ASTR-1010 Lecture Notes - Lecture 4: Antarctic Circle, Solar Time, Hour Angle

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Chapter s2 celestial coordinates and motion in the sky. Celestial poles and equator correspond with earth"s poles and equator. Equinoxes and solstices are special points on the ecliptic. How to locate objects in the sphere each point corresponds to a location on the sphere. Right ascension longitude on the celestial sphere measured in hours east of the march equinox with the march equinox being 0 hours. Declination latitude on the celestial sphere measured in +/- degree above the celestial equator. Celestial coordinates of vega dec = +38 44" , ra = 18 h 35. 3 m. All objects with the same ra cross the meridian at the same time. Ra tells us how long after the march equinox we see the star/planet/celestial object. Sun"s declination negative in fall/winter and positive in spring/summer. Number of daylight hours varies by time of year: increase quickly in the spring, decreases quickly in the fall, stays nearly constant around the solstices.

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