0: the universe over time
DESCRIPTION
This introduction to our course draws an illustration of how our understanding evolves over time and with it, how we see the universe.TRANSCRIPT
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The Human Cosmos
in powers of ten
0
10 km
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< 500 BC Ancient World
10 km ?
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200 BC Greek Astronomy
4.5 million km
Aristarchus - estimates relative distances and size of earth,
moon and sun from watching the shadow of the earth on the
moon during eclipse.
Eratosthenes - measured the size of the earth from the angle
the sun cast on a well at summer solstice (6100 km vs 6378
km).6
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14th CenturyIbn al-Shatir141 million km
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Stronger
geometric
proofs revise
the estimates of
the distance to
the sun
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Tycho Brahae
the 1572 supernova
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Copernican system
the orbit of Saturn
1.52 x 109 miles
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1780 Herschelestimates size of the Milky Way by counting
stars in each direction
9000 light years
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1838 - Friedrich BesselMeasures distance to nearby stars by
Parallax
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More accurate size of Milky
Way
91,500 light years
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1923 Edwin Hubble “Nebulae” are other galaxies
Andromeda Galaxy
2,900,000 light years
Discovery of the expansion of space
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Hubble constant (H)
Shows Universe is Expanding1/H 13 billion light years
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Most distant Galaxies
1975 Dark Matter13 billion light years
1995 Hubble Telescope
Deep Field Pictures
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2002 Acceleration of universal expansion
Dark Energy15,000,000,000 light years
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