The Sun passes the vernal equinox and spring begins at 8 a. m. March 21, Pacific Time. Mercury passed superior conjunction with the Sun and became an evening star on February 23, but does not attain a sufficient distance for naked eye visibility until after the first week of March. It then sets about an hour after sunset and may be seen if weather conditions are very good. The interval does not fall below an hour during the rest of the month and at the time of greatest east elongation, March 2 1 , it is about an hour and one-half. The March greatest east elongation is much smaller than the average since it occurs only a week after the planet passes perihelion. Conditions for visibility will be about as good at the next greatest east elongation occurring in July, altho the spring greatest east elongations are usually the best of the year for naked-eye observationsAfter passing elongation Mercury approaches the Sun quite rapidly, reaching conjunction and becoming a morning star on April 7. By the end of the month it has nearly reached greatest west elongation, and rises nearly an hour before sunrise. On March 11 Mercury is in conjunction with Mars, the latter planet passing about i° to the south. Venus remains an evening star, gradually drawing away from the Sun and setting later, on March 1 not quite two hours after sunset and on April 30 rather more than three hours. Altho by no means at its greatest brilliancy, which it will not reach until August, it is, after the Sun and Moon, easily the most conspicuous object in the sky. It moves during the two months not quite 6o° northward and eastward from Pisces, thru Aries, into the western part of Taurus: About the middle of April it passes between the Pleiades and Hyades groups in Taurus. Mars remains an evening star, setting thruout the two months' period at a few minutes after seven o'clock local mean time. The
Read full abstract