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The Book of Stars: Being a Simple Explanation of the Stars and Their Uses to Boy Life cover

The Book of Stars: Being a Simple Explanation of the Stars and Their Uses to Boy Life

Chapter 25: APPENDIX I DOUBLE STARS
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About This Book

A practical, instructional guide for young readers presents a clear introduction to the night sky and its practical uses. It teaches how to locate major constellations and the North Star, distinguishes the sun, planets, moon, comets and meteors, and explains observing techniques with the naked eye, field glasses, and small telescopes. Chapters describe navigation and timekeeping by stars, construction and use of sundials, heliographs and sextants, and basic mapping and charts. Appendices provide definitions, illustrations, and step‑by‑step exercises aligned with scouting tests and beginner observational practice.

APPENDICES

APPENDIX A

According to the official Handbook of the Boy Scouts, if you are a Scout and want to win a merit badge for starcraft, you must

(1) Have a general knowledge of the nature of the stars and planets.

(a) By the nature of the stars and planets is meant their colors and what they are made of. Their sizes and their distances from the Earth in a general way may also be included.

(b) It is easy to tell the color of both the stars and the planets by looking at them, or by looking them up in the foregoing chapters.

(c) The spectroscope shows that the stars are made of metals and gases and other substances which we have on Earth. The planets are probably made of the same kinds of metals, gases and substances as those which form the Earth, but there is no way of proving this, for the planets shine by reflected light, and in this case the spectroscope is of little use.

(d) The stars are known to be suns as large or larger than our Sun; while the planets are about as large as our Earth—some smaller and some larger.

(e) All of the planets are within 2,800 millions of miles of the Earth, while the nearest star, except our Sun, is 25 trillions of miles from the Earth, or 8,000 times as far away.

(2) Have a general knowledge of the movements of the stars and planets.

(a) While all the stars revolve in orbits and are moving through space at high speed, they are so far away from us that they seem to be fixed and for all practical purposes they may be considered to be fixed in their positions.

(b) All the planets turn on their own axes and travel in orbits round the Sun.

(3) Point out and name 12 principal constellations.

(a) Twelve easy constellations are: (1) The Big Dipper; (2) The Little Dipper; (3) Cassiopeia; (4) Pegasus; (5) Orion; (6) Auriga and (7) Taurus, all of which are shown in Chapters I and II; (8) Gemini; (9) Leo; (10) Virgo; (11) The Scorpion, and (12) Sagittarius, which are constellations of the zodiac, and are shown in Chapter XI.

(4) Find the North by means of other stars than the Pole Star (which is the North Star) in case that star is obscured by clouds.

(a) This can be done by finding the constellation of Cassiopeia, see Chapter I; and also by Pegasus; Auriga and Orion, as explained in Chapter II.

(5) Have a general knowledge of the positions and movements of the Earth, Sun, Moon, and the Planets; and of tides, eclipses, meteors and comets.

(a) By reading the chapters on the Sun, Planets, Earth and Moon and

(b) Other things in the sky carefully, you will be able to pass the requirements named in No. 5.

(6) Plot on at least two nights per month for six months the positions of all naked eye planets visible between sundown and one hour thereafter. The plot of each planet shall contain at least three fixed stars with their names or designations; colors of planets and stars are to be recorded as observed.

(a) How to plot the position of a planet is fully explained in the chapter on Planets, but you should also read the one on The Stars of the Zodiac, and have a good star map (App. O).

APPENDIX B

Figures.—When explaining the positions and forms of things, it is often necessary to use certain terms and figures, that is to say, lines which are either real or imaginary, but which can be drawn on paper. See Fig. 185.

