The Moon and Uranus will make a close approach, passing within a mere 38.1 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 19 days old.
From Cambridge , the pair will be visible in the dawn sky, rising at 23:21 (EDT) and reaching an altitude of 38° above the south-eastern horizon before fading from view as dawn breaks at around 03:40.
The Moon will be at mag -12.2; and Uranus will be at mag 5.8. Both objects will lie in the constellation Aquarius.
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 | 23h19m40s | 5°52'S | Aquarius | -12.2 | 29'58"9 |
| Uranus | 23h19m00s | 5°15'S | Aquarius | 5.8 | 3"5 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 114° from the Sun, which is in Gemini at this time of year.
The sky on 22 Jul 2024
| The sky on 22 July 2024 | ||||||||||||||||||||||||||||||||||
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93% 17 days old |
All times shown in EDT.
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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.
Related news
| 24 Jun 2091 | – Uranus enters retrograde motion |
| 10 Sep 2091 | – Uranus at opposition |
| 24 Nov 2091 | – Uranus ends retrograde motion |
| 27 Jun 2092 | – 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.