find your galactic address lecture 1.1 the scale of the cosmos

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Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

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Page 1: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

• Find your Galactic Address• Lecture 1.1 The Scale of the Cosmos

Page 2: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

• Astronomy deals with objects on a vast range of size scales and time scales.

• Most of these size and time scales are way beyond our every-day experience.

• Humans, the Earth, and even the solar system are tiny and unimportant on cosmic scales.

Page 4: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Now… we’ll check your answers… Lecture 1.1

• Journey through the vast range of scales in the Universe.

From each image to the next we are zooming out by a factor of 100.

Page 5: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

• Marco Polo journeyed east and Columbus west.

• You will travel outward away from your home on Earth; out past the moon, sun, and other planets; past the stars you see in the evening sky; and past billions more that can be seen only with the aid of the largest telescopes.

Page 6: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

• You live on a small planet circling a small sun drifting through the universe.

• Astronomy can take you beyond these boundaries and help you not only see where you are in the universe but understand what you are.

• To understand you must consider the word: SCALE– You have a right to know these things. – Perhaps, you have a duty to know them.

Page 7: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Scale of Universe• Our sense of

the Universe has changed over the years:

Page 8: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

• Each successive picture in the powerpoint will show you a region of the universe that is 100 times wider than the preceding picture.– That is, each step will widen your field of

view—the region you can see in the image—by a factor of 100.

Page 9: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

16 x 16 m

A Campus Scenesomething familiar

Page 10: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

A City View

Your field changes by a factor of 100

16 m x 16 m1 mile x 1 mile1.609 km x 1.609 km

Page 11: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

The Landscape of Pennsylvania

The photo in the figure is 1 mile in diameter.A mile equals 1.609 kilometers.So, you can see in the photo that a kilometer is a bit over two-thirds of a mile—

1 mile x 1 mile1.609 km x 1.609 km

100 miles × 100 miles160 km x 160 km

Page 12: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Diameter of the Earth: 12,756 km

The Earth

100 miles × 100 miles160 km x 160 km

The Allegheny Mountains of southern Pennsylvania cross the image in the upper left. The Susquehanna River flows southeast into Chesapeake Bay.What look like white bumps are a few puffs of cloudsThis is an infrared photograph in which healthy green leaves and crops show up as red. Human eyes are sensitive to only a narrow range of colors.

Page 13: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Earth–Moon distance: 384,000 km

Earth and Moon

At the next step in your journey, you will see your entire planet—which is 12,756 km in diameter.

• Earth rotates on its axis once a day, exposing half of its surface to daylight at any particular moment.

• The photo shows most of the daylight side of the planet.

• The blurriness at the extreme right is the sunset line.

• The rotation of the planet causes the cycle of day and night

• Rotation of the earth is eastwards

Page 14: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Sun–Earth distance: 150,000,000 km

Earth Orbiting around the SunEarth is the small blue dot in the center.The moon—whose diameter is only one-fourth that of Earth—is an even smaller dot along its orbit 380,000 km from Earth.

Page 15: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Earth Orbiting around the Sun

In order to avoid large numbers beyond our

imagination, we introduce new units:

1 astronomical unit (AU)

= Sun–Earth distance =

150 000 000 km

150 million km

Page 16: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

– This is nothing more than a simple way to write numbers without writing lots of zeros.

– In scientific notation, you would write 380,000 as ______________.

– The universe is too big to discuss without using scientific notation.

Page 17: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Approximately 100 AU

The Solar SystemLike Earth, Venus and Mercury are planets—small, non-luminous

bodies that shine by reflected light.

1 AU

Page 18: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Approximately 10,000 AU

(Almost) Empty Space Around our Solar System

Page 19: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Our Solar System to Scale

Page 20: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Approximately 17 light years

The Solar NeighborhoodThere are not any stars visible except for the sun.

The sun is a fairly typical star, and it seems to be located in a fairly average neighborhood in the universe. Although there are many billions of stars like the sun, none is close enough to be visible in the diagram— which shows an area only 11,000 AU in diameter.

