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Program by: Kevin Bagley & David Kampschafer
Documentation by: Mary Lynne Sanford
All rights reserved Copyright (c) 1981 SYNERGISTIC SOFTWARE 5221 120th Ave. S.E. Bellevue, WA 98006 ( 206) 226-3216
Apple] [and Applesoft are trademarks of Apple Computer, Inc. (
TABLE OF CONTENTS LIST OF TABLES AND FIGURES
SECTION TITLE PAGE FIGURE TITLE PAGE List of Tables and Figures 3 1 Main Menu 6 I Introduction 5 2 Planet Symbols 7 II Getting Started 6 3 Phases of the Moon 11 Ill Using the Program 7 4 Mars Retrograde Motion ( 1973) 12 Menu Item 1: Planets and Related Data 7 Menu Item 2: Relative Sizes 8 TABLE TITLE PAGE Menu Item 3: Relative Orbits 8 1 Planet Orbital Data 9 Menu Item 4: Other Solar System Members 8 Menu Item 5: Planet Position 9 Menu Item 6: Terminate 10 IV Additional Solar System Information 10 The Ecliptic 10 Phases of the Moon 10 Retrograde Motion 11 Glossary of Astronomical Terms 13 Bibliography 16
2 3
4 4
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t Menu Item 2: Relative Sizes TABLE 1 PLANET ORBITAL DATA This option will assist you in visualizing planetary size. Here, the program asks if you wish to view one planet, two for comparison, or all. The indica ted planet(s) will then be drawn on the screen, again with their universal DISTANCE FROM SUN SIDEREAL PERIOD symbols (see Figure 2). PLANET AU 106 KM YEARS DAYS Menu Item 3: Relative Orbits '1) Mercury 0.3871 57.9 0.24085 87.97 The information in this section illustrates the position of the planets in re 0.7233 108.1 0.61521 224.70 ~ Venus lation to each other. Here, there is a choice of viewing all nine planets, the Earth 1.0000 149.5 1.000039 365.26 inner four, or outer five. Viewing the planetary orbits by inner four or oute r Mars 1.5237 227.8 1.88089 686.98 five at a time gives an improved scale while viewing all nine at once gives some Jupiter 5.2028 778 11.86223 indication of the tremendous distances involved. After requesting one of Saturn 9.5388 1426 29.4577 these options, the program will draw the orbits of the planets as seen from an Uranus 19.182 2868 84.013 oblique angle. This angle is necessary to give maximum view since the planets' Neptune 30.058 4494 164.793 orbital sizes vary so greatly. Also, the great eccentricity of Pluto's orbit actu Pluto 39.439 5896 247.686 ally causes it to cross that of Neptune. Sub-section #4 of Relative Orbits is provided to give an understanding of For the mean equator and equinox of 1960. Source: Supplement to the various orbital speeds of the planets. After selecting this option, you wil l The American Ephemeris and Nautical Almanac. key in a time increment (the amount of time between each positioning of the planets). The screen will then show the sun and the planets below it in order of closeness to the sun. The scale is not true, but spaced so that you can more easily place each planet. The planets will begin to move and, with each move Menu Item 5: Planet Position ment, the number of elapsed increments (week-month-year-decade) wil l be displayed. For true planet postions, see option #5 on the Main Menu or refer This section offers several ways of viewing the planets in relation to each to Table 1 which lists both distance from the sun and orbital period of each other. Choosing the inner fou r, outer five, or al l planets, the program can planet. draw either a representation of the planets as they orbit the sun, or the plan ets as they are seen in the night sky within the constellations of the ecliptic Menu Item 4: Other Solar System Members (see section IV). The orbit opt ion shows relative orbit position at a specified date to aid in spatial orientation of planetary position for that date. (You also This section offers information on the sun and the moon, satellites of the key in a time increment and a choice between a stationary or dynamic view.) planets, asteroids and interplanetary dust, and comets. The options are avail The constellation option allows you to display the night sky with planets able by indicated number; further directions are given on the program as you shown in their correct position for the specified date. Press the space bar to proceed. see a table of right ascension and declination for the indicated planets. These The sun-moon section provides text on both of these bodies, also a graphic values will help you locate the planets in the sky using a telescope. demonstration of the phases of the moon. Under the constellation option, the selection of t/1, Information, will pro The satellites sub-section lists the planets; you press the number of the vide a list of all the planets' locations within constellations as of your speci planet to see information about its satellites or moons. Statistical material fied date. If you select a constellation number, you will see a graphical rep about them will appear on the screen, one satellite at a t ime, beginning with resentation of the constellation and the planets within it. Note that