Term
| 1.Our latitude can be found by measuring the |
|
Definition
| altitude of the North Celestial Pole (near Polaris) |
|
|
Term
| 2. The local celestial meridian passes through all of the following points on the celestial sphere except |
|
Definition
| the east point on the horizon |
|
|
Term
| 3. We call the point directly overhead the |
|
Definition
|
|
Term
| 4. The meter is used to measure |
|
Definition
|
|
Term
| 5. Which celestial body appears to cross the local celestial meridian about once/day due to diurnal motion |
|
Definition
| a star, a planet, sun, moon |
|
|
Term
| 6. Where on earth would the celestial equator pass through the zenith of an observer |
|
Definition
|
|
Term
| 7. What name do we give to the apparent path of the sun in the sky |
|
Definition
|
|
Term
| 8. The astronomical unit AU is equal to |
|
Definition
| the distance between the earth and the sun |
|
|
Term
| 9. The apparent paths of the stars in the night sky are easily pictured when the stars are imagined to live on an imaginary object called the |
|
Definition
|
|
Term
| 10. The point on the celestial sphere directly beneath the observer is know as the |
|
Definition
|
|
Term
| 11. A time exposure of the North Sky shows a circular pattern. The center of the circle is |
|
Definition
| exactly at the North Celestial pole |
|
|
Term
| 12. Where on the earth do objects in the sky appear to move in circular paths parallel to the horizon |
|
Definition
|
|
Term
| 13. The sun appears to move through the sky |
|
Definition
| about 1 degree eastward/day |
|
|
Term
| 14. The circle in the sky lies halfway between (or 90˚ from) the celestial poles and passes through the East and West points on the horizon. It is called the |
|
Definition
|
|
Term
| 15. The line in the sky which runs East to West and divides the sky into Northern and Southern hemispheres is called the |
|
Definition
|
|
Term
| 16. Much of the difficulty in studying celestial bodies arises from the large |
|
Definition
|
|
Term
| 17. The number 3.3X10 to the -3 power is equal to |
|
Definition
|
|
Term
| 18. The plane of the earth’s equator is inclined to the plane of its orbit at an angle of |
|
Definition
|
|
Term
| 19. A first magnitude star is ___ times brighter than a 2nd magnitude star |
|
Definition
|
|
Term
| 20. At what location on the earth would the South Celestial pole be located on your horizon |
|
Definition
|
|
Term
| 21. 30 arc minutes is about |
|
Definition
|
|
Term
| 22. As seen by an observer at the earth’s equator, where does the North Celestial pole appear in the sky |
|
Definition
| at the North point on the horizon |
|
|
Term
| 23. A star of the 6th magnitude differs in brightness from one of the 1st magnitude in that it is |
|
Definition
|
|
Term
| 24. At the north pole of the earth the horizon and the _____ _____ appear to coincide |
|
Definition
|
|
Term
| 25. Aristarchus of Samos was famous for |
|
Definition
| calculating the relative sizes and distances of the sun and moon |
|
|
Term
| 26. Suppose you are at the earth’s south pole, where would the North Celestial pole be |
|
Definition
|
|
Term
| 27. Stars which are said to be circumpolar |
|
Definition
| never go below or rise above one’s horizon |
|
|
Term
| 28. The universe contains |
|
Definition
| hundreds of billions of galaxies |
|
|
Term
| 29. During the night, most stars appear to |
|
Definition
| move across the sky from East to West |
|
|
Term
| 30. The solar system is located |
|
Definition
| near the outer portion of the galaxy |
|
|
Term
| 31. The name “planet” was used by ancient astronomers to mean |
|
Definition
| any object which appeared to move relative to the sun |
|
|
Term
| 32. The ancient Greeks believed the earth was stationary because |
|
Definition
| dropped objects fall straight down, no stellar parallax was seen, no strong winds from East to West |
|
|
Term
| 33. Where on the earth’s surface is each star above the horizon ½ the time |
|
Definition
|
|
Term
| 34. The person who is remembered for measuring the circumference of the earth was |
|
Definition
|
|
Term
| 35. The apparent annual motion of the sun is |
|
Definition
| from East to West along the ecliptic |
|
|
Term
| 36. The rotation axis of the earth reaches the celestial sphere and defines 2 points called the |
|
Definition
| North and South Celestial poles |
|
|
Term
| 37. The distance between which is the largest is the |
|
Definition
|
|
Term
| 38. Which abbreviation below represents 1,000 m |
|
Definition
|
|
Term
| 39. For an observer located at earth’s North Pole the Celestial Equator |
|
Definition
| is located on the observer’s horizon |
|
|
Term
| 40. Polaris is called the pole star because it lies very close to the |
|
Definition
|
|
Term
| 1. The truth about the telescope |
