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The Sky

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The Sky

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  1. The Sky Edward M. Murphy Space Science for Teachers 2005 The Sky

  2. Horizon and Zenith • It is sometimes useful to think of the sky as a great dome over our heads. • The horizon is where the dome meets the Earth. • The zenith is the point directly overhead. • As the Earth turns, this dome turns over our heads. It appears as if the sky is a large hollow sphere centered on the Earth. The Sky

  3. Horizon and Zenith The Sky

  4. Altitude and Azimuth • The height of a star above the horizon is called the altitude. • The direction to the star as measured from true north is called the azimuth. • Note: True north is not the same as magnetic north. The magnetic north pole is not located in the same place as the true north pole. • On maps, the legend will show you how to correct from magnetic north, as measured by a compass, to true north. The Sky

  5. Altitude and Azimuth The Sky

  6. Magnetic North Pole The Sky

  7. Magnetic North The Sky

  8. Correction from Magnetic North to True North The Sky

  9. Altitude and Azimuth • The altitude and azimuth of a star change during the course of night as the star rises and sets. • Angles are measured using degrees, minutes of arc, and seconds of arc. The Sky

  10. Measuring Angles in the Sky The Sky

  11. Measuring Angles • Angles in astronomy are measured in degrees, arcminutes and arcseconds. • 1 degree = 60 arcminutes • 1 arcminute = 60 arcseconds • 1 degree = 3600 arcseconds • 1 arcsecond is the size of a U.S. quarter as seen from 5 km (3 miles) or a penny as seen from 2.2 miles. The Sky

  12. Measuring Angles • The Sun and Moon appear to be about ½ degree in size. • Your finger held at arms length is about one degree across. • Your fist at arms length is about 10 degrees. • Your outstretched hand at arms length is about 20 degrees across. The Sky

  13. Angular Sizes and Distances The Sky

  14. The Celestial Sphere The Sky

  15. The Celestial Sphere The Sky

  16. The Celestial Sphere • North Celestial Pole: The point directly over the Earth’s true north pole. • The north star, Polaris, is near the North Celestial Pole, but not exactly at the pole. It is currently about 1 degree away from the pole. • South Celestial Pole: The point directly over the Earth’s true south pole. • Celestial Equator: The equator of the Earth projected onto the celestial sphere. • Meridian: A line from due north to due south that passes straight overhead. The Sky

  17. Longitude and Latitude The Sky

  18. Longitude and Latitude • Latitude: Your north-south position on Earth. The equator is defined to have a latitude of 0o. The north pole is at 90oN and the south pole at 90oS. • Longitude: Your east-west position on Earth. An arbitrary point, the Prime Meridian in Greenwich, England marks a longitude of 0o. • Leander McCormick Observatory is at: • Longitude 78o 31’ 19.8” W • Latitude 38o 01’ 58.2” N • Altitude 264 meters The Sky

  19. Rotation of the Earth The Sky

  20. The stars move from east to west because the earth rotates from west to east. The Sky

  21. The Motion of the Stars • Just like the Sun and Moon the stars rise and set due to the rotation of the Earth. • They rise in the east and set in the west because Earth rotates from west to east. • Stars near the celestial poles do not rise or set. Instead they circle the poles and are called circumpolar. • In the northern hemisphere, the stars circle the pole in a counterclockwise direction. The Sky

  22. Daily (Diurnal) Motion of the Stars The Sky

  23. Circumpolar Stars The Sky

  24. Diurnal Paths of Stars The Sky

  25. Diurnal Paths of Stars The Sky

  26. Diurnal Paths of Stars at Intermediate Latitude The Sky

  27. Celestial Poles The Sky

  28. North Celestial Pole • In the northern hemisphere, the altitude of the north celestial pole is equal to your latitude on Earth. • This is useful for navigation. • If you measure the altitude of the north celestial pole, you can determine your latitude on Earth. • In the southern hemisphere, it is difficult, but not impossible, to find the location of the south celestial pole. The Sky

  29. Diurnal Paths of Stars at Intermediate Latitude The Sky

  30. Celestial Sphere • To find due north, drop straight down from the North Celestial Pole to the horizon. • The celestial equator meets the horizon at due east and due west. The Sky

  31. Diurnal Paths of Stars The Sky

  32. Celestial Sphere Movie The Sky http://brahms.phy.vanderbilt.edu/~rknop/astromovies/

  33. Celestial Coordinates • Just as Earth has lines of longitude and latitude, the celestial sphere has a system of celestial coordinates: • Declination (dec): The north-south position of a star on the celestial sphere. Declination is measured in degrees, arcminutes, and arcseconds. The celestial equator is defined to have a declination of 0o. • Right Ascension (RA): The east-west coordinates of an object on the celestial sphere. R.A. is measured in hours, minutes, and seconds of time. The vernal equinox is defined to be 0h. The Sky

  34. Celestial Coordinates The Sky

  35. Celestial Coordinates Vega RA 18h35m DEC +38o44’ The Sky

  36. The Sky

  37. The Sky

  38. The Sky

  39. Classroom Exercise • Find Orion in the night sky. Is it on the equator, the ecliptic, both, or neither. • How long is Orion above the horizon each day? • Find Sagittarius. Is it north or south of the equator? • How long is Sagittarius above the horizon each day? The Sky

  40. Classroom Exercise • Find Taurus. Is it north or south of the equator? • How long is it above the horizon each day? • Find the Sun on December 21. Which constellation is it in? How long is it above the horizon each day? • Find the sun on June 21. Which constellation is it in? How long is it above the horizon each day? The Sky