TOPIC: [excerpt of] Calculate the distance to the Sun (where is the Sun?)

Your point being? Stick to the topic at hand. Have you tried to disprove the far easier to understand video that I posted, or is your math's not up to it?

Thinkers in Ancient Greece were among the first to try and construct a comprehensive model of the cosmos. With nothing but naked-eye observations, a few things could be worked out. The Moon loomed large in the sky so it was probably pretty close. Solar eclipses revealed that the Moon and Sun were almost exactly the same angular size, but the Sun was so much brighter that perhaps it was larger but farther away (this coincidence regarding the apparent size of the Sun and Moon has been of almost indescribable importance in advancing astronomy). The rest of the planets appeared no larger than the stars, yet seemed to move more rapidly; they were likely at some intermediate distance. But, could we do any better than these vague descriptions? With the invention of geometry, the answer became a resounding yes.

The first distance to be measured with any accuracy was that of the Moon. In the middle of the 2nd century BCE, Greek astronomer Hipparchus pioneered the use of a method known as parallax. The idea of parallax is simple: when objects are observed from two different angles, closer objects appear to shift more than do farther ones. You can demonstrate this easily for yourself by holding a finger at arm’s length and closing one eye and then the other. Notice how your finger moves more than things in the background? That’s parallax! By observing the Moon from two cities a known distance apart, Hipparchus used a little geometry to compute its distance to within 7% of today’s modern value – not bad!

Some truth seeker you are.

Yes, I';ve seen the thread. I thought some might want to hear his opinions on this whole non-spherical earth/close sun theory, even if you didn't. As I said, some truth seeker you are.