|
Definition
| Galieo didn’t invent it, but he was the first to use it |
|
|
Term
| 2. One theory that places the earth at the center of the solar system with the sun and the planets orbiting about it is the |
|
Definition
|
|
Term
| 3. The distance between crests of a wave is called the |
|
Definition
|
|
Term
| 4. Astronauts in orbit are |
|
Definition
| apparently weightless because they are in free fall |
|
|
Term
| 5. The gravitational attraction of the sun on a planet is _____ when the planet is at larger distances from the sun |
|
Definition
|
|
Term
| 6. “For every action there is an equal and opposite reaction” is a statement of |
|
Definition
| Newton’s 3rd Low of Motion |
|
|
Term
| 7. The ecliptic and celestial equator intersect at 2 points called the |
|
Definition
|
|
Term
| 8. The earth is closest to the sun |
|
Definition
|
|
Term
|
Definition
| “force is proportional to mass multiplied by acceleration” |
|
|
Term
| 10. At about what time of night would you expect to see a full moon highest in the sky |
|
Definition
|
|
Term
| 11. The theory of universal gravitation was developed by |
|
Definition
|
|
Term
| 12. Of the colors of visible light listed below, which has the longest wavelength |
|
Definition
| a. Blue RED green orange yellow |
|
|
Term
| 13. Which of the following lows describes the shapes of planetary orbits |
|
Definition
|
|
Term
| 14. Summer occurs for an observer on the earth because |
|
Definition
| days are longer than nights |
|
|
Term
| 15. When we experience spring in the North Hemisphere it is ____ in the South Hemisphere |
|
Definition
|
|
Term
| 16. The retrograde motion of Mars can best be explained as |
|
Definition
| the earth overtaking and passing Mars |
|
|
Term
| 17. The plane of the earth’s equators inclined to the plane of it’s orbit is at an angle of |
|
Definition
|
|
Term
| 18. The observation that Mercury and Mars never get high in the night sky was explained by |
|
Definition
| both the geocentric and heliocentric models |
|
|
Term
| 19. The North Star will not always lie close to the North Celestial Pole and be our North Star because of the |
|
Definition
|
|
Term
| 20. Precession is caused by |
|
Definition
| the gravitational attraction of the sun, rotation of the earth, the oblate shape of the earth |
|
|
Term
| 21. Temperature is a measure of the average ______ __ ______ of the particles of a substance |
|
Definition
|
|
Term
| 22. If the force of the sun’s gravity were suddenly turned off |
|
Definition
| the earth would continue to move, but in a straight line |
|
|
Term
| 23. The seasons are caused by the |
|
Definition
| 23 ½ ˚ tilt of the earth’s axis |
|
|
Term
| 24. Kepler’s 3rd law states that the square of the orbital period of a planet is proportional to |
|
Definition
| it’s orbital semi-major axis cubed |
|
|
Term
| 25. The arrangement of light by colors is called |
|
Definition
|
|
Term
| 26. Where in their orbits do planets move the greatest speed about the sun |
|
Definition
| when they are closest to the sun |
|
|
Term
| 27. If you see the moon rise at noon, it’s phase must be |
|
Definition
|
|
Term
| 28. Newton’s 3rd law: the strength of the gravitational force of the earth pulling on the moon is |
|
Definition
| equal to that of the moon pulling on the earth |
|
|
Term
| 29. The apparent annual motion of the sun is |
|
Definition
| from West to East along the ecliptic |
|
|
Term
| 30. It is summer in the Northern Hemisphere when |
|
Definition
| the sun is furthest North of the Celestial Equator |
|
|
Term
| 31. The band of constellations through which the planets, sun and moon move is called |
|
Definition
|
|
Term
| 32. If you were spending July in Australia, you’d be experiencing |
|
Definition
|
|
Term
| 33. The change in the orientation of earth’s axis of rotation has a period of about 26,000 years is called |
|
Definition
|
|
Term
| 34. With one of the 1st telescopes Galileo discovered |
|
Definition
| the mountains of the moon, the 4 brightest moons of Jupiter, the Milky Way is made up of individual stars, sunspots |
|
|
Term
| 35. Ptolemy could not explain _______ _______ __ __ ________ without epicycles and deferents |
|
Definition
| retrograde motion of the planets |
|
|
Term
| 36. A 3rd quarter moon will set at |
|
Definition
|
|
Term
| 37. The sideral day and the solar day are not the same length because the earth is |
|
Definition
|
|
Term
| 38. According to the Special Theory of Relativity the _____ __ _____ are the same for all observers |
|
Definition
|
|
Term
| 39. We remember Tycho Brahe as |
|
Definition
| the best observational astronomer of his time |
|
|
Term
| 40. The moon at 1st quarter looks like a ____ circle |
|
Definition
|
|
Term
