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Here and Now Chapter 1. Where are You? To find our place among the stars, we will zoom out from a familiar scene, to the largest scales in the universe.

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Presentation on theme: "Here and Now Chapter 1. Where are You? To find our place among the stars, we will zoom out from a familiar scene, to the largest scales in the universe."— Presentation transcript:

1 Here and Now Chapter 1

2 Where are You? To find our place among the stars, we will zoom out from a familiar scene, to the largest scales in the universe. From each frame to the next, we zoom out by about a factor 100.

3 A Campus Scene 16 x 16 m

4 A City View 1 mile x 1 mile

5 The Landscape of Pennsylvania 100 miles x 100 miles

6 The Earth Diameter of the Earth: 12,756 km

7 Earth and Moon Distance Earth – Moon: 384,000 km

8 Earth Orbiting Around the Sun Distance Sun – Earth = 150,000,000 km

9 Earth Orbiting Around the Sun (2) In order to avoid large numbers beyond our imagination, we introduce new units: 1 Astronomical Unit (AU) = Distance Sun – Earth = 150 million km

10 The Solar System Diameter of Neptune’s orbit: Approx. 60 AU

11 (Almost) Empty Space Around Our Solar System Approx. 10,000 AU

12 The Solar Neighborhood Approx. 17 light years

13 The Solar Neighborhood (2) Approx. 17 light years New distance scale: 1 light year (ly) = Distance traveled by light in 1 year = 63,000 AU = 10 13 km = 10,000,000,000,000 km (= 1 + 13 zeros) = 10 trillion km Nearest star to the Sun: Proxima Centauri, at a distance of 4.2 light years

14 The Extended Solar Neighborhood Approx. 1,700 light years

15 The Milky Way Galaxy Diameter of the Milky Way: ~ 80,000 ly

16 The Local Group: Our Cluster of Galaxies Distance to the nearest large galaxies: several million light years

17 The Universe on Very Large Scales Clusters of galaxies are grouped into superclusters. Superclusters form filaments and walls around voids.


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