Camelopardalus is a very inconspicuous constellation, yet it furnishes considerable occupation for the telescope. Sigma 390, of magnitude five, has a companion of magnitude nine and a half, distance 15", 160 deg.. Sigma 385, also of the fifth magnitude, has a ninth-magnitude companion, distance only 2.4", p. 160 deg.. According to some observers, the larger star is yellow and the smaller white. The star 1 is a very pretty double, magnitudes both six, distance 10.4". Its neighbor 2 of magnitude six has an eighth-magnitude companion, distance 1.7", p. 278 deg.. The star 7 of magnitude five is also double, the companion of magnitude eight being distant only 1.2". A glance at star cluster 940, which shows a slight central condensation, completes our work in Camelopardalus, and we turn to Ursa Major, represented in map No. 26. Here there are many interesting doubles and triples. Beginning with iota we find at once occupation for our largest glass. The magnitudes are three and ten, distance 10", p. 357 deg.. In the double star 23 the magnitudes are four and nine, distance 23", p. 272 deg.. A more pleasing object is sigma^2, a greenish fifth-magnitude star which has an eighth-magnitude companion, distance 2.6", p. 245 deg.. A good double for our four-inch glass is xi, whose magnitudes are four and five, distance 1.87", p. 183 deg.. This is a binary with a period of revolution of about sixty years, and is interesting as the first binary star whose orbit was determined. Savary calculated it in 1828. Near by is nu, a difficult double, magnitudes four and ten and a half, distance 7", p. 147 deg.. In 57 we find again an easy double magnitudes six and eight, distance 5.5", p. 4 deg.. Another similar double is 65, magnitudes six and eight, distance 3.9", p. 38 deg.. A third star, magnitude seven, is seen at a distance of 114" from the primary. We come now to Ursa Major's principal attraction zeta, frequently called Mizar. The naked eye perceives near it a smaller star, named Alcor. With the three-inch glass and a medium power we divide Mizar into two bright stars brilliantly contrasted in color, the larger being white and the smaller blue-green. Beside Alcor, several fainter stars are seen scattered over the field of view, and, taken all in all, there are very few equally beautiful sights in the starry heavens. The magnitudes of the double are three and four, distance 14.5", p. 148 deg.. The large star is again double, although no telescope has been able to show it so, its duplicity being revealed, like that of beta Aurigae, by the periodical splitting of the lines in its spectrum.