(1) A straight line is, of course, a line which runs uniformly in the same direction, and which is regular and without curves. A straight line is the shortest distance between two points. (2) When we say that lines are parallel, we mean that they lie so that every part of each is equally spaced from the other. (3) A line is horizontal when it is parallel with the level surface of the Earth under it. (4) A line is perpendicular to the surface of the Earth when it is plumb, that is, in a line with the center of the Earth. (5) A vertical line generally means a plumb line. (6) A right angle is formed when a vertical, or a perpendicular, line meets a horizontal line. (7) A circle is a curved line, all points of which are equally distant from its center. Circular means round like a circle. (8) By diameter is meant a straight line drawn from one side, or half of a circle, to the opposite side through its center. (9) The radius of a circle is a straight line drawn from the center of a circle, or a ball, to its circumference. (10) A ring is a disk or object having a circular hole cut in its center. (11) An arc of a circle is a part of a circle. (12) A quarter circle is, of course, the one-fourth part of a circle. (13) A tangent is a line which touches a curve but does not cut it. (14) An ellipse is an oval figure, drawn on a plane surface. (15) The equator is a circle which divides the Earth or other ball into equal parts, and is 90 degrees from the north and south poles. (16) The ecliptic is a circle round the Sky in whose plane lies the orbit of the Earth.

Fig. 185.—Geometrical Figures.

APPENDIX C
THE GREEK ALPHABET

Many of the brighter stars have names, as Aldebaran, Capella, Sirius, etc., but astronomers now indicate the stars of a constellation by the letters of the Greek alphabet. The usual method is to call the brightest star of a constellation α, that is, Alpha, the next brightest β which is Beta, and so on, but sometimes the stars are lettered in order of position in the sky.

The following is the Greek alphabet:

α Alpha ν Nu
β Beta ξ Xi (Zi)
γ Gamma ο Omicron
δ Delta π Pi
ε Epsilon ρ Rho
ζ Zeta σ Sigma
η Eta τ Tau
θ Theta υ Upsilon
ι Iota φ Phi
κ Kappa χ Chi
λ Lambda  ψ Psi
μ Mu ω Omega

APPENDIX D
STAR TESTS FOR EYESIGHT

There are a number of stars which are considered to be good tests for the seeing power of the eyes. The faint stars of the Pleiades are a fine test of this kind; but usually these tests are double stars and while one will be bright and easily seen its companion will be very faint. The test is to see the faint one, and if you can see it you may consider you have very good eyesight.

Eyesight tests are given on the following pages:

Page  
11— Mizar and Alcor
34— Spots on the Sun
94— Grimaldi on the Moon
119— Nebula in Orion
150— Epsilon in Lyra
150— Pleiades
182— Alpha and Beta in Capricornus

APPENDIX E
MAGNITUDES OF STARS

There are not nearly as many stars in the sky as you might at first suppose. The stars are divided into magnitudes, that is, according to their brightness. Stars of the first magnitude are the brightest stars; stars of the second magnitude are second brightest, and so on. The total number of stars which can be seen with the naked eye on any one night in the United States is probably not more than 3,000. The following table gives the number of stars of the different magnitudes up to and including the sixth:

Magnitudes  Number
of Stars
1st   20
2nd about 65
3rd about 200
4th about 500
5th about 1,400
6th about 5,000

APPENDIX F
FIRST MAGNITUDE STARS

The brightness of a star is known by its magnitude. A star of the first magnitude is one of the 20 brightest stars, and is 2½ times as bright as a star of the second magnitude; a star of the second magnitude is 2½ times as bright as a star of the third magnitude; and so on. A star of the sixth magnitude can just be seen with the naked eye on a clear night when there is no Moon.

Fifteen of the twenty first magnitude stars can be seen in our latitude, and these are:

NAME OF STAR   NAME OF CONSTELLATION
1. Sirius, the Dog Star, in Canis Major
2. Capella Auriga
3. Arcturus Bootes
4. Vega Lyra
5. Rigel ( β ) Orion
6. Procyon Canis Minor
7. Betelgeux ( α ) Orion
8. Altair Aquila
9. Aldebaran Taurus
10. Spica Virgo
11. Antares Scorpius
12. Pollux Gemini
13. Regulus Leo
14. Deneb Cygnus
15. Fomalhaut Piscis Australis

APPENDIX G
CONSTELLATIONS HAVING
FIRST MAGNITUDE STARS

The following important constellations are not described in the foregoing chapters of this book. They can be found, though, without trouble, since a star of the first magnitude is located in each.

