365 Starry Nights : An Introduction to Astronomy for Every Night of the Year - Softcover

Raymo, Chet

Softcover

ISBN 10: 0671766066 ISBN 13: 9780671766061

Publisher: Simon & Schuster, 1990

Synopsis

THE AMATEUR STARGAZER'S ULTIMATE HOME COMPANION
365 Starry Nights is a unique and fascinating introduction to astronomy designed to give you a complete, clear picture of the sky every night of the year. Divided into 365 concise, illustrated essays, it focuses on the aesthetic as well as the scientific aspects of stargazing. It offers the most up-to-date information available, with hundreds of charts, drawings, and maps-that take you beyond the visible canopy of stars and constellations into the unseen realm of nebulae and galaxies.
This simple yet substantial text is full of critical information and helpful hints on how to observe the stars; describe their position; calculate their age, brightness, and distance; and much more. Whether you observe the sky with a telescope or the naked eye, 365 Starry Nights makes the infinite intimate and brings the heavens within your grasp. Keep this invaluable, informative guide close at hand, and you'll find that the sky is the limit 365 nights a year.

About this title

About the Author:

Chet Raymo is the author of The Soul of the Night and Honey from the Rock. He is a professor of physics and astronomy at Stonehill College in North Easton, Massachusetts.

Excerpt. © Reprinted by permission. All rights reserved.:

Chapter 1

JANUARY

JANUARY 1

1st: The map at the left shows all of the stars we will study during January -- and more. To find them in the sky, it is best to start with Orion, one of the most conspicuous constellations. The stars of Orion vividly suggest the mythological figure they are supposed to represent -- a bold hunter armed with a club and sword and faced by a charging bull. To observe Orion, find a place where you have a clear view of the sky. Turn so that you are facing south. During the evening hours this month you will find Orion about halfway up from the horizon to the zenith. The zenith is the point in the sky directly above your head. The most striking feature of the constellation is the alignment of three equally bright stars in the hunter's belt. If you are looking in the fight direction you can't miss it. As you stand facing giant Orion, the glittering yellow star almost directly over your head is Capella in the constellation Auriga the Charioteer. Capella, with Aldebaran in Taurus the Bull, Rigel in Orion, Sirius and Procyon in the Big and Little Dogs, and the Gemini twins Castor and Pollux, make up the Winter Hexagon. Betelgeuse, the brilliant red star in the arm of Orion, is near the center of the Hexagon. In January and February we will look closely at each of these stars and constellations in turn.

JANUARY 2

2nd: Once you have found and learned the stars of Orion's belt, you will never again have trouble recognizing this constellation. Look also for the bright stars of the shoulders and feet and the fainter stars of the head and sword. Orion rises in the early evening at the beginning of December and dominates the sky all winter long. The hunter's stars, which include two of the brightest in the heavens, outshine those of any other constellation. Because Orion stands above the earth's equator, it is visible from every inhabited place on earth. All human cultures in every time and place have given special note in story and myth to this wonderful array of stars. Sailors of old feared the sight of Orion, for his appearance on the eastern horizon forecast stormy winter weather. But the hunter has also long been associated in myth with the forces of goodness and light, and as such we welcome his appearance as a promise of sparkling starry nights to come.

JANUARY 3

3rd: It is important to acquire early a sense of your own place under the stars. Orion's belt will help. Point to the place on your horizon that is due east of your observing location (a map of your town will help you find the approximate compass points -- later you will use the stars). Now swing your arm up in an arc through the stars of Orion's belt, and on to the point on your horizon that is due west. You have traced out the sky's equator, or celestial equator. The celestial equator is the imaginary line among the stars that lies directly above the equator of the earth.

JANUARY 4

4th: It is convenient to imagine, as the ancients believed, that all of the stars lie on one great skysphere that surrounds and encloses the earth. We call this imaginary sphere the celestial sphere. In fact, as we know, the stars are distributed in space at different distances from earth, and there is no "sky-sphere." The three stars of Orion's belt, however, do lie at about the same distance from the earth and are therefore part of a true cluster. Like many of the stars, the stars of the belt have Arabic names. These names derive from the time of Europe's "Dark Ages" when the Arabs were the keepers and developers of ancient Greek astronomy. When Europeans rediscovered astronomy during the late Middle Ages, it was often by way of Arabic translations of the Greek texts. Mintaka (MIN-tack-a) means "belt." Alnitak (Al-NYE-tack) also means "the belt." The meaning of Alnilam (Al-NILE-am) is less dear but is possibly "the belt of pearls," a beautiful name for this string of dazzling stars. As we go along, you may begin to wonder why so many star names begin with "Al-." The answer is a simple one. "Al-" is the Arabic prefix which means "the."