only the the one nearest the planet. As directed by the program, press any key to go_ 1 constellations of the zodiac are listed because the planets only appear within from one satellite to the next. This material will help you appreciate how j the belt of the zodiac (the ecliptic). The planets maintain their positions in much the satellites vary. For instance, Saturn and Jupiter both have moons the constellation as it appears to move across the sky during the night. that are larger than the planet Mercury, yet some moons are smaller than A demonstration of retrograde motion is included in section 5. Retro many asteroids. When the list is complete, pressing any key returns you to grade motion is an apparent phenomenon occuring when the Earth, which is the Other Solar System Members Menu . moving faster around the sun than the outer planets appears to stop its reg Descriptive information about asteroids and interplanetary dust is avail ular eastward motion through the sky and go backward for a time. (For a able in that sub-section. more detailed explanation, see section IV, 3.) The comet sub-section offers graphic displays of a comet itself and the The program presents a model of retrograde motion by placing the sun in path a comet takes when entering the solar system, as well as textual informa the Earth's orbit. As you view the planets in motion, then, it is as though tion. The program indicates which keys to press for each option. they are orbiting the Earth. You observe all of the outer planets' retrograde
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a GLOSSARY OF ASTRONOMICAL TERMS
ALBEDO: The fraction of light which a body reflects of that which falls on it. The higher a body's albedo, the brighter it appears in the sky compared to other bodies of the same distance from the sun. ALTITUDE: Angular distance above or below the horizon, measured along Figure 4 a vertical circle, to a celestial object. Mars Retrograde Motion (1973) ASTEROID: Synonym for minor planet. ASTRONOMICAL UNIT (AU): The approximate distance from the sun to the Earth. CELESTIAL EQUATOR: The projection of the Earth's Equator onto the celestial sphere. CELESTIAL SPHERE: The apparent sphere of sky and stars that surrounds 'f ', • ·· ------· Earth. I I I COMET: A small body of ice and dust revolving around the sun, sometimes -:. I • developing a 'tail' pointing away from the sun when near perihelion •'... I ' (closest approach to the sun) . I , PEGASUS : I I CONSTELLATION: A configuration of stars in a certain limited region of the • I I I I sky, regardless of their distance from Earth. JANl I 0 I ~------· CRATER: A more or less circular depression on the moon or other solar sys tem member caused by volcanic activity or meteor impact. PISCES • DECLINATION: One of a system of coordinates, along with right ascension, SEPT 1 -...... _ ,• that is measured on the celestial sphere instead of on Earth, as latitude and ---·-~------...--...,...-•, / - longitude. The position of a star or other point is measured on an hour I - .....~ I ' I< circle north or south of the celestial equator . .__--.-'I / ECCENTRICITY: The degree to which the orbit of a revolving body is oval, ', JU LY 1 or elliptical, instead of round. •. ~ , ECLIPTIC: The area in the sky where constellations of the zodiac, planets, ', ~"' ' the sun and moon are observed, since the orbital planes of the moon around the Earth, and other planets around the sun, etc. roughly corre '' '~----.---.''------.. -~ spond. (See explanation in Section IV, Other Solar System Information.) ' \ CETUS EQUATIONAL INCLINATION: The tilt of a rotating body's equator as com • • pared to its orbital plane . • EQUINOX: One of the intersections of the ecliptic and celestial equator. The two equinoxes are the vernal equinox (the advent of spring) and the autumnal equinox (the beginning of fall). ESCAPE VELOCITY: The velocity needed to escape the gravitational pull of Retrograde motion occurs when the Earth, which is moving faster around a body. the sun than the outer planets, overtakes and passes one of them. As the ESTRASOLAR: Outside of the sun. Earth passes, the outer planet is in opposition, that is, it is in a straight line HORIZON: An extension onto the celestial sphere of the Earth's horizon. with the Earth and Sun, with the outer planet and sun on opposite sides of INCLINATION OF ORBIT: The difference in angle of orbits between are- the Earth. Against the backdrop of distant stars, the outer planet appears to volving planet or body and the ecliptic. stop and move westward, or backward, during this period of opposition. As INTERPLANETARY MEDIUM: The sparse distribution of gas and solid par the Earth moves on around the sun and out of opposition with the outer ticles in the interplanetary space. planet, the outer planet appears to resume its eastward motion across the sky. KELVIN: The temperature scale most often used in astronomy . It measures The same apparent phenomenon occurs as you overtake another car travel temp erature from absolute zero (-273 degrees C.=O degrees K.), the point ing in the same direction on the highway. As you approach it, the other car at which all molecular activity stops. moves in the same direction as your car against the landscape. As you pass it, LIGHT YEAR: The distance light travels in one year or roughly 5.88*10e12 it appears to be moving backwards in relation to the more distant landscape. miles or 5,880,000,000,000 miles. If you look back after you have passed, the other car again appears to move forward. ,
