From: EXOS%"green@noao.edu" 30-DEC-1988 13:20:24.87 To: JMS CC: Subj: Phases of the Moon Return-path: Received: from carina.noao.arizona.edu (noao.edu) by mis.arizona.edu id 20A000B8002 ; Wed, 28 Dec 88 00:27:49 MST Received: by noao.edu (5.59/SAG.G11) id AA08699; Tue, 27 Dec 88 12:11:31 MST; for jms@mis.arizona.edu Date: Tue, 27 Dec 88 12:11:31 MST Message-Id: <8812271911.AA08699@noao.edu> To: jms@mis.arizona.edu Hello Joel Snyder, Your questions about the moon's phases are reasonable and interesting. That "high point" is called "transit" by astronomers, and is achieved by every celestial object, including the moon. It's a natural consequence of their rising on the Eastern horizon and setting in the West; their highest apparent elevation in the sky (off the horizon) occurs halfway in between. When the moon is full, it is exactly on the other side of the Earth from the Sun. Since the Sun transits at about noon, the full moon transits at about midnight. Interestingly enough, the elevation of the moon's transit varies a great deal throughout the year, and through each month (or lunation). The moon's orbital plane is tipped by about 29 degrees with respect to the Earth's equatorial plane. Each month, the moon describes a complete circuit, appearing at +29 degrees to -29 degrees with respect to the Earth's equator projected onto the sky. The Earth "carries" the Moon and its orbit around the Sun with it, so once a year the full Moon transits near the "top" of its orbit at +29 degrees (almost overhead in Tucson). Six months later, the Moon will transit very low in the sky, at about -29 degrees (28 degrees above the horizon). While the full Moon transits at midnight each month, then, the height of that transit varies from month to month. I'll be happy to provide an astronomy E-mail answering service. Please give my regards to Bruce. Richard Green