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- Powers of ten on the web: http://micro.magnet.fsu.edu/primer/java/scienceopticsu/powersof10/index.html
- Finish chapter 2 topics
- Magnitude Scale
- The Celestial Sphere
- Start chapter 3: Cycles in the Sky
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- From our Text, Horizons by Seeds
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- Imagine being in a rotating restaurant on top of a tall building. All
the outside objects are very far away – much farther than the distance
across the room.
- Paint the view on the windows – and keep the people near the center of
the room – away from the windows themselves.
- Can the people tell if the room is rotating, or if the painted windows
are just moving around the room?
- Which is more reasonable – a rotating room or rotating painted windows?
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- HORIZON: The horizontal circle
which separates the part of the sky visible to you and the part of the
sky hidden by the earth.
- ZENITH: The point on the sky
directly overhead.
- MERIDIAN: The circle which
starts on the northern horizon, runs through the zenith, continuing on
to the southern horizon. It
separates the eastern half of the sky from the western half.
- CELESTIAL POLES: The points where
the extension of the rotation axis of the earth would intersect the
celestial sphere.
- CELESTIAL EQUATOR: The circle
around the sky which would be a projection of the earth’s equator.
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- At the Earth’s north pole, looking overhead all stars appear to circle
around the north celestial pole.
- At the equator:
- Stars on the celestial equator rise in the east, move overhead, then
set in the west
- The N and S celestial poles are just on your N and S horizons, and
stars near those points still circle around them. But those stars are only visible for
the upper half of their circles.
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- Stars close enough to the north celestial pole are always above the
horizon, and just circle the pole star.
(CIRCUMPOLAR STARS)
- Stars on the celestial equator rise in the east, move higher along a
slanted path which crosses the “meridian” to the south of the zenith,
then descend and set due west.
- Stars far enough to the south never make it above the horizon.
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- The earth’s axis of rotation is tilted 23.50 relative to the
plane containing the sun and other planets.
- The gravity from the Sun and moon is trying to tip the earth just like
gravity is trying to tip a spinning top.
- As with the top, the axis of the earth wobbles or PRECESSES in space,
with a 26,000 year period.
- Because the directions to the celestial poles are defined by the spin
axis – those poles move with time.
- It isn’t that the stars move – it is that the grid we paint on the
celestial sphere has to be redrawn from time-to-time.
- Eventually Polaris will not be the “pole” star.
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- Plot position of Sun relative to stars, over one full year.
- Complicated by fact you can’t see Sun and stars at same time.
- Once you have full map of sky, you can work this out by seeing what
stars are opposite sun 12 hours later.
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- Seasons almost entirely due to TILT of Earth
- Seasons opposite (not the same) in N & S Hemispheres
- Earth’s orbit slightly elliptical
- Slightly closer to the sun in N. Hemisphere Winter
- But this changes as tilt precesses in 26,000 yr cycle
- Expect N. Hemisphere winter to be slightly milder
- Positions of continents and oceans actually more important
- Effect is important for Mars -- more elliptical orbit
- Cyclic variations in climate as tilt precesses (and tilt and ellipticity
also gets slightly larger and smaller
- VERY IMPORTANT TOPIC (Re: Global Warming)
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