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  2. Earth's circumference is the distance around Earth. Measured around the equator, it is 40,075.017 km (24,901.461 mi). Measured passing through the poles, the circumference is 40,007.863 km (24,859.734 mi). Measurement of Earth's circumference has been important to navigation since ancient times.

  3. en.wikipedia.org › wiki › PosidoniusPosidonius - Wikipedia

    Posidonius calculated the Earth's circumference by the arc measurement method, by reference to the position of the star Canopus. As explained by Cleomedes, Posidonius observed Canopus on but never above the horizon at Rhodes, while at Alexandria he saw it ascend as far as 7½ degrees above the horizon (the meridian arc between the latitude of ...

  4. Posidonius calculated the Earth's circumference by observing the position of the bright star Canopus. He observed that the star could be viewed on, but never above, the horizon at Rhodes, while at Alexandria he saw it emerge clearly above the horizon.

  5. The procedure is to find the circumference of the earth at about 180,000 stades. difference in latitude between two places on the same meridian, measure the terrestrial distance between these places, and thus find the measure of 10 and of the whole circumference.

  6. May 1, 2017 · Posidonius attempted to calculate the circumference of the Earth by assuming the cities of Rhodes (Greece) and Alexandria (Egypt) were on the same meridian. He also thought that the star Canopus touched the horizon at Rhodes at a meridian altitude of 7 30' or V48 of the circumference of a circle at Alexandria.

  7. Posidonius used the stars to determine the earth's circumference. He observed that a given star could be seen just on the horizon at Rhodes. He then measured the star's elevation at Alexandria, Egypt, and calculated the angle of difference to be 7.5 degrees or 1/48th of a circle.

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