Page 21: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

 In other words, light from Alpha Centauri takes 4.2 years to reach Earth.

New distance scale:

1 light year (ly) =

distance traveled by light in 1 year

= 63,000 AU = 1013 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

Approximately 17 light years

These stars are so distant that it is not reasonable to give their distances in astronomical units.

In the figure, the sizes of the dots represent not the sizes of the stars but their brightness. Bright stars make larger spots on a photo than faint stars. The size of a star image in a photo informs you not how the star is but only how bright it looks.

Page 22: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Approximately 1,700 light years or 1 million

The Extended Solar Neighborhood

Approximately 17 light years

Page 23: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Diameter of the Milky Way: ~75,000 ly

The Milky Way Galaxy

Most stars are concentrated in spiral arms

A galaxy is a great cloud of stars, gas, and dust bound together by the combined gravity of all the matter. Galaxies range from 1,500 to over 300,000 ly in diameter and can contain over 100 billion stars.

Page 24: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Distance to the nearest large galaxies: several million light years

The Local Group of Galaxies a common grouping of galaxies

Page 25: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Clusters of galaxies are grouped into superclusters.Superclusters form filaments and walls around voids.

Superclusters: a group of clusters The superclusters are linked to form long filaments and walls outlining voids that seem early empty of galaxies. These appear to be the largest structures in the universe.

Page 26: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

3 Conclusions:1. The solar system is the sun and its

planets.

2. The galaxy contains billions of stars and whatever planets orbit around them.

3. The universe includes everything—all the galaxies, stars, and planets, including our galaxy and our solar system.

Page 27: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

A Flight Through the Universe

• Explanation: What would it be like to fly through the universe? Possibly the best simulated video of this yet has been composed from recently-released galaxy data from the Sloan Digital Sky Survey. Every spot in the above video is a galaxy containing billions of stars. Many galaxies are part of huge clusters, long filaments, or small groups, while expansive voids nearly absent of galaxies also exist. The movie starts by flying right through a large nearby cluster of galaxies and later circles the SDSS-captured universe at about 2 billion light years (a redshift of about 0.15) from Earth. Analyses of galaxy positions and movements continues to bolster the case that our universe contains not only the bright matter seen, like galaxies, but also a significant amount of unseen dark matter and dark energy.

http://www.youtube.com/watch?feature=player_embedded&v=08LBltePDZw

http://apod.nasa.gov/apod/ap120813.html

Page 28: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Use your notes- answer on an index card

A quick review

Page 29: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

1. How is a planet different than a star?

1. Planets are larger than stars.

2. Planets reflect light while stars produce their own light.

3. Stars move faster in the sky than planets.

4. Planets are brighter than stars.

Page 30: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

2. The average distance from Earth to the sun is 1 AU.

1. True

2. False

Page 31: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

3. A light-year is the distance light travels in one year.

1. True

2. False

Page 32: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

4. A typical galaxy like our Milky Way galaxy contains

1. primarily planets.

2. gas only.

3. stars (some with planets), gas and dust.

4. a single star and planets.

5. thousands of superclusters.

Page 33: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

5. Which sequence is correct when ordered by increasing size?

1. Earth, Solar System, Milky Way Galaxy, clusters of galaxies

2. Solar System, Earth, galaxy clusters, Milky Way Galaxy

3. Earth, Milky Way Galaxy, Solar System, galaxy clusters

4. Galaxy clusters, Solar System, Milky Way Galaxy, Earth

Page 34: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

6. The sun is a star in the Milky Way Galaxy.

1. True

2. False

Page 35: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

7. A supercluster refers to a large group of stars within the Milky

Way.

1. True

2. False

Page 36: Find your Galactic Address Lecture 1.1 The Scale of the Cosmos

Answers

1. 2

2. 1

3. 1

4. 3

5. 1

6. 1

7. 2