Distances of the sun, and the four planets, Venus, Mars, Jupiter and Saturn, from the moon : Calculated according to Mr. Bessel's method, together with their places for every day in the year 1835, to which is added an ephemeris of the moon calculated for every third hour of mean Greenwich time upon Damoiseau's tables, the culmination of the moon for every day in 1835 for the altona meridian, with auxiliay quantities to reduce it to other meridians and tables for finding the latitude by the Polestar for 1835 /Calculated under the direction of H. C. Schumacher