Notes on the study guide for Mr. Sepikas’ PCC Astronomy class.  Notes are taken from http://encyclopedia.tfd.com/ or wikipedia unless otherwise noted.

1. degrees, minutes, seconds

2. the astronomical unit

3. diurnal motion

4. the north celestial pole

5. zenith, celestial equator, ecliptic, meridian

6. cause of the seasons

7. the equinox and the solstice

8. precession

9. leap year

10. tropical and sidereal year

11. phases of the moon

12. solar and lunar eclipses

13. Eratosthenes and the size of the Earth

Eratosthenes knew that on the summer solstice at local noon in the Ancient Egyptian city of Swenet (known in Greek as Syene) on the Tropic of Cancer, the sun would appear at the zenith, directly overhead. He also knew, from measurement, that in his hometown of Alexandria, the angle of elevation of the Sun would be 1/50 of a full circle (7°12′) south of the zenith at the same time. Assuming that Alexandria was due north of Syene he concluded that the distance from Alexandria to Syene must be 1/50 of the total circumference of the Earth. His estimated distance between the cities was 5000 stadia (about 500 geographical or nautical miles). He rounded the result to a final value of 700 stadia per degree, which implies a circumference of 252,000 stadia. The exact size of the stadion he used is frequently argued. The common Attic stadion was about 185 m, which would imply a circumference of 46,620 km, i.e. 16.3% too large. However, if we assume that Eratosthenes used the “Egyptian stadion”^[1] of about 157.5 m, his measurement turns out to be 39,690 km, an error of less than 1%.^[2]

Although Eratosthenes’ method was well founded, the accuracy of his calculation was inherently limited. The accuracy of Eratosthenes’ measurement would have been reduced by the fact that Syene is not precisely on the Tropic of Cancer, is not directly south of Alexandria, and the Sun appears as a disk located at a finite distance from the Earth instead of as a point source of light at an infinite distance. There are other sources of experimental error: the greatest limitation to Eratosthenes’ method was that, in antiquity, overland distance measurements were not reliable, especially for travel along the non-linear Nile which was traveled primarily by boat. So the accuracy of Eratosthenes’ size of the earth is surprising.

Eratosthenes’ experiment was highly regarded at the time, and his estimate of the Earth’s size was accepted for hundreds of years afterwards. His method was used by Posidonius about 150 years later.

14. the difference between planets and stars

15. Newton’s Laws

16. Kepler’s Laws

17. The electromagnetic spectrum and the optical window

18. the speed of light

19. the meaning of temperature

20. the Kelvin scale

21. atomic spectra

22. emission, absorption, and continuous spectra

23. The Rutherford experiment and the discovery of the nucleus

24. refraction, reflection and dispersion

25. refracting telescopes and reflecting telescopes

26. Nicholas Copernicus

27. CCD’s

28. telescopes in space

29. Newton’s law of gravity

30. the difference between mass and weight

31. the atomic hypothesis

Astronomy Test 2 Study Guide

The following study guide is intended to provide a focus fro your reading and study. It is not intended to be

comprehensive. There may be questions on the test that are not covered by this guide and topics in the guide

that do not appear on the test. Some of the topics may require you to look them up in another book or an

encyclopedia in the school library.

1. size of the photosphere

2. solar granules

3. determination of the chemical composition of the sun

4. appearance of the solar spectrum

5. temperatures inside and on the Sun

6. know what the words photosphere, chromosphere, and core mean

7. why are sunspots dark

8. how do we know that the Sun rotates

9. what is stellar parallax

10. what is proper motion

11. what is the difference between absolute and apparent magnitude

12. what is meant by luminosity

13. what are spectral classes

14. know and understand the Hertzsprung-Russel diagram

15. what are binary stars and what do they tell us

16. what is the material between the stars

17. what is nuclear fusion

18. read the section on the Orion nebula

19. understand the formula E=mc²

20. what is the Pauli exclusion principle

21. what is electron degeneracy

22. what is a pulsar

Astronomy Test 3 Study Guide

The following study guide is intended to provide a focus fro your reading and study. It is not intended to be comprehensive. There may be questions on the test that are not covered by this guide and topics in the guide that do not appear on the test. Some of the topics may require you to look them up in another book or an encyclopedia in the school library.

1. Know the names of the planets and their correct sequence from the Sun.

2. Know the difference between the term terrestrial and Jovian planets.

3. Know how the masses of planets are determined.

4. Know what substances make up what are called in space sciences “ices”.

5. Know what fraction of the universe is made up of hydrogen and helium.

6. Understand the formation process of the solar system.

7. Know the age of the Earth.

8. Understand the process of chemical differentiation on the Earth.

9. Understand how earthquake waves give us information about the interior of the Earth.

10. What is plate tectonics and how does it explain the mid-Atlantic ridge

11. How did oxygen come to be in the atmosphere of the Earth.

12. How is the magnetic field of the Earth created.

13. Know the relationship between the rotational period of the moon and its orbital period.

14. What are the lunar Maria and what caused them.

15. What caused the craters on the Moon.

16. Understand the theory that best explains the origin of the Moon.

17. Understand what is a scarp on Mercury and what caused them.

18. Know the surface temperature on Venus in Fahrenheit and Kelvin temperature scales.

19. Understand the greenhouse effect and what chemical causes it.

20.What is the optical illusion that caused the apparent “canals on Mars”.

21.What is Olympus Mons.

22. What is the evidence for the existence of flowing water on Mars

23. Understand how Jupiter can emit more heat than it receives from the Sun.

24. What material is thought to be responsible for the large magnetic fields on Jupiter and

Saturn.

25. What are the names of the moon of Jupiter.

26. Understand the mechanism that causes the heating of Io.

27. What is the composition of Saturn’s rings.

28. Understand the Roche limit.

29. Understand the angle relationship between the spin axis of Uranus and the orbital

plane of Uranus.

31. Know the story of how the plane Neptune was discovered.

32. Know what Bode’s law is.

33. Know the location of the asteroid belt in the solar system.

34. Understand the experimental technique for finding the shapes of asteroids.

35. Know what comet nuclei are.

36. What governs the direction of a comet’s ion tail.

37. Understand how comets orbit the Sun. Are the orbit random or is there a pattern.

38. What is a “meteor shower” and why are they seen at predictable times of the year.

39. Understand the current thinking on the cause of the deaths of the dinosaurs.

The McDonalds had a farm and children had they three.
They taught them as they had been taught — from bell and classroom free.
They did not send them off to school, but taught them ‘neath a tree.

With a moo moo here, and an oink oink there, the knowledge seeds they sow.
From book and brook and fruit and flute they learn all one need know.
Their school is not called E – I – E, but E – I – E – I – O

–kt

*   Excellence In Education Homeschooling Resource Center