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This very parallax effect. We know how far the Sun is from the Earth, and the Earth has moved twice this distance from January 1 to July 1. This in turn allows us to extrapolate distance to some of the nearest stars by their apparent motion relative to the other, "fixed" stars.

https://en.wikipedia.org/wiki/Cosmic_distance_ladder

https://www.youtube.com/watch?v=7ne0GArfeMs




OK but then how do we know how far the sun is from the earth? Is it like "bounce a signal off it and count time of flight?"

(Another serious question.)


> The first rigorous and accurate scientific measurement of the Earth-Sun distance was made by Cassini in 1672 by parallax measurements of Mars. He and another astronomer observed Mars from two places simultaneously. A century later, a series of observations of transits of Venus provided an even better estimate.

http://curious.astro.cornell.edu/about-us/41-our-solar-syste...


We can't bounce signals off the sun, but we can do "interplanetary radar" bouncing signals off at least the nearby planets.

Knowing those distances, the distance to the sun becomes a trigonometry problem.


The video of Terence Tao I linked addresses that and many other questions about climbing the cosmic distance ladder.




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