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ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106
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ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Dec 19, 2015

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Page 1: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

ASTR100 (Spring 2008) Introduction to AstronomyDiscovering the Universe

Prof. D.C. RichardsonSections 0101-0106

Page 2: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How can we know what the universe was like in the past?

Thus, we see objects as they were in the past:The farther away we look in distance,

the further back we look in time.

Destination Light travel time

Moon 1 second

Sun 8 minutes

Sirius 8 years

Andromeda Galaxy 2.5 million years

Light travels at a finite speed (c = 300,000 km/s).

Page 3: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Example:

This photo shows the Andromeda Galaxy as it looked about

2½ million years ago. Question: When will be able to see what it looks like now?

M31, The Great Galaxy in Andromeda

Page 4: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Definition: A light-year

The distance light can travel in one year.

About 10 trillion km (6 trillion miles).

Distance = Speed x Time

= (300,000 km/s) x (1 yr) x (31,557,600 s/yr)

= 9,500,000,000,000 km!

= 9.5 x 1012 km

Page 5: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

• At great distances, we see objects as they were

when the universe was much younger.

Page 6: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

• Can we see the entire universe?

Page 7: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

A. Because no galaxies exist at such a great distance.

B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see.

C. Because looking 15 billion light-years away means looking to a time before the universe existed.

Why can’t we see a galaxy 15 billion light-years away?

(Assume the universe is 14 billion years old)

Page 8: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

A. Because no galaxies exist at such a great distance.

B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see.

C. Because looking 15 billion light-years away means looking to a time before the universe existed.

Why can’t we see a galaxy 15 billion light-years away?

(Assume the universe is 14 billion years old)

Page 9: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How do our lifetimes compare to the age of the universe?

The Cosmic Calendar: a scale on which we compress the history of the universe into 1 year.

New Year’s Day: The Big Bang

Milky Way forms

Sun & planets form

Oldest known life (single-celled)

First multi-cellular organisms

Page 10: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How do our lifetimes compare to the age of the universe?

The Cosmic Calendar: a scale on which we compress the history of the universe into 1 year.

Page 11: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Spaceship Earth

Page 12: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How is Earth Moving inOur Solar System?

The Earth rotates around its axis once every day.

Page 13: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

How is Earth Moving inOur Solar System?

The Earth orbits the Sun (revolves) once every year.

Page 14: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How is Earth Moving inOur Galaxy?

The Sun moves randomly relative to other nearby stars, and orbits the

galaxy once every 230 million years.

Page 15: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

More detailed study of the Milky Way’s rotation reveals one of the greatest mysteries in astronomy…dark matter!

Most of Milky Way’s light comes from disk and bulge …

…. but most of the mass is in its halo

Page 16: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How do Galaxies Move Within the Universe?

Galaxies are carried along with the expansion of the universe.

Page 17: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Part CThe following statements describe ways in which the analogy might apply to the real universe. Which statements are correct?

A. Both the raisin cake and the universe have a well-defined inside and outside. B. Raisin 1 is near the center of the cake, just as our galaxy is near the center of the universe. C. The temperature starts low and ends high in both the raisin cake and the universe. D. The raisins stay roughly the same size as the cake expands, just as galaxies stay roughly the same size as the universe expands. E. The average distance increases with time both between raisins in the cake and between galaxies in the universe. F¡. An observer at any raisin sees more distant raisins moving away faster, just as an observer in any galaxy sees more distant galaxies moving away faster.

Enter the letters of all correct statements in alphabetical order (without spaces). For example, if statements C and E are correct, enter CE.DEFCorrect

Like any scientific model, the raisin cake analogy has limitations, but it gives us a good overall picture of how the universe is expanding.

Page 18: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Are we ever sitting still? No!

Earth rotates on axis: > 1,000 km/hr

Earth orbits Sun: > 100,000 km/hr

Solar system moves among stars: ~ 70,000 km/hr

Milky Way rotates: ~ 800,000 km/hr

Milky Way moves in Local Group

Universeexpands

Page 19: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Patterns in the Night Sky

Page 20: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

What are constellations?

A constellation is a region of the sky.

88 constellations fill the entire sky (North & South).

Page 21: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Thought Question

The brightest stars in a constellation…

• all belong to the same star cluster.

• all lie at about the same distance from Earth.

• may actually be quite far away from each other.

Page 22: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

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.

Page 23: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

The Celestial Sphere

Stars at different distances all appear to lie on the celestial sphere.

The ecliptic is the Sun’s apparent path through the celestial sphere.

Page 24: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

The Celestial Sphere

Page 25: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

A band of light making a circle around the celestial sphere.

What is it?Our view into the plane of our galaxy.

The Milky Way

Page 26: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

The Milky Way

Page 27: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

How do we locate objects in the sky?

An object’s altitude (above horizon) and direction (along horizon) specify its location in your local sky.

Page 28: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

We measure the sky in angles...

blank

Page 29: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Angular Measurements

• Full circle = 360º

• 1º = 60 (arcminutes)

• 1 = 60 (arcseconds)

Page 30: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Thought Question

The angular size of your finger at arm’s length is about 1. How many arcseconds is this?

• 60 arcseconds.• 600 arcseconds.A. 60 60 = 3,600 arcseconds.

Page 31: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Thought Question

The angular size of your finger at arm’s length is about 1. How many arcseconds is this?

A. 60 arcseconds.B. 600 arcseconds.C. 60 60 = 3,600 arcseconds.

Page 32: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Why do stars rise and set?

Earth rotates west to east, so stars appear to circle from east to west.

Page 33: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

What moves? The Earth or the sky?

Page 34: ASTR100 (Spring 2008) 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

Page 35: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Celestial SphereNorth Celestial Pole: Point on celestial sphere above North Pole

Celestial Equator: Line on celestial sphere above Equator

Page 36: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Our view from Earth• Stars near the north celestial pole are circumpolar and never set.

• We cannot see stars near the south celestial pole.

• All other stars (and Sun, Moon, planets) rise in east and set in west.

Celestial equator

Your horizon

A circumpolar star never sets

This star never rises

Page 37: ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe Prof. D.C. Richardson Sections 0101-0106.

Ended Here 1/31/08

(lots of questions during lecture, plus organizational

stuff)