Curiosities of the Sky by Garrett P. (Garrett Putman) Serviss
page 45 of 165 (27%)
page 45 of 165 (27%)
|
conspicuous and situated at an equal distance from the pole on the
other side -- Cassiopeia. This famous star-group commemorating the romantic Queen of Ethiopia whose vain boasting of her beauty was punished by the exposure of her daughter Andromeda to the ``Sea Monster,'' is well-marked by five stars which form an irregular letter ``W'' with its open side toward the pole. Three of these stars are usually ranked as of the second magnitude, and two of the third; but to ordinary observation they appear of nearly equal brightness, and present a very striking picture. They mark out the chair and a part of the figure of the beautiful queen. Beginning at the right-hand, or western, end of the ``W,'' their Greek letter designations are: Beta ({\beta}), Alpha ({\alpha}), Gamma ({\gamma}), Delta ({\delta}), and Epsilon ({\epsilon}). Four of them, Beta, Alpha, Delta, and Epsilon are traveling eastwardly at various speeds, while the fifth, Gamma, moves in a westerly direction. The motion of Beta is more rapid than that of any of the others. It should be said, however, that no little uncertainty attaches to the estimates of the rate of motion of stars which are not going very rapidly, and different observers often vary considerably in their results. In the beautiful ``Northern Crown,'' one of the most perfect and charming of all the figures to be found in the stars, the alternate combining and scattering effects of the stellar motions are shown by comparing the appearance which the constellation must have had five hundred centuries ago with that which it has at present and that which it will have in the future. The seven principle stars of the asterism, forming a surprisingly perfect coronet, have movements in three directions at right angles to one another. That in these circumstances they should ever have arrived at positions giving them so striking an appearance of definite association is certainly surprising; from its |
|