In most disciplines, finding the distance from one object to the next is, at least in theory, a simple operation. Not so in astronomy. While the size of Earth itself was determined with a fair degree of accuracy in ancient times, the scale of the solar system wasn’t fully understood until just a few centuries ago, and the distances to even the closest of stars wasn’t reliably determined until Friedrich Bessel measured the distance to 61 Cygni in 1838.

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Earth’s orbit is slightly elliptical, so astronomers make appropriate adjustments when applying the parallax method for real.

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There are some interesting historical reasons for the choice of 360 that lie beyond the scope of this article. A quick hint is to compare this to the number of days in a year.

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Tycho, the best observer before the invention of the telescope, cited angular measurements to a precision of 2 arcminutes.

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Always excepting the Sun, of course!

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And now you know the origin of the biggest astronomical gaffe in cinematic history. Han Solo should be ashamed of himself.

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See the activity under [supplementary material] under the References tab at TPT Online, http://dx.doi.org/10.1119/1.4976671 .

Supplementary Material

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