stars, galaxies, and the universe

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Stars, Galaxies, and the Universe Instructor: Prof. Kaaret 702 Van Allen Hall philip-kaaret @ uiowa.edu Lectures: MWF 12:30 pm – 1:20 pm Lecture Room 1 Van Allen Hall Textbook: Universe: Stars and Galaxies, Second Edition, by Freedman and Kaufmann Lab book: Imaging the Universe by Mutel & Wilson

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Stars, Galaxies, and the Universe. Instructor: Prof. Kaaret 702 Van Allen Hall philip-kaaret @ uiowa.edu Lectures: MWF 12:30 pm – 1:20 pm Lecture Room 1 Van Allen Hall Textbook: Universe: Stars and Galaxies, - PowerPoint PPT Presentation

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Page 1: Stars, Galaxies, and the Universe

Stars, Galaxies, and the Universe

Instructor: Prof. Kaaret

702 Van Allen Hall

philip-kaaret @ uiowa.edu

Lectures: MWF 12:30 pm – 1:20 pm

Lecture Room 1 Van Allen Hall

Textbook: Universe: Stars and Galaxies,

Second Edition,

by Freedman and Kaufmann

Lab book: Imaging the Universe

by Mutel & Wilson

Page 2: Stars, Galaxies, and the Universe

Why study Astronomy?

From modern astronomy, we have our best answers, so far, to questions such as:

• How and where are the atoms in our bodies formed?

• Is there life anywhere else than on Earth?

• What is the history of the Universe and what will eventually happen to the Universe?

Page 3: Stars, Galaxies, and the Universe

Why study Astronomy?

• Astronomy allows us to understand our place in the cosmos.

• Astronomy also reveals objects that stretch the imagination such as black holes, exploding stars, and giant jets of matter larger than a galaxy but moving at the speed of light.

• Astronomy shows us that the Universe is comprehensible.

Page 4: Stars, Galaxies, and the Universe

How empty is the solar system?

• What fraction of the volume in the solar system (which we will take to be a sphere enclosing the orbit of Pluto) is taken up with solid stuff (the Sun, planets, asteroids, …)?

• Any guesses?

Page 5: Stars, Galaxies, and the Universe

Scale model solar system

• To try to address this question, we are going to build a scale model of the solar system.

• So, what is a scale model?

Page 6: Stars, Galaxies, and the Universe

A scale model …

1. is made out of plastic?

2. corresponds to a real object?

3. is a World War II airplane?

4. has the same proportions as a real object?

5. has the same colors as a real object?

Page 7: Stars, Galaxies, and the Universe

Scale models

• A scale model is a representation of a real object or set of objects in which all of the different parts of the model have sizes in the correct proportions to the real thing.

Page 8: Stars, Galaxies, and the Universe

Scale models

• For scale factor s, real dimension D

then model dimension d = sD

For example, with a scale factor

s = 1:50 = 1/50 = 0.02, an airplane with a

length of D = 36 feet becomes a model with

a length of d = 0.02*36 feet = 8.64 inches.

Page 9: Stars, Galaxies, and the Universe

Scale model solar system

• We need the measurements of the real solar system. For our purposes, we will limit this to the diameter and distance from the Sun for each planet.

Page 10: Stars, Galaxies, and the Universe

Solar system dataDiameter Distance from Sun

[meters] [meters]

Sun 1,392,700,000 0

Mercury 4,878,000 57,900,000,000

Venus 12,104,000 108,200,000,000

Earth 12,756,000 149,600,000,000

Mars 6,787,000 227,900,000,000

Jupiter 142,980,000 778,300,000,000

Saturn 120,540,000 1,427,000,000,000

Uranus 51,120,000 2,870,000,000,000

Neptune 49,530,000 4,497,000,000,000

Pluto 2,300,000 5,900,000,000,000

Page 11: Stars, Galaxies, and the Universe

The Sequence of Planets

• Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto

• My Very Excellent Mother Just Sent Us Nine Pizzas

Page 12: Stars, Galaxies, and the Universe
Page 13: Stars, Galaxies, and the Universe
Page 14: Stars, Galaxies, and the Universe

Scale model of solar systemScale factor s = 2:1,000,000,000,000 = 0.000000000002

Distance from Sun Scaled distance

meters meters

Sun 0 0.000

Mercury 57,900,000,000 0.116

Venus 108,200,000,000 0.216

Earth 149,600,000,000 0.299

Mars 227,900,000,000 0.456

Jupiter 778,300,000,000 1.557

Saturn 1,427,000,000,000 2.854

Uranus 2,870,000,000,000 5.740

Neptune 4,497,000,000,000 8.994

Pluto 5,900,000,000,000 11.800

Page 15: Stars, Galaxies, and the Universe

Scale model of solar systemScale factor s = 2:1,000,000,000,000 = 0.000000000002

Diameter Scaled diameter

meters meters

Sun 1,392,700,000 0.002785

Mercury 4,878,000 0.000010

Venus 12,104,000 0.000024

Earth 12,756,000 0.000026

Mars 6,787,000 0.000014

Jupiter 142,980,000 0.000286

Saturn 120,540,000 0.000241

Uranus 51,120,000 0.000102

Neptune 49,530,000 0.000099

Pluto 2,300,000 0.000005

Page 16: Stars, Galaxies, and the Universe

Scale model of solar system

• To fit the solar system into the classroom, we scaled the orbit of Pluto to 11.8 meters = 38.7 feet

• Sun is the size of a match head

• Jupiter is smaller than a grain of salt

• Earth has the diameter of a strand of hair

Page 17: Stars, Galaxies, and the Universe

Course information• Website:

http://phobos.physics.uiowa.edu/~kaaret/sgu_s05• Survey of modern astronomy, conceptual approach• Course covers

– Night sky, moon, eclipses– Sun, stars– Black holes, neutron stars– Galaxies– Cosmology– Search for extra-solar planets, intelligence

• Does not cover solar system in detail

Page 18: Stars, Galaxies, and the Universe

PRS (Personal Response System)

• We will be using a student feedback technology called PRS during most lectures.

• PRS transmitters (looks like a TV remote) with an individual code are sold in a package with the textbook.

• Every student must have a PRS unit and bring it to class.

Page 19: Stars, Galaxies, and the Universe

Course information

• Some math will be needed– Simple algebraic equations– Plugging numbers into equations– Understanding powers of ten– Simple geometry

• Students will be expected to observe the sky– At least one hour per week– The only way to get extra credit is via

supervised observing on the roof of Van Allen Hall during clear week nights

Page 20: Stars, Galaxies, and the Universe

Course information

• Laboratory – If you are registered for 4 s.h., you are

already assigned to a weekly laboratory section.

– Laboratory sessions start next week.– Observing with a research-grade optical

telescope in Arizona (Rigel telescope). You will be using this facility for a research project in the second half of the semester.

Page 21: Stars, Galaxies, and the Universe

Grading• The course grade (letter grade will include +/- grading)

will be determined by the sum of points accumulated during the semester. The total possible points are given in the table below. The only way to get extra credit is by supervised observing on the roof of Van Allen Hall.

One-hour exams (4 total, highest 3 counted), 80 pts each

240

Final exam 160

Total 400