Download Study Guide for 1ST Astronomy Exam

Study Guide for 1ST Astronomy Exam
The successful will be able to…
Unit 1: Our Planetary Neighborhood
 Write the planets in order of increasing distance from the Sun,
 Define a dwarf planet,
 Identify dwarf planets in the solar system,
 Using a ratio determine how much larger one object is compared to another given their diameters,
 Convert AU into kilometers and kilometers into AU.
Unit 2: Beyond the Solar System
 Define a galaxy giving a representative diameter,
 List the hierarchical structures of the universe in order of increasing size,
 Define a light year and convert light-years into kilometers and kilometers into light-years.
 Calculate the travel time between two objects given their distance apart and the speed of travel, t=d/v,
 Using a proportion, calculate how big an object would be given the model size of another object. e.g. “If the Earth were the
size of a softball (diameter = 8 cm, how big would the Milky Way galaxy be?”,
Unit 3: Astronomical Numbers
 Convert between cm, m and km,
 Work in scientific notation,
 Identify astronomical numbers from a list of such numbers (e.g. the page in the text with Physical and Astronomical
Constants and Useful Formulas
Unit 5: The Night Sky
 Know and apply Dr. Fred’s Five Rules Regarding the Apparent Motion of the Stars for any given latitude,
o Identify the altitude of Polaris (i.e. the NCP)
o Determine the declination boundary of the circumpolar region
o Determine the slant angle of rising and setting stars,
o Determine the declination of the southernmost visible star,
o Determine the maximum altitude of a star given its declination,
 Draw and label the celestial sphere for an observer at any latitude,
 Draw the apparent motion of stars as seen by any observer looking North, East, South or West at any given latitude,
 Define a constellation and distinguish it from an asterism,
 Use celestial coordinates of Right Ascension and Declination appropriately in written work and problem solving,
 Use the simplified celestial sphere diagram to determine the visibility of an object and its maximum altitude, given its
declination at any latitude on the Earth,
 Use the fact that the Earth rotates 15 degrees per hour to calculate time periods between celestial events for two observers
located at different longitudes on the Earth.
Unit 6: The Year
 Describe in words and using the Whole Sky Map, developed in class, the annual motion of the Sun eastward through the stars
along the ecliptic defining and identifying the special points on the ecliptic (solstices and equinoxes),
 Correctly characterize the maximum and minimum declination of the Sun with the tilt of the Earth’s axis,
 Define precession,
 Identify precession as the cause for Polaris not always being the “North Star”,
 Describe quantitatively the apparent daily motion of the Sun on an equinox or solstice from any latitude (where sun rise
occurs, maximum altitude of the Sun, where sun set occurs, and the length of daylight) using the simplified celestial sphere
diagram,
Unit 7: The Day
 Describe in words and using the Local Horizon figure, developed in class, the daily motion of the Sun westward with the
stars along its circle of declination identifying approximately where the Sun rises and sets along the horizon, the length of
daylight, and calculate the maximum altitude of the Sun,
 Describe the location of sunrise and sunset along the horizon for any given day of the year. (Figure 7.1)
 Describe how the maximum altitude of the Sun depends on day of the year. (Fig 7.1)
 Explain why the solar day is different from the sidereal day. (Fig 7.2)
 Describe how day length varies depending on whether the Sun is above, on, or below the celestial equator.
Unit 8: The Lunar Cycles
 Describe the daily and monthly apparent motion of the Moon and its relationship to the Zodiac.
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Be able to draw and interpret Figure 8.1 illustrating the lunar phases and the Moon’s relationship to the Sun at each phase.
Name the phase of the Moon from a photograph of the Moon.
Estimate the number of days between lunar phases.
Rank images of the Moon in different phases in order of occurrence first to last.
Estimate the time of day given the Moon’s position in the observer’s sky and the lunar phase.
Locate the position of the Moon on the local observer’s celestial sphere diagram given its phase and the time of day. E.g. If
the Moon is in the last quarter phase and the time is 6 a.m. draw the location of the Moon on the celestial sphere diagram to
the right.
Explain why the lunar sidereal period is different than the time for a cycle of lunar phases.
Unit 10: Geometry of the Earth Sun and Moon
 Use the angular size relation to estimate the distance or true size of an astronomical object form a photograph.
Unit 11: Planets the Wandering Stars
 Describe the characteristics of the inferior and superior planets as regards their apparent motion in the sky. (Motion,
elongation, configuration while retrograde…)
 Work with and identify planetary configurations of opposition, conjunction, quadrature and maximum elongation.
 Present the basic ideas of the Aristotelian model of the Universe.
o Types of matter
o Location and Motion of the Earth
o Location of the planets and the observational basis for that ordering (See Figure 11.4)
 Describe the basic ideas of the Copernican model of the Universe.
o Location and Motion of the Earth
o Location of the planets and the observational basis for that ordering. (See Figure 11.10)
 Describe the cause of retrograde motion in our modern Copernican Model.
 Describe why inferior planets demonstrate a maximum elongation in their motion.
Types of Mathematical Problems
 Ratio Problems
 Proportion Problems (i.e. scale problems)
 t=d/v problems
 Angular size problems