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Chapter 1 Our place In The Universe Student information Sheets Semester: ______________________ Astronomy 105 Section ___________ Dr. Robert Friedfeld How To Access on-line Materials http://www.physics.sfasu.edu/ http://www.astronomyplace.com/ What is this lecture section? 001 002 003

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chapter 1

Chapter 1

Our place In The Universe

student information sheets
Student information Sheets

Semester: ______________________

Astronomy 105 Section ___________

Dr. Robert Friedfeld

how to access on line materials
How To Access on-line Materials

http://www.physics.sfasu.edu/

a modern view of the universe
A Modern View of the Universe
  • The sun, moon, planets and stars appear to circle around the earth.
  • We cannot feel the earth move, although it does.
  • It seems natural to place the earth at the center of everything (Geocentric model).
  • Today, we know that the earth is one of nine planets which orbits the Sun.
our cosmic address
Our Cosmic Address

~ 40 Galaxies

More than 100 billion stars

The Local Supercluster

our cosmic origins
Our Cosmic Origins

How did we come to be?

slide9

First let’s look at what we know.

  • Telescopic evidence points to an expanding universe.

From the observed rate of expansion, Astronomers estimate that the expansion began sometime between (12-16) billion years ago.

  • The universe as a whole continues to expand, but on smaller scales, gravity brings matter together to form galaxies and clusters of galaxies.
slide10

Our Cosmic Origins

Galaxies form a few billion years after the Big Bang

Star forms

A Region of Space Expands with time

Star explodes

Earth was made of elements produced in stars long ago.

Star shines

slide11
Within galaxies, gravity causes the collapse of clouds of gas and dust, forming stars and planets.
  • When stars die, they release much of their content back into interstellar space.
  • Galaxies function as cosmic recycling plants.
  • All elements heavier than H, He, and Li were manufactured by stars through nuclear fusion.
images of time
Images of Time
  • We study the universe by studying light from distant stars and galaxies.
  • The speed of light is 300,000 km/s.
  • This is fast enough to circle the earth 8 times in 1 second.
  • Light from stars can take many years to reach us.
  • We measure distances to the stars in Light-Years. (ly)
  • 1 ly is the distance light can travel in one year.
slide13
1 ly = 9.46 x 1012km (9.46 trillion km)
  • Because it takes time for light to travel through space, the farther away we look in distance, the further back we look in time. (Look back time)
  • The speed of light limits the portion of the universe that we can see.
slide14
Any picture of a distant galaxy is a picture of both space and time.
  • The Great Spiral Galaxy in Andromeda (aka M31)
    • lies about 2.5 million light-years from the earth.
    • A picture of the Galaxy taken now is a picture of how M31 looked about 2.5 million years ago.
    • The diameter of M31 is ~ 100,000 ly.
    • light from the far side of the galaxy took 100,000 years longer to reach us than the light from the near side.
slide15
The Great Spiral Galaxy in Andromeda (aka M31)
    • lies about 2.5 million light-years from the earth.
    • A picture of the Galaxy taken now is a picture of how M31 looked about 2.5 million years ago.
    • The diameter of M31 is ~ 100,000 ly.
    • light from the far side of the galaxy took 100,000 years longer to reach us than the light from the near side.
slide16

When we study the universe, it is impossible to separate space and time.

The Great Spiral Galaxy in Andromeda

100,000 ly

onward to the stars
Onward To The Stars
  • The nearest star system to our own is called Alpha Centauri.
  • It is approximately 4.4 ly from us.
the milky way galaxy and beyond
The Milky Way Galaxy and Beyond
  • How many stars are there in the visible universe?
slide23

Spaceship Earth

The Earth rotates on its axis once each day.

As the Earth rotates, your speed around the Earth’s axis depends on your latitude.

slide24

The Earth revolves around the Sun once each year.

The average distance of the earth from the Sun is called an astronomical unit or AU.

1AU = 150 million km = 93 million miles.

slide25

The plane of the Earth’s orbit around the Sun is called the ecliptic plane.

Axial Tilt of 23.5o

seasons
Seasons
  • The combination of Earth’s axial tilt, axial rotation and its revolution around the Sun explains why we have seasons.
spring vernal equinox
Spring (Vernal) Equinox
  • On about March 21 each year.
  • Both hemispheres receive equal amounts of sunlight.
  • Beginning of Spring in the Northern Hemisphere.
  • Beginning of Fall in the Southern Hemisphere.
summer solstice
Summer Solstice
  • On around June 21, the northern hemisphere receives its most direct sunlight.
  • The northern hemisphere has the longest period of daylight of any day of the year.
  • This is usually considered the first day of summer in the northern hemisphere.
  • The Southern Hemisphere receives its least direct sunlight.

and has its shortest period of daylight of any day of the year.

  • This is the first day of winter in the Southern Hemisphere.
fall autumnal equinox
Fall (Autumnal) Equinox
  • Occurs around September 21.
  • Both hemispheres receive the same amount of sunlight. but now the seasons are the reverse of the spring (Vernal) equinox.
  • In the Northern Hemisphere we have the beginning of Fall.
  • In the Southern Hemisphere we have the beginning of Spring.
winter solstice
Winter Solstice
  • Around December 21.
  • We have the reverse situation to that of the summer solstice.
  • It is usually considered the first day of winter for the northern hemisphere and the first day of summer for the southern hemisphere.
precession
Precession
  • The axis of the Earth will remain pointed toward Polaris throughout our lifetimes.
  • However, this has not always been the case and the direction will change again in the distant future.
  • The reason is a that the rotation axis of the Earth precesses - like a spinning top.
traveling in the milky way galaxy
Traveling in the Milky Way Galaxy
  • The local solar neighborhood is only a tiny portion of the Milky Way Galaxy.
  • The stars in the local solar neighborhood move quite fast relative to our solar system. (~ 70,000 km/h)
the entire milky way galaxy rotates
The Entire Milky Way Galaxy Rotates
  • Our Sun and solar system are located about 28,000 ly from the galactic center.
  • At this distance, each orbit around the galactic center takes about 230 million years.
edge on view of the milky way galaxy
Edge-On View of the Milky Way Galaxy.
  • Most visible stars reside within the galaxy’s thin disk.
  • Careful study of galactic rotation shows that most of the mass lies in the galactic halo.
  • Because this mass emits no light that we have detected, we call it dark matter.
the expanding universe
The Expanding Universe
  • When we look outside the local group of galaxies (remember, this is the group to which the Milky Way belongs.) we find two astonishing facts.
  • Virtually every galaxy outside the Local Group is moving away from us.
  • The more distant the galaxy, the faster it appears to be moving away from us.
  •  The entire universe is expanding