The Moon and Saturn will share the same right ascension, with the Moon passing 1°01' to the south of Saturn. The Moon will be 13 days old.
At around the same time, the two objects will also make a close approach, technically called an appulse.
From Cambridge , the pair will be visible in the evening sky, becoming accessible around 16:42 (EDT), 16° above your eastern horizon, as dusk fades to darkness. They will then reach their highest point in the sky at 22:30, 68° above your southern horizon. They will continue to be observable until around 05:00, when they sink below 8° above your western horizon.
The Moon will be at mag -12.6, and Saturn at mag -0.5, both in the constellation Taurus.
The pair will be too widely separated to fit within the field of view of a telescope, but will be visible to the naked eye or through a pair of binoculars.
A graph of the angular separation between the Moon and Saturn around the time of closest approach is available here.
The positions of the two objects at the moment of conjunction will be as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| The Moon | 05h07m40s | 20°18'N | Taurus | -12.6 | 29'51"6 |
| Saturn | 05h07m40s | 21°20'N | Taurus | -0.5 | 20"5 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 162° from the Sun, which is in Sagittarius at this time of year.
The sky on 26 Dec 2031
| The sky on 26 December 2031 | ||||||||||||||||||||||||||||||||||
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98% 12 days old |
All times shown in EST.
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Source
The circumstances of this event were computed using the DE430 planetary ephemeris published by the Jet Propulsion Laboratory (JPL).
This event was automatically generated by searching the ephemeris for planetary alignments which are of interest to amateur astronomers, and the text above was generated based on an estimate of your location.
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| 24 Dec 2032 | – Saturn at opposition |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.