • #26
mentalhealth said:
The Newtonian tidal bulge can be seen as an approximation of Laplace's dynamic theory of tides in certain limits. When considering the predominant mode, the Newtonian theory aligns with the basic tidal forces described by Laplace. However, Laplace's model incorporates additional factors like the Coriolis effect and ocean basin resonances, making it more realistic and comprehensive. The key difference is that Laplace's model accounts for the dynamic response of the ocean to tidal forces, while the Newtonian model is a simpler, static approximation2.

1.Beyond the Tidal Bulge 2. Laplace’s dynamic theory of tides 3. Tide Dynamics
This is how I thought of it but I am getting mixed vibes. Every time I read a "there is no bulge" article it fails to say that it is still a valid approximation and treats the Newtonian bulge as complete fiction. We do not discard classical mechanics because special relativity exists. We just have to be clear on the limitations of the approximation.
 
  • #27
pines-demon said:
This is how I thought of it but I am getting mixed vibes. Every time I read a "there is no bulge" article it fails to say that it is still a valid approximation and treats the Newtonian bulge as complete fiction. We do not discard classical mechanics because special relativity exists. We just have to be clear on the limitations of the approximation.
Thanks for sharing. It's important to remember that scientific models like the Newtonian bulge are valuable approximations. Even with more accurate theories like special relativity, classical mechanics remains useful for many practical purposes. We should acknowledge the limitations of these approximations without dismissing their utility.
 
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  • #28
Laroxe said:
I was just wondering about this and was thinking about the fact that gravity itself is not distributed equally around the globe. I wonder how much this would influence the sea level.

pbuk said:
One of the most interesting applications, as pointed to by pbuk's reference, is that we have been able to derive modern global bathymetry maps with global coverage from satellite altimeters.
 
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