Okay, Penguin, I'll leave alone lunar eclipses right now since I can't seem to convince you that the power of prediction pretty much means that RE'es are right. Ignoring that, let's bring up something else I brought up in my initial post. All of the time, we see the same side of the moon, however, because the speed at which the moon is orbiting doesn't quite equal the rate that we're spinning at to meet it, there are some variances in this.
These are called librations. It is only a slight variance, however, it does allow us to see a bit of what is called the "dark side of the moon". Now, if the moon was flat as FE'ers profess, how come the moon does not become oblong when it librates. After all, if you turn a circle a little bit away from you, it appears to become more elliptical in shape. How do you explain this?
If you have never noticed this before, there is a picture in one of Ubuntu's posts on page twelve that has a sped up rendition of the moon waxing and waning. You can see the moon "wobble" a little bit in this short movie. That is because it is librating. However, during the entire "film", the moon stays a sphere. How do you explain this?