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RECAP Refractor and Reflector Lens Mirror The Celestial Sphere & more on Constellations (Week 4) Why do we see what we see?? 90 deg. 34 deg. Latitude Rotation Daily Changes Revolution Monthly Changes The Zodiac Constellations – the 88 semirectangular regions that make up the sky • Northern constellations have Latinized Greek-mythology names: – Orion, Cygnus, Leo, Ursa Major, Canis Major, Canis Minor • Southern constellations have Latin names: – Telescopium, Sextans, Pyxis What do you think? • What causes the stars to move? • Do the stars actually move in the way they appear from Earth? • Do the stars stay in the same position in the sky all day/night long? Consider the dome of the sky over our heads…. mixing bowl Consider the dome of the sky over our heads…. inverted mixing bowl …. Imagining a spinning Celestial Sphere surrounding Earth aids in thinking about the position and motion of the sky Animation of Celestial Sphere http://bcs.whfreeman.com/universe6e/pages/bcsmain.asp?v=category&s=00110&n=01000&i=02110.02&o =|02000|01000|&ns=0 Imagining a spinning Celestial Sphere surrounding Earth aids in thinking about the position and motion of the sky Altitude is like latitude or declination Celestial Sphere Rotation Celestial Sphere Rotation Star B Star B 2 2 Star A Star A 1 2 1 2 North Star Celestial Sphere Celestial Sphere 3 3 1 1 4 4 3 3 Horizon Earth’s Equator 4 4 Celestial Sphere Rotation Celestial Sphere Rotation Figure 1 Figure 2 1) Explain how to find North on the horizon from the North star. 2) Where is the North star when you’re at the North pole? 1) Is the horizon shown a real physical horizon, or an imaginary plane that extends from the observer and Earth out to the stars? Celestial Sphere Rotation Star B 2 Star A 1 2 Celestial Sphere 2) Can the observer shown see an object located below the horizon? Celestial Sphere 3 1 4 3 3) Is there a star that is in an unobservable position? 4)When a star travels from being below the observer’s horizon to being above the observer’s horizon, is that star rising or setting? 4 Celestial Sphere Rotation Figure 2 Horizon • • • • • • Tutorial: Position – p.1 PUT NAMES in Tutorials Work with a partner Read the instructions and questions carefully Talk to each other and discuss your answers with each another Come to a consensus answer you both agree on If you get stuck or are not sure of your answer ask another group If you get really stuck or don’t understand what the Lecture Tutorial is asking ask your Professor for help • I WILL BEGIN STAMPING TUTORIALS A LITTLE BEFORE YOU FINISH THE TUTORIAL SINCE THERE ARE 70+ OF YOU, BUT YOU MUST ALL FINISH THE TUTORIAL OR YOU WILL GET A ZERO! DO NOT WALK OUT OF THE ROOM OR GET OFF TASK WHEN WE ARE COMPLETING A TUTORIAL OR YOU WILL GET POINTS DEDUCTED OR GET A ZERO! • IF THE TUTORIAL IS COMPLETED AT THE END OF LECTURE, NO ONE IS ALLOWED TO LEAVE EARLY UNLESS YOU CHECK WITH ME FIRST! IF YOU LEAVE EARLY YOU’LL GET A ZERO. Did you get the Key Ideas from the Position Lecture Tutorial? Celestial Sphere Rotation Star B In what direction is the observer facing? 2 Star A 1 2 Celestial Sphere Celestial Sphere 3 1 4 3 4 A. B. C. D. toward the South toward the North toward the East toward the West Celestial Sphere Rotation Figure 2 Horizon Imagine that from your current location you observe a star rising directly in the east. When this star reaches its highest position above the horizon, where will it be? Celestial Sphere Rotation A. B. C. D. high in the northern sky high in the southern sky high in the western sky directly overhead Star B 2 Star A 1 2 Celestial Sphere Celestial 3 1 4 3 4 Celestial Sphere Rotation Figure 2 Horizon Celestial Sphere Rotation Where would the observer look to see the star indicated by the arrow? A. B. C. D. High in the Northeast High in the Southeast High in the Northwest High in the Southwest Star B 2 Star A 1 2 Celestial Sphere Celestial Sphere 3 1 4 3 4 Celestial Sphere Rotation Figure 2 Horizon Telescope Field of View Moon=0.5 deg. Field of View = Eyepiece apparent FOV ÷ Magnification Large Magnification = Small field of view Small Magnification = Large Field of view Right Ascension (RA) and Declination (Dec) are similar to latitude and longitude on the surface of the Earth. Latitude and longitude are fixed with respect to positions on Earth. But RA and Dec are fixed with respect to positions of stars in the sky. What is moving, the celestial sphere or the Earth? To an Earthling observer, what appears to move? Declination (like latitude) is measured in degrees north or south of the Celestial equator. Right ascension (like longitude) is measured in units of hours, minutes, and seconds eastward from the position of the vernal equinox on the Celestial equator. The Vernal Equinox is the position of the Sun on the first day of Spring.