1.2 The "Obvious" View
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Figure 1.6 Constellation Orion (a) A photograph of the group of bright stars that make up the constellation Orion. (b) The stars are connected to show the pattern visualized by the Greeks: the outline of a hunter. You can easily find this constellation in the winter sky by identifying the line of three bright stars in the hunters "belt." (c) The true three-dimensional relationships among the brightest stars (the Greek letters indicate brightnesssee More Precisely 1-2). The distances were determined by the Hipparcos satellite in the early 1990s (Chapter 17). (S.Westphal) |
Perhaps not surprisingly, the patterns have a strong cultural biasthe astronomers of ancient China saw mythical figures different from those seen by the ancient Greeks, the Babylonians, and the people of other cultures, even though they were all looking at the same stars in the night sky. Interestingly, different cultures often made the same basic groupings of stars, despite widely varying interpretations of what they saw. For example, the group of seven stars usually known in North America as "the Dipper" is known as "the Wagon" or "the Plough" in western Europe. The ancient Greeks regarded these same stars as the tail of "the Great Bear," the Egyptians saw them as the leg of an ox, the Siberians as a stag, and some Native Americans as a funeral procession.
Early astronomers had very practical reasons for studying the sky. Some constellations served as navigational guides. The star Polaris (part of the Little Dipper) indicates north, and the near-constancy of its location in the sky, from hour to hour and night to night, has aided travelers for centuries. Other constellations served as primitive calendars to predict planting and harvesting seasons. For example, many cultures knew that the appearance of certain stars on the horizon just before daybreak signaled the beginning of spring and the end of winter.
Figure 1.7 Constellations Near Orion The region of the sky conventionally associated with the constellation Orion, together with some neighboring constellations (labeled in all capital letters). Some prominent stars are also labeled in lowercase letters. The 88 constellations span the entire sky, so that every astronomical object lies in precisely one of them. |
Generally speaking, as illustrated in Figure 1.6(c) for the case of Orion, the stars that make up any particular constellation are not actually close to one another in space, even by astronomical standards. They merely are bright enough to observe with the naked eye and happen to lie in roughly the same direction in the sky as seen from Earth. Still, the constellations provide a convenient means for astronomers to specify large areas of the sky, much as geologists use continents, or politicians use voting precincts to identify certain localities on planet Earth. In all, there are 88 constellations, most of them visible from North America at some time during the year. Figure 1.7 shows how the conventionally defined constellations cover a portion of the sky in the vicinity of Orion.
Figure 1.8 Celestial Sphere Planet Earth sits fixed at the hub of the celestial sphere, which contains all the stars. This is one of the simplest possible models of the universe, but it doesnt agree with all the facts that astronomers know about the universe. |
Over the course of a night, the constellations seem to move smoothly across the sky from east to west, but ancient skywatchers were well aware that the relative locations of stars remain unchanged as this nightly march takes place. It was natural for those observers to conclude that the stars must be firmly attached to a celestial sphere surrounding Eartha canopy of stars resembling an astronomical painting on a heavenly ceiling. Figure 1.8 shows how early astronomers pictured the stars as moving with this celestial sphere as it turned around a fixed, unmoving Earth. Figure 1.9 shows how all stars appear to move in circles around a point very close to the star Polaris (better known as the Pole Star or North Star). To the ancients, this point represented the axis around which the entire celestial sphere turned.
From our modern standpoint, the apparent motion of the stars is the result of the spin, or rotation, not of the celestial sphere but of Earth. Polaris indicates the directiondue northin which Earths rotation axis points. Even though we now know that the celestial sphere is an incorrect description of the heavens, we still use the idea as a convenient fiction that helps us visualize the positions of stars in the sky. The points where Earths axis intersects the celestial sphere are called the celestial poles. In the Northern Hemisphere, the north celestial pole lies directly above Earths North Pole. The extension of Earths axis in the opposite direction defines the south celestial pole, directly above Earths South Pole. Midway between the north and south celestial poles lies the celestial equator, representing the intersection of Earths equatorial plane with the celestial sphere. These parts of the celestial sphere are marked on Figure 1.8.
When discussing the locations of stars "on the sky," astronomers naturally talk in terms of angular positions and separations. More Precisely 1-1 presents some basic information on angular measure. More Precisely 1-2 discusses in more detail the system of coordinates used to specify stellar positions.
Figure 1.9 Norhern Sky A time-lapse photograph of the northern sky. Each trail is the path of a single star across the night sky. The duration of the exposure is about five hours. (How can you tell that this is so?) The center of the concentric circles is near the North Star, Polaris, whose short, bright arc is prominently visible. (AURA) |
Why do astronomers find it useful to retain the fiction of the celestial sphere when describing the sky? What vital piece of information about stars is lost when we talk about their locations "on" the sky?