Canis Major, the Big Dog, is a winter constellation, and can be seen on your meridian at 9 o’clock P. M. in February. Look for it in the southern sky and you will quickly find it because of the dazzling brightness of Sirius, the Dog Star.

Bootes (pronounced Bo-ō´-tes), the Bear Leader, is a summer constellation, and can be seen on the meridian at 9 o’clock P. M. in June. It is to the north of the ecliptic, or path of the Sun. It lies between a crown of stars and Virgo. You can’t miss it, for midway is Arcturus, a red star of the first magnitude.

Lyra, the Lyre.—Is a summer constellation, and can be seen on the meridian at 9 o’clock P. M. in August. Look for it almost overhead, and you can’t mistake it, for three bright stars, of which Vega is one, form a triangle.

Canis Minor.—The Little Dog: is a spring constellation, and can be seen on the meridian at 9 o’clock P. M. in March. It lies to the south of the constellation of Gemini, the Twins, and Cancer, the Crab. In it you will see Procyon, the Little Dog Star.

Aquila, the Eagle.—Is a summer constellation, and can be seen on the meridian in August. Look for it south of Lyra, and far to the west of Pegasus. The star that put Aquila on the map is Altair.

Cygnus, the Swan.—Is also a summer constellation, and can be seen on your meridian at 9 o’clock P. M. in September. You will find it north of Pegasus and east of Lyra, and in it you will see the Northern Cross clearly traced out with seven stars, the brightest one being Deneb, a first magnitude star.

Piscis Australis, the Southern Fish, is an inconspicuous constellation far south of the Equator. Fomalhaut, its brightest star comes only 20 degrees above our horizon and must be looked for when it is near the meridian—about 9 o’clock P. M. in October.

APPENDIX H
COLORED STARS

You can easily notice that the stars differ in color. The following list gives the colors of a few of the brighter stars:

  • White Stars:  Sirius, Regulus, Vega.
  • Blue Stars:  Rigel and Spica.
  • Red Stars:    Aldebaran, Antares, and Betelgeux.
  • Green Stars:  B Librae.
  • Yellow Stars: The Sun, Arcturus, and Capella.

APPENDIX I
DOUBLE STARS

When two stars are very close together they form what is called a double star, but double stars of which the two components are really near together in space and revolve around each other usually cannot be resolved, that is separated, into two stars without the aid of a telescope.

The North Star; Rigel, Castor; Procyon and Sirius, are all famous double stars.

APPENDIX J
VARIABLE STARS

A variable star is one whose brightness changes from time to time. A great many variable stars are known, but very few of them can be seen with the naked eye. There are different reasons given for a star varying in brightness. Our Sun is a variable star, and we are told that this is due to his spots. Another type of variation is perhaps produced by pulsations—the star periodically expanding and contracting. Again a double star formed of two bright stars which revolve round each other, as many double stars do, may eclipse one another, and this would cause a change in brightness. Here, then, are three good reasons for a star being variable.

The following are a few of the variables which can be seen with the naked eye:

  • Betelgeux, in Orion.
  • Alpha Cassiopeia, that is, the brightest star in Cassiopeia.
  • Beta Lyra, that is, the second brightest star in Lyra, and
  • Beta Pegasus, that is, the second brightest star in Pegasus.
  • Mira, in Cetus.
  • Algol, in Perseus.

APPENDIX K
INVISIBLE OR DARK STARS

Stars are born, live and die, just like human beings. All the stars, including the Sun, are either in the process of making, are at their brightest brilliancy, are dying out, or are cold and dead or have not yet become bright.

Procyon and Sirius is each attended by a comparatively dark companion. Procyon and Sirius both move slowly back and forth a short distance in the sky and this motion was attributed to the pull of satellites long before these bodies were discovered with the telescope.