JANUARY 5

5th: We require a convenient way to describe the positions of the stars on the celestial sphere. This is accomplished through the use of an angular method of measurement, with the vertex of the measured angle at the eye of the observer. The full circle of the sky, all the way around the earth, is 360 degrees (360°). The angle from horizon to horizon passing over your head is 180°, and the angle from the horizon to the zenith is 90°. If you stretch your arm out in front of you and sight along it with one eye, the angle between the tips of your spread fingers is about 15°. This is the width of the constellation Orion. It should take about six handspans to measure the distance from the horizon to the zenith. Try it and see how closely your hand and arm fit the rule.

JANUARY 6

6th: Our custom of dividing a circle into 360° derives from ancient Babylonian astronomy. As seen from the earth, the sun appears to make a full circuit of the sky in a little over 365 days (see Jan. 8). A degree, then, as defined by the Babylonians, was about the distance the sun moved each day with respect to the background of stars. The three little stars of Orion's head occupy a circle of about 1° diameter. The angular size of the moon against the sky is 1/2°, or about half the width of your little finger held at arm's length. The moon would therefore fit nicely between the three stars of Orion's head. If you look for these stars on a clear night you might have the impression that the moon is much larger than the space they enclose. Hold out your little finger against these stars and then against the moon, and you will discover that the moon is smaller than you think. Some other useful guides for measuring angles in the sky are shown at the right.

JANUARY 7

7th: The earth turns on its axis under the stars once every 24 hours, and carries us around as it goes. The stars remain fixed in the deeps of space. The earth turns west to east on its axis. As a result, the stars -- with sun, moon, and planets -- seem to move from east to west, making one full circuit around the earth each day. Like the sun and moon, the stars of Orion rise in the east and set in the west about 12 hours later. If you watch Orion throughout the evening, you will see him move one handspan (15°) toward the west each hour. In 24 hours, Orion will set in the west, pass beneath the earth, and rise again from the east to regain his present position. The illusion that it is the stars, not us, which move is very powerful. The earth is near at hand and seems massive and stationary compared to the apparently tiny celestial objects. Only since the brilliant theoretical work of Nicholas Copernicus in the 16th century have we come to recognize that the "turning" of the stars is actually the turning of the earth.

JANUARY 8

8th: In addition to a daily spin on its axis, the earth makes a great annual journey around the sun. Since the stars we see at night are those on the side of the earth opposite the sun, the evening sky changes as our vantage point changes. As the earth carries the observer eastward around the sun, the stars seem to move night by night toward the west at a rate of about 1° per day. In 6 months' time, looking out into space from the other side of the sun, we shall find other stars in our starry night.

JANUARY 9

9th: The stars do not appear equally bright in the sky. This is due to two things: (1) the stars are at different distances from the earth, and (2) the stars are not all of the same intrinsic brightness. The scale that is used to describe the brightness of stars as they appear to earth observers is called the scale of apparent magnitude. The scale was invented by the astronomer Hipparchus who lived and worked in the city of Alexandria 2100 years ago. The brightest stars in the sky, like Rigel and Betelgeuse in Orion, Hipparchus called stars of the first magnitude. The faintest stars he could see, he called sixth-magnitude stars. To other stars he assigned appropriate magnitudes between these limits. Thousands of years later we still use Hipparchus' scale of apparent brightness, although it has of course been made quantitatively more exact. Hipparchus was one of several great astronomers of the ancient world who was associated with the city of Alexandria.

JANUARY 10

10th: The exact modem magnitudes of the stars of Orion are shown above. If you live near city lights you will not see stars less bright than about the fourth magnitude, or no more than several hundred stars at any one time. If you live where the sky is very dark, on a clear night you might see several thousand stars down to the sixth magnitude. The stars of Orion's head are about the fourth magnitude and are a good test of the quality of the night. Of course, with binoculars or a telescope, you can see many more stars than could be seen by Hipparchus, even on dark Alexandrian nights unmarred by atmospheric pollution or electric lights. With the invention of the telescope it was necessary to extend the scale of apparent magnitude to encompass stars less bright than the sixth magnitude (see Oct. 25-28). At the other end of the scale, a few stars in the sky -- Sirius, Canopus, Alpha Centauri, and Arctutus -- have been assigned negative magnitudes on the modem scale.

JANUARY 11

11th: Just below the star Alnitak in Orion's belt is one of the most famous objects in the sky. The Horsehead Nebula is a dark cloud of dust and gas silhouetted against a brighter region of glowing interstellar gas heated to incandescence by the energy of the many stars embedded within it. The Horsehead takes its name from its shape. The size of this dark cloud is almost too great to imagine. A billion solar systems would fit neatly inside, and the Horsehead is just a wisp of a much larger cloud! You will not see the Horsehead with the naked eye. It is best seen with long-exposure telescopic photographs.

