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An Earth Day Sidereal Day: 23 hr 56 min 4 sec Motion relative to background stars Mean Solar Day: 24 hours The average time between meridian crossings.

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Presentation on theme: "An Earth Day Sidereal Day: 23 hr 56 min 4 sec Motion relative to background stars Mean Solar Day: 24 hours The average time between meridian crossings."— Presentation transcript:

1 An Earth Day Sidereal Day: 23 hr 56 min 4 sec Motion relative to background stars Mean Solar Day: 24 hours The average time between meridian crossings of the Sun Apparent Solar Day: varies The actual time between the meridian crossings of the Sun

2 Solar vs. Sidereal Day

3 Lunar Month Synodic month: days. Defined by the period of the phases. Sidereal month: days. Defined by the motion relative to the stars. Anomalistic month: days. Defined as time between perigees.

4 Synodic vs. Sidereal Month

5 An Earth Year Julian Year: mean solar days. Used in calendars before 1582. Gregorian Year: mean solar days. Used in calendars today. Sidereal Year: mean solar days. Defined by the motion relative to stars. Tropical year: mean solar days. Defined from equinox to equinox. Thus, related to the seasons.

6 Earth Orbits Sun

7 Definitions Zenith: The point on the sky that is directly overhead of the observer. Horizon: The great circle on the celestial sphere that is 90 degrees from the zenith Hour circle: The great circle through the position of a celestial body and the celestial poles Meridian: The hour circle that passes through the zenith and both celestial poles

8 Directions on the Local Sky
Altitude: The minimum angular distance between the position of a celestial body and the horizon Azimuth: The angular bearing of an object, measured from North (0 degrees) through East (90 degrees), South (180 degrees), West (270 degrees), and back to North (360 degrees) Hour Angle: The angle between the meridian and an object’s hour circle (west is positive)

9 The Celestial Sphere

10 Celestial Coordinates
1 hour = 15 degrees Declination: The minimum angular distance from the position of a celestial body and the celestial equator Right Ascension: The eastward angle from the vernal equinox to the intersection of an object’s hour circle with the equator

11 Measuring Time Apparent Solar Time: The actual hour angle of the Sun + 12 hours (using 24-hour clock). Mean Solar Time: The hour angle of the average Sun + 12 hours Universal Time: Mean Solar Time at Greenwich, England Standard Time: Time assigned by time zone

12 Time Zones

13 Measuring Time Equation of Time: the difference between the apparent solar time and mean solar time Local Sidereal Time: Time measured by the position of the stars. Local Sidereal Time = Right Ascension of objects at the Merdian Local Sidereal Time = Right Ascension + Hour Angle


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