| 1. Periodic decreases in the total amount of light received from a star may indicate that our single star is an |
|
Definition
|
|
Term
| 2. What is the function of the objective of an optical telescope designed for visual use |
|
Definition
| to gather light and form an image |
|
|
Term
| 3. In a reflecting telescope, the focus behind the hole in the main mirror is called the |
|
Definition
|
|
Term
| 4. If a star has a parallax of ¼ second of an arc, then its distance is |
|
Definition
|
|
Term
| 5. The largest telescope used for observation in the visible light region of the spectrum |
|
Definition
| are reflecting telescopes |
|
|
Term
| 6. The greatest proportion of the mass of the atom is found |
|
Definition
|
|
Term
| 7. The visible light spectrum of Hydrogen atom is made up of laws which make up the ______ series of Hydrogen |
|
Definition
|
|
Term
| 8. On the H-R diagram, where would you find the sun |
|
Definition
|
|
Term
| 9. Compared to the 100” reflector of Mt Wilson, how much light can be gathered by the 200” reflector on Mt Palomar |
|
Definition
|
|
Term
| 10. Which of the following is produced by a very hot solid |
|
Definition
|
|
Term
| 11. The frequency at which a star emits the most light depends upon the star’s |
|
Definition
|
|
Term
| 12. A star which has an annual parallax of 1 arc second is at a distance form the sun of |
|
Definition
|
|
Term
| 13. Most stars on the H-R diagram are |
|
Definition
|
|
Term
| 14. Why do stars appear to be of different colors |
|
Definition
| because of their surface temp. |
|
|
Term
| 15. The absolute magnitude of a star is a measure of it’s |
|
Definition
| brightness as seen from a distance of 10 parsecs |
|
|
Term
| 16. Refracting telescopes are telescopes which |
|
Definition
| use lenses to form an image |
|
|
Term
| 17. When an electron jumps spontaneously from a higher state to it’s lowest orbit |
|
Definition
|
|
Term
| 18. An object is observed to have a spectrum consisting only of emission lines. Therefore, it is |
|
Definition
|
|
Term
| 19. The H-R diagram is a graph of |
|
Definition
| absolute magnitude vs. spectral type (temp.) |
|
|
Term
| 20. The higher the frequency of electromagnetic radiation |
|
Definition
| the shorter its wavelengh |
|
|
Term
| 21. Stars in the main sequence that have a small mass are |
|
Definition
|
|
Term
| 22. The resolution of a telescope (the ability to see fine details) is dependent on |
|
Definition
| the diameter of the objective (primary lens or mirror) |
|
|
Term
|
Definition
| much smaller than an inch |
|
|
Term
| 24. The distances to the nearer stars may be measured by observing the |
|
Definition
|
|
Term
| 25. The radial velocity of a star is |
|
Definition
| its speed toward or away from us |
|
|
Term
| 26. If the light from a star produces 2 sets of absorption lines with different Doppler shifts, the star is called |
|
Definition
|
|
Term
| 27. Of the following types of electromagnetic radiation, which has the shortest wavelength |
|
Definition
| a. Red light, radio, infared, ultraviolet, X-Ray |
|
|
Term
| 28. In order of increasing wavelength |
|
Definition
| gamma ray, x-ray, ultraviolet, infared, radio |
|
|
Term
| 29. For a star moving away from us at 100 km/sec, which shift would spectral lines have and how would the shift depend on the star’s distance |
|
Definition
| shifted to the red, independent of the distance |
|
|
Term
| 30. The major spectral classes in order from hottest to coolest are |
|
Definition
|
|
Term
| 31. In the H-R diagram the supergiants are |
|
Definition
|
|
Term
| 32. The difference in apparent position of an object as seen from 2 different locations |
|
Definition
|
|
Term
| 33. The type of binary which are actually to be seen as 2 stars when viewed through a telescope is |
|
Definition
|
|
Term
| 34. If one had a Newtonian reflecting telescope, where would one look to find the eyepiece of it |
|
Definition
| near the top of the telescope to one side |
|
|
Term
| 35. The change in the observed wavelength from a wave source due to its motion toward or away from us is called |
|
Definition
|
|
Term
| 36. How does the astronomer obtain a star’s radial velocity |
|
Definition
| from the Doppler shift in the star’s spectrum |
|
|
Term
| 37. Stefan-Boltzman law states that |
|
Definition
| the total energy emitted by an object (star) equals the 4th power of its temperature |
|
|
Term
| 38. The masses of celestial objects are usually found from the |
|
Definition
| gravitational effects on outer objects |
|
|
Term
| 39. What characteristics of a telescope can we change when we change the eyepiece |
|
Definition
|
|
Term
| 40. Which of the following is not formed electromagnetic radiation |
|
Definition
| a. X-rays, beta rays, gamma rays, ultraviolet light, radiant heat |
|
|