APPENDIX L
THE EQUATION OF TIME

TABLE OF THE EQUATION OF TIME
 
Day of
Month 
January February March April May June
   m   s  m   s  m   s  m   s  m   s  m   s
 1 S  3 31  S 13 44  S 12 37  S 4  6  F 2 56  F 2 30
 6 S  5 49  S 14 15  S 11 33  S 2 37  F 3 27  F 1 41
11 S  7 59  S 14 27  S 10 19  S 1 14  F 3 45  F 0 44
16 S  9 49  S 14 19  S  8 57  F 0  4  F 3 48  S 0 18
21 S 11 24  S 13 52  S  7 28  F 1 12  F 3 28  S 1 23
26 S 12 39  S 13 10  S  5 56  F 2 10  F 3 15  S 2 27
31 S 13 35  S 12 13  S  4 24  F 2 56  F 2 39  S 3 38
 
 
Day of
Month 
July August September October November December
   m   s  m   s  m   s  m   s  m   s  m   s
 1 S 3 28  S 6 10  S  0  6  F 0  8  F 16 18  F 11  3
 6 S 4 24  S 5 46  F  1 31  S 11 41  F 16 17  F  9  3
11 S 5 11  S 5  8  F  3 13  F 13  4  F 15 56  F  6 51
16 S 5 46  S 4 15  F  4 58  F 14 16  F 15 13  F  4 30
21 S 6  9  S 3  9  F  6 45  F 15 13  F 14 10  F  2  2
26 S 6 11  S 1 51  F  8 29  F 15 54  F 12 45  S  0 28
31 S 6 12  S 0 24  F 10  8  F 16 16  F 11  3  S  2 55

As we have seen in Chapter X every day of the year is exactly 24 hours long by our clock time. The time by the Sun is usually either ahead or behind local clock time. The difference between clock time and Sun time is called the equation of time, and a table to show how many minutes and seconds the Sun is fast or slow, according to clock time, is given above, taken from “The New Astronomy,” by Professor Todd, who has kindly permitted me to use it here. In the table S means that the Sun is slow, that is, that the Sun does not cross the meridian until after the clock shows noon, and F means that the Sun is fast, that is, that the Sun has crossed the meridian before the clock shows noon. m means minutes, and s means seconds above the figures.

The table gives the average values of the equation of time, which may differ by a few seconds from the values for any particular year.

APPENDIX M
THE KULLMER STAR FINDER

The star finder shown in the picture was invented by Dr. C. J. Kullmer, of Syracuse, N. Y., and has been highly praised by many great astronomers.

Fig. 186.—Kullmer Star Finder.

You should own one if possible, for you do not need to know anything about the stars to operate it. It is mounted on the principle of a big telescope, but it is a naked eye instrument, an arrow taking the place of the telescope.

The finder is placed on a table, or other level surface, with the dial facing north. Then the pointer and dial are set for the day and hour when you want to find the position in the sky of a certain constellation. The indicator is turned to the name of the constellation on the dial, and this also tells the direction to set the arrow.

This is all there is to it and the arrow points right at the group of stars you want, whether they are above the horizon or not.

The finder can be used for many purposes, and it is a wonderful aid in making out in the sky the path of the stars, Sun, Moon and planets, and when they rise and set. In fact, it is a complete observatory on a small scale. Its cost is only $5.00.

APPENDIX N
THE ELLIS SEASONAL TWILIGHT CHART

A useful chart, designed by Miss E. Rebecca Ellis, of Wellesley College, Wellesley, Mass. It makes clear the changes in the lengths of the day, the phenomena of the seasons, etc. Its price is $1.00.

APPENDIX O
THE CAMP FIRE SKY MAP

This map, prepared by Prof. R. S. Dugan of Princeton University, shows the constellations as far south as the Southern Cross and is adjustable for the time of night, date, and for the latitude. Full instructions are given for its use. It is used in many schools and colleges. It is sold by the Camp Fire Stores Co., price 19 cents.