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© 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 2 Discovering the Universe for Yourself Mark Twain (1835 – 1910) American author, from.

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Presentation on theme: "© 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 2 Discovering the Universe for Yourself Mark Twain (1835 – 1910) American author, from."— Presentation transcript:

1 © 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 2 Discovering the Universe for Yourself Mark Twain (1835 – 1910) American author, from Huckleberry Finn We had the sky, up there, all speckled with stars, and we used to lay on our backs and look up at them, and discuss about whether they was made, or only just happened.

2 2.1 Patterns in the Night Sky What are constellations? How do we locate objects in the sky? Why do stars rise and set? Why don’t we see the same constellations throughout the year? Our goals for learning:

3 © 2005 Pearson Education Inc., publishing as Addison-Wesley What are constellations? A constellation is a region of the sky. 88 constellations determined by IAU in 1928

4 © 2005 Pearson Education Inc., publishing as Addison-Wesley Thought Question The brightest stars in a constellation… A.All belong to the same star cluster. B.All lie at about the same distance from Earth. C.May actually be quite far away from each other.

5 © 2005 Pearson Education Inc., publishing as Addison-Wesley The brightest stars in a constellation… A.All belong to the same star cluster. B.All lie at about the same distance from Earth. C.May actually be quite far away from each other.

6 The Celestial Sphere

7 © 2005 Pearson Education Inc., publishing as Addison-Wesley How do we locate objects in the sky? Locate an object by its altitude (above horizon) and direction (along horizon)

8 This doesn’t measure the absolute size! © 2005 Pearson Education Inc., publishing as Addison-Wesley We measure the sky in angles...

9 Angle measurements: Full circle = 360º 1º = 60 (arcminutes) 1 = 60  (arcseconds)

10 Why do stars rise and set? Earth rotates toward the east, so stars seem to rise in east and set in west Circumpolar Stars

11 Our view from Earth: Stars near the north celestial pole are circumpolar and never set. We cannot see stars near the south celestial pole from our location. All other stars (and Sun, Moon, planets) rise in east and set in west. Celestial Equator Your horizon

12 © 2005 Pearson Education Inc., publishing as Addison-Wesley Thought Question What is the arrow pointing to? A. the zenith B. the north celestial pole C. the celestial equator

13 © 2005 Pearson Education Inc., publishing as Addison-Wesley What is the arrow pointing to? A. the zenith B. the north celestial pole C. the celestial equator

14 Why don’t we see the same constellations throughout the year? 1.Depends on whether you stay home: Constellations vary with latitude. 2.Depends on time of year: Constellations vary as Earth orbits the Sun.

15 Review: Coordinates on the Earth Latitude: position north or south of equator Longitude: position east or west of prime meridian (runs through Greenwich, England)

16 The sky varies with latitude but not longitude.

17 altitude of the celestial pole = your latitude

18 © 2005 Pearson Education Inc., publishing as Addison-Wesley Thought Question The North Star (Polaris) is 50° above your horizon, due north. Where are you? A.You are on the equator. B.You are at the North Pole. C.You are at latitude 50°N. D.You are at longitude 50°E. E.You are at latitude 50°N and longitude 50°E.

19 © 2005 Pearson Education Inc., publishing as Addison-Wesley The North Star (Polaris) is 50° above your horizon, due north. Where are you? A.You are on the equator. B.You are at the North Pole. C.You are at latitude 50°N. D.You are at longitude 50°E. E.You are at latitude 50°N and longitude 50°E.

20 The sky varies as Earth orbits the Sun As the Earth orbits the Sun, the Sun appears to move eastward along the ecliptic. At midnight, the stars on our meridian are opposite the Sun the in the sky.

21 Special Topic: How Long is a Day? Solar day = 24 hours –Average time for sun to make one circuit through sky Sidereal day (Earth’s rotation period) = 23 hr, 56 min, 4.09 s Why the difference?

22 What have we learned? What are constellations? A region of the sky; every position on the sky belongs to one of 88 constellations. How do we locate objects in the sky? By its altitude above the horizon and its direction along the horizon.

23 What have we learned? Why do stars rise and set? Because of Earth’s rotation. Why don’t we see the same constellations throughout the year? The sky varies with latitude. The night sky changes as Earth orbits the Sun.


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