How was the radius of Earth calculated?

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How was the radius of Earth calculated?
« on: 08/06/2010 08:30:02 »
Adnan Nasir asked the Naked Scientists:
How did scientists calculate the radius of the Earth and Sun?

What do you think?
« Last Edit: 08/06/2010 08:30:02 by _system »


Offline LeeE

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How was the radius of Earth calculated?
« Reply #1 on: 08/06/2010 18:16:32 »
Eratosthenes, c. 276 BC c. 195 BC, is believed to be the first person to calculate the circumference, and thereby the radius, of the Earth.


Eratosthenes calculated the circumference of the earth without leaving Egypt. Eratosthenes knew that on the summer solstice at local noon in the Ancient Egyptian city of Swenet (known in Greek as Syene, and in the modern day as Aswan) on the Tropic of Cancer, the sun would appear at the zenith, directly overhead. He also knew, from measurement, that in his hometown of Alexandria, the angle of elevation of the sun would be 1/50 of a full circle (712') south of the zenith at the same time. Assuming that Alexandria was due north of Syene he concluded that the distance from Alexandria to Syene must be 1/50 of the total circumference of the earth. His estimated distance between the cities was 5000 stadia (about 500 geographical miles or 800 km) by estimating the time that he had taken to travel from Syene to Alexandria by camel. He rounded the result to a final value of 700 stadia per degree, which implies a circumference of 252,000 stadia. The exact size of the stadion he used is frequently argued. The common Attic stadium was about 185 m, which would imply a circumference of 46,620 km, i.e. 16.3% too large. However, if we assume that Eratosthenes used the "Egyptian stadium"[8] of about 157.5 m, his measurement turns out to be 39,690 km, an error of less than 1%.

Once the radius of the Earth, and thereby its curvature was known, the distance to the Sun could be measured by parallax from two separated points on the Earth's surface (although in theory, you only need to know the baseline length between the two observation stations, this assumes that the two stations are on a flat surface.  Over the length of the baseline required though, the curvature of the Earth became significant and had to be allowed for).  Once the distance to the Sun was known, it was then just basic trigonometry to work out its absolute size from its apparent angular size.
...And its claws are as big as cups, and for some reason it's got a tremendous fear of stamps! And Mrs Doyle was telling me it's got magnets on its tail, so if you're made out of metal it can attach itself to you! And instead of a mouth it's got four arses!