KurtLudwig said:
Then each day, there will be two high tides due to the moon and, in addition, there will be two lower high tides due to the sun at a different phase. But we only observe about two high tides and two low tides each 24 hours.
That's not how you add up amplitudes. The wiki article explains this comprehensively, with animations and graphs. I'm not sure what more you'd like us to tell you to make it understandable other than to point to places in the article.
This is how various components add up:
As you can see in this example, despite six components in total, of different phases, amplitudes, and periods, the end result is still two high and two low.
This animation shows how the two principal components (solar and lunar) add up visually:
KurtLudwig said:
On the side facing away from the moon, the sea water will be still attracted to the moon but to a lesser extent. Gravity only attracts. This will result in a lower sea level. I think Wikipedia is incorrect in this very rare instance.
The wiki is not wrong - you just have a common misconception.
Look at this picture:
You start by noticing that the lines of gravitational force from a nearby massive body are not parallel (1)
As long as you treat the body as completely rigid, you only ever have to worry about the force on the centre of mass, expressed by Newton's law (2).
But since planets are not completely rigid, different parts of them will be deformed by relative differences in the strength and direction of the gravitational force (3). Parts closer to the massive body will be attracted more (F5) than the force on the centre of mass (F), parts farther will be attracted less (F4). Parts offset from the line connecting the centres of masses will be attracted in different directions (F2 & F3).
You can deduct the magnitude of the force vector acting on the centre of mass (F) from all other forces to find out the relative force w/r to the centre of mass of the planet. Since F>F4, the force resulting from deduction: F'=F4-F will be negative, i.e. it will be pulling away from the centre of mass. If you deduct F from F2 & F3, you'll end up with a component directed towards the CoM (roughly speaking).
If this weren't a semi-rigid planet, but a collection of loose particles, from the point of reference of the CoM, points 5 and 4 would be moving away due to the differences in the magnitude of acceleration, while points 2 and 3 would be moving closer due to the differences in direction.
If you repeat that process for all points on the surface, you end up with this picture (from wiki again):
KurtLudwig said:
Are you stating that the whole Earth deforms, with the sea bottom on the far side moving away from the moon? I tend to think that the sea water moves a little up, but is constrained by gravity, and moves mainly horizontally. I tend to think that the solid Earth does not deform much.
Since there is no such thing as a perfect rigid body, everything deforms. Parts that are more rigid deform less, parts that are more fluid deform more.
The crust deforms by centimetres, the oceans by metres, the atmosphere by kilometres.