'Celestial pole' diaporamas de présentation

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself. 2.1 Patterns in the Night Sky. Our goals for learning:. What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we see depend on latitude and time of year?. What does the universe look like from Earth?.

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Observing the Universe for Yourself

Observing the Universe for Yourself. Patterns in the Night Sky. Our goals for learning:. What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we see depend on latitude and time of year?. What does the universe look like from Earth?.

828 views • 71 slides

Observing the Universe for Yourself

Observing the Universe for Yourself. Patterns in the Night Sky. Our goals for learning:. What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we see depend on latitude and time of year?. What does the universe look like from Earth?.

838 views • 71 slides

Motion in the Sky

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Spaceship Earth

Spaceship Earth. Our goals for learning :. How is Earth moving in our solar system? How is our solar system moving in the Milky Way Galaxy? How do galaxies move within the universe? Are we ever sitting still?. How is Earth moving in our solar system?.

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ASTR100 (Spring 2006) Introduction to Astronomy Discovering the Universe

ASTR100 (Spring 2006) Introduction to Astronomy Discovering the Universe. Prof. D.C. Richardson Sections 0101-0106. Celestial Sphere. Zenith : Point directly overhead. Horizon : Where the sky meets the ground. Celestial Sphere. North Celestial Pole : Point on

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The Age of Things: Sticks Stones and the Universe

The Age of Things: Sticks Stones and the Universe. Precession, Polaris, and the Pyramids of Egypt. http://cfcp.uchicago.edu/~mmhedman/compton1.html. Last Time: Calendars are the Key to Mayan History. Piedras Negras Stela 3, Drawn by Linda Schele. When calendrical information is unavailable,

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The Age of Things: Sticks Stones and the Universe

The Age of Things: Sticks Stones and the Universe. Precession, Polaris, and the Pyramids of Egypt. http://cfcp.uchicago.edu/~mmhedman/compton1.html. Last Time: Calendars are the Key to Mayan History. Piedras Negras Stela 3, Drawn by Linda Schele. When calendrical information is unavailable,

459 views • 36 slides

Indoor Preparation

Indoor Preparation. Plan the observing run. Select a mix of objects. Check your star maps. Know and keep your equipment together. Must have pencils, torch, paper, clipboard and clips. Eye patch. Outdoors. Start with an easy object.

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Chapter 2

Celestial Motions. Chapter 2. Fig. 2.1. The Celestial Sphere

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Chapter 2

Celestial Motions. Chapter 2. Fig. 2.1. The Celestial Sphere

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A100 Solar System

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The Scale of the Cosmos

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Happy Haunted Homeroom October 9, 2012

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Finding celestial objects in our night sky: Right Ascension Declination Local Time of Day

Finding celestial objects in our night sky: Right Ascension Declination Local Time of Day. Every star, cluster, nebula, galaxy, radio source, and quasar has a position in the night sky. All the Solar System objects - the Sun, the Moon, the other planets, asteroids, and comets have their

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Every star, cluster, nebula, galaxy, radio source, and quasar has a position

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The Celestial Sphere

The Celestial Sphere. Stars at different distances all appear to lie on the celestial sphere. The 88 official constellations cover the celestial sphere. Why do stars rise and set?. Earth rotates from west to east, so stars appear to circle from east to west. Our view from Earth:.

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The contribution of LLR data to the estimation of the celestial pole coordinates

2. 3. 1. Figure 4. (red : fitted parameters, blue : DX or DY). Figure 5. Figure 3. (red : fitted parameters, blue : DX or DY). (red : fitted parameters, blue : DX or DY). The contribution of LLR data to the estimation of the celestial pole coordinates.

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