JANUARY 12

12th: The vast spaces between the stars are filled with dust and gas. It is in just such dense nebulae as the Horsehead that astronomers believe stars and possibly planets are born, condensing by gravity from the material of the cloud. If a knot of condensing gas -- it is mostly hydrogen -- is compressed to a density and temperature great enough for nuclear fusion to occur (see Jan. 14), a star is born. This is the process that is occurring even now in the Great Orion Nebula. What looks to the naked eye like three stars in Orion's sword are revealed by a small telescope to be a fascinating complex of stars and glowing gas clouds. Even to the unaided eye the central "star" of the sword may seem fuzzy. This "star" is the Great Nebula, a spectacular region of turbulent gas and dust heated by the radiation of hot young stars that have only recently (by star time!) condensed from the matter of the cloud. The diameter of the Great Nebula is more than 20,000 times that of the solar system, and there is enough hydrogen, helium, and other materials in the cloud to form at least 10,000 stars similar to our sun. Stars have lifetimes such as we do, although much longer ones. In the Great Orion Nebula we observe their births; shortly we will see how they die.

JANUARY 13

13th: Embedded in the very heart of the Great Orion Nebula, and visible with binoculars or a small telescope, is the beautiful multiple star system known as the Trapezium, four hot young stars in a tight trapezoid-shaped cluster. Actually, these four stars are only the brighter components of an expanding cluster containing hundreds of faint stars. The intense radiation from these high-temperature stars excites the gas of the surrounding nebula and makes it glow. To the eye the nebula glows with an eerie green light, but photographs show beautiful hues of pink, blue, and violet.

JANUARY 14

14th: From the expansion rate of the Trapezium cluster and from the color and brightness characteristics of the member stars (see Mar. 19-20), it has been estimated that the stars in the group may be less than half a million years old -- making it one of the youngest associations of stars known. Indeed, some members of the group may even now be "turning on" their nuclear energy sources to become stars. As gravity pulls together a knot of gas and dust from the Great Nebula, the pressure and temperature at the core of the contracting cloud go up. When the temperature reaches about 10 million degrees Celsius, nuclei of hydrogen atoms fuse together to form the heavier nuclei of helium. This is the same process that occurs in the explosion of a hydrogen bomb and results in a release of energy. The energy makes its way to the surface of the contracting sphere where it is radiated as heat and light. A star is born! The new energy source at the star's core stops the gravitational contraction of the star. The star can continue to burn steadily -- an outward pressure sustained by nuclear fusion balanced against gravity -- for as long as the hydrogen at the core holds out. The lifetime of a hot blue star such as Bellatrix might be as little as 10 million years. Bellatrix is larger than the sun and contains 10 times as much matter. Although it has more fuel than the sun, Bellatrix is a hotter star and "bums" its hydrogen at a faster rate. The slower-burning sun will probably have a lifetime of 10 or 15 billion years. Since our star is now about 5 billion years old, we have about at least 5 billion years to go!

JANUARY 15

15th: When a star such as Bellatrix has used up the hydrogen fuel at its core, gravity again gets the upper hand and the core of the star collapses. The sudden increase in pressure and temperature in the core releases new (but limited) sources of nuclear energy which heat the outer layers of the star and cause them to expand outward. As the star swells, the outer layers cool and change color from bluish, to white, to yellow, to red. The massive white star Rigel (RYE-jell, "foot") is possibly at this stage of its evolution and has begun the process of expansion. Rigel is 50 times bigger than the sun.

JANUARY 16

16th: If Rigel continues to expand, in tens of thousands of years it will become a red giant star like Betelgeuse (BET-el-jews, or beetle juice is close enough, "armpit of the giant"). Betelgeuse is one of the largest stars known. Its diameter is greater than the earth's orbit around the sun! It is one of the very few giant stars that has been seen as an actual disk, rather than a mere point of light. Using special techniques, astronomers have taken photographs that show features of its surface. The distinctive reddish, color of Betelgeuse is readily apparent to the eye, particularly by contrast with white Rigel.

JANUARY 17

17th: As he stands in the winter sky with his club raised, Orion faces a formidable opponent. Plunging toward him from the west is Taurus (TOR-us) the Bull, an awesome long-homed creature with threatening red eye and head lowered in a tumultuous charge. The bull is not so conspicuous a constellation as bright Orion, but the "vee" of stars that outlines the bull's face is easily recognized. Taurus is almost certainly one of the most ancient of the constellations. It is one of the familiar signs of the zodiac, the constellations that the sun moves through during its yearly journey across the sky (see June 25). Six thousand years ago, when astronomy and agriculture were developing together in the civilizations of the East an...

About this edition

• Publisher: Simon & Schuster
• Publication date: 1990
• ISBN 10: 0671766066
• ISBN 13: 9780671766061
• Binding: Paperback
• Number of pages: 240