Ionlv when they get out into the country, a the ơrniining of stars, t only need phase counterclockwise direction to the moon. in this case this is the situation, and the moon rises or sets after the sun. since the moon is 90°e of the sun, this places the sun south on the observer's celestial meridian. if we now measare from the sun in a counterclockwise or eastward direction along the ecliptic, it will place the moon at the east point of the horizon. to find the moon's phase note the elongation, and refer to the diagram of question one and determine the corresponding phase. in this case it is the first quarter using the position of the sun determine the time of obser- vation. for mid-northern latitudes appraximate the time based upon the sun as follows: 6: 00am. -rising near east point, noon-south on celestial meridian, 6: 00 p. m - setting near west point, and midnight -below horizon opposite noon position. in this case it is moon, note that all determinations of angular measure and time are approx- imate, and no measuring devices are used a. b. c. 文 a. moon position rising b. elongation 180° c. phase fui d. time a. moon position b. elongation a. moon position b. elongation c. phase wening gibbousc. phase 3rd quarter d. time d·time 6: 00 p. m. d. f. a. moon position settinga. moon position rising a. moon position b. elongation c. phase sfues b. elongationa. d. time c. phase d. time waxing gibbousc. phase d·time g. h. a. moon position setting b. elongation c. phase a. moon position a. moon position b. elongation c. phase 180