The Moon and Uranus will make a close approach, passing within a mere 41.0 arcminutes of each other. From some parts of the world, the Moon will pass in front of Uranus, creating a lunar occultation. The Moon will be 18 days old.
From Cambridge , the pair will be visible in the dawn sky, rising at 23:16 (EST) and reaching an altitude of 29° above the southern horizon before fading from view as dawn breaks at around 03:33.
The Moon will be at mag -12.4; and Uranus will be at mag 5.7. Both objects will lie in the constellation Capricornus.
They will be a little too widely separated to fit comfortably within the field of view of a telescope, but will be visible through a pair of binoculars.
A graph of the angular separation between the Moon and Uranus around the time of closest approach is available here.
The positions of the pair at the moment of closest approach will be as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| The Moon | 21h01m20s | 18°20'S | Capricornus | -12.4 | 30'44"1 |
| Uranus | 21h00m20s | 17°42'S | Capricornus | 5.7 | 3"6 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 130° from the Sun, which is in Taurus at this time of year.
The sky on 23 Nov 2024
| The sky on 23 November 2024 | ||||||||||||||||||||||||||||||||||
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40% 22 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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| 17 May 2082 | – Uranus enters retrograde motion |
| 03 Aug 2082 | – Uranus at opposition |
| 19 Oct 2082 | – Uranus ends retrograde motion |
| 22 May 2083 | – Uranus enters retrograde motion |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.