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Published byAlan Walters Modified over 9 years ago
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Stars and star names
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88 official constellations
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α alpha i iota ρ rho β beta κ kappa σ sigma γ gamma λ lambda τ tau δ delta μ mu υ upsilon ε epsilon ν nu φ phi ζ zeta ξ xi χ chi η eta ο omicron ψ psi θ theta π pi ω omega Constellation Possessive Aries Arietis Taurus Tauri Gemini Geminorum Cancer Cancri Leo Leonis Virgo Virginis Libra Librae Scorpius Scorpii Sagittarius Sagittarii Capricornus Capricornii Aquarius Aquarii Pisces Piscium
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Betelgeuse = - Orionis = HIP 27989 = etc…. Mintaka = - Orionis = HIP 29530 = etc…..
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Objects move daily across the sky. Why?
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North pole (Right hand rule) Because we live on a ball that’s spinning!
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Because we live on a ball that’s spinning: N up E WRise in the East
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because we live on a ball that’s spinning: up N E
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N N E W Sets in the West
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So, everything appears to move from east to west. (On a daily basis)
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Two kinds of day! Solar day: The time it takes the earth to rotate once with respect to the sun. Trouble: The solar day changes with the time of the year!
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Mean Solar day: The average of the solar day over a year. Our clocks measure mean solar time (MST): 1 hour = 1/24 th of a mean solar day 1 min = 1/60 th of an hour 1 sec = 1/60 th of a min
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Sidereal Day: time between a star’s meridian crossings 1 sidereal day = 23 hr 56 min and 4.091 sec (MST) If the sidereal day is constant, why not use it to calibrate our watches? sidereal day also divided up into hour, minutes, sec (sidereal)
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The Celestial Sphere
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We can think of all these stars as fixed on a big celestial sphere C.S. fixed Earth spins towards East OR …
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We can think of all these stars as fixed on a big celestial sphere Earth fixed C.S. spins towards West
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What we see from our specific locale
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The natural (local) way: Apparent S Horizon Apparent N Horizon Zenith N pole S pole Apparent horizons depend on your height, mtns etc …
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The natural (local) way: Zenith N pole S pole ‘True’ (local) horizon
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celestial N pole celestial S pole celestial equator celestial sphere rotates Polaris
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celestial N pole celestial S pole celestial equator local horizon zenith Earth’s equator latitude
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celestial N pole celestial S pole celestial equator local horizon Make Earth very small (Since everything is so far away!) zenith latitude Polaris latitude
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local horizon
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celestial N pole celestial S pole celestial equator local horizon celestial sphere rotates (instead of the earth) Motions of the stars relative to the fixed earth!
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celestial N pole celestial S pole celestial equator local horizon zenith Blue area is below observer’s horizon
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon zenith
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celestial N pole celestial S pole celestial equator local horizon Circumpolar!
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celestial N pole celestial S pole local horizon: observer at earth’s equator Observer’s zenith No circumpolar
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celestial N pole celestial S pole local horizon: observer at 45˚ N Observer’s zenith
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celestial N pole celestial S pole local horizon: observer N pole zenith All circumpolar
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Putting the sun’s position on the celestial sphere (The ecliptic) Earth’s tilted by 23 ½ °
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Sun’s daily motion Sun’s yearly motion on celestial sphere
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The seasons Earth’s tilted by 23 ½ ° Relative to the plane of its orbit around the sun
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Axis always points in the same direction (celestial N pole)
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celestial N pole (N) summer solstice ≈ June 21
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celestial N pole Equinox: (N) Autumn (Autumnal) ≈ September 22 (N) Spring (Vernal) ≈ March 21
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celestial N pole (N) winter solstice ≈ December 21
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Why is winter cold and summer hot?
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“Precession of the equinox”
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The Earth isn’t a perfect sphere! Non-zero torque from sun and moon!
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Spinning objects subjected to a torque precess!
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Precession of the North celestial pole.
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