12 13 MAGNITUDE: A measure of the amount of light received from a star or VELOCITY OF ESCAPE: The speed with which an object must move in other luminous object- its relative brightness. order to enter a parabolic orbit about another body, and hence move per MASS: A measure of the total amount of material in a body; defined either manently away from the vicinity of that body. by the inertial properties of the body or by its gravitational influence on VISUAL MAGNITUDE: A measure of the amount of visible light received other bodies. from a star or other luminous or reflecting body. MEAN DENSITY: The ratio of an object's mass to its volume. A density less ZENITH: The point exactly overhead in a line extended upward from Earth than one will float in water while greater than one will sink. to the celestial sphere. At the Earth's North Pole, an observer would see METEOR: The luminous phenomenon observed when a meteroid enters the the north celestial pole directly overhead (at zenith). Earth's atmosphere and burns up. ZODIAC: A belt around the sky centered on the ecliptic within which the 12 METEORITE: A portion of a meteoroid that survives passage through the constellations are found. The sun and the planets, with the exception of atmosphere and strikes the ground. Pluto, are always seen within it. METEOROID: A stony or metallic particle in space before any encounter with the Earth. MINOR PLANET: Synonym for asteroid. One of several tens of thousands of small planets, ranging in size from a few hundred kilometers to less than one kilometer in diameter. Most minor planets in our solar system orbit between Mars and Jupiter. OBLATENESS: The amount of flattening that occurs at the poles of a rotat ing body. PERIOD OF ROTATION: The time required for one complete rotation. On earth, this is one day. PLANET: Any of the nine largest solid bodies revolving about the sun. RETROGRADE MOTION: An apparent westward motion of a planet on the celestial sphere or with respect to the stars. (See Section IV, Other Solar System Information.) RIGHT ASCENSION: One of a system of coordinates, along with declina tion, that is measured on the celestial sphere instead of on the Earth, as latitude and longitude. Right ascension is the position of a star or other point measured eastward to the hour circle of the star from a reference point (the vernal equinox) on the celestial equator . SATELLITE: A body that revolves about a larger one; for example, a moon of a planet. SEMI MAJOR AXIS: In an elliptical orbit, the distance from the center of the ellipse out to one end of the orbit. SIDEREAL PERIOD: The period of revolution of one body about another; in our solar system, the time required for a planet to make one revolution of the sun. SOLAR SYSTEM: The system of the sun and the planets, their satellites, the minor planets, comets,meteoroids, and other objects revolving around the sun. SOLAR WIND: Charged particles ejected from the sun and flowing outward in gusts throughout the entire solar system, traveling at speeds between 200 and 400 miles per second. SPECIFIC GRAVITY: The ratio of the density of a body or substance to that of water. SYNODIC PERIOD: For planets, this is the interval in which the Earth gains a lap on one of the outer planets; or in which Mercury or Venus gains a lap on Earth. TROPICAL YEAR: Period of revolution of a body about the sun with re spect to a fixed location in space (vernal equinox).
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Bl BLIOG RAPHY
Abell, George 0., Realm of the Universe, New York: Holt, Rinehart and Winston, Inc., 1976.
Alter, Dinsmore, et. al., Pictorial Astronomy, New York: Lippincott and Crowell, 1974.
Beatty, J. Kelly, et. al., The New Solar System, Cambridge, Mass, Sky Publishing Corp., 1981
Huxley, Julian, Space, London: Aldus Book Ltd., 1968.
Menzel, Donald H., A Field Guide to the Stars and Planets, Boston: Houghton Mifflin Company, 1964.
Moore, Patrick, The Atlas of the Universe, Rand McNally, 1970.
Moore, Patrick, The Observer's Book of Astronomy, New York, Frederick Warne 6 Company Ltd., 1971.
Nicholson, ian, Exploring the Planets (Life Science Library), New York: Time Incorporated, 1966.
Ridpath, I an, Ed., The Illustrated Encyclopedia of Astronomy and Space, New York: Thomas E. Crowell Co., 1976.
Sagan, Carl & Leonard, Johnathan N., Planets (Life Science Library), New York: Time Incorporated, 1966.
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