SLIDE 2 Aristarchus of Samos (310-230 BC)
He created the first heliocentric cosmology; that is, he was the first to propose that the Earth, and the other planets, went around the Sun. 1,750 years later Copernicus will claim the credit. Aristarchus is also famous for devising a way of measuring the size of the moon in terms of the size of the Earth. Hipparchus later used this to conclude that the moon had about
- ne quarter the radius of the Earth (modern value 0.27) and that
its distance was about 60 Earth radii away (modern value 60.4). However, his calculations did not give absolute values; only those relative to the unknown radius of the Earth. Aristarchus also measured the relative distances of the Sun and
- Moon. He underestimated that badly, but even so realised that the
Sun was bigger than the Earth.
Eratosthenes (276 - 195 BC)
Measured the circumference of the Earth with amazing accuracy. He did so with a particularly powerful piece of observational technology, namely a long stick.
Hipparchus (190 - 120 BC)
Powerful insights into many aspects of
- astronomy. Invented the magnitude scale,
worked out the size of the moon, developed star and eclipse catalogues. Perfected the geocentric model with epicycles. It will go unchallenged for 1300 years.
Ptolemy (~85 - 165 AD)
Ptolomey’s revised epicycle mode See also http://astro.unl.edu/naap/ssm/animation s/ptolemaic.swf
Nicolaus Copernicus (1473-1543)
Credited with the heliocentric model of the Solar System. He divided the planets into the `inferior’ ones closer to the Sun than the Earth, and the `superior’
- nes outside the Earth’s orbit.
Only planets out to Saturn were known at that time. The orbits were all taken as circular.
Finally we shall place the Sun himself at the centre of the Universe. All this is suggested by the systematic procession of events and the harmony of the whole Universe, if only we face the facts, as they say, `with both eyes open'.
Nicolaus Copernicus