The Moon and Jupiter will share the same right ascension, with the Moon passing 8'22" to the north of Jupiter. The Moon will be 15 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 between 20:02 and 05:28. They will become accessible at around 20:02, when they rise to an altitude of 7° above your eastern horizon. They will reach their highest point in the sky at 00:45, 38° above your southern horizon. They will become inaccessible at around 05:28 when they sink below 7° above your western horizon.
The Moon will be at mag -12.6, and Jupiter at mag -2.5, both in the constellation Virgo.
The pair will be close enough to fit within the field of view of a telescope, but will also be visible to the naked eye or through a pair of binoculars.
A graph of the angular separation between the Moon and Jupiter 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 | 13h39m50s | 8°34'S | Virgo | -12.6 | 30'26"6 |
| Jupiter | 13h39m50s | 8°43'S | Virgo | -2.5 | 43"3 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 178° from the Sun, which is in Pisces at this time of year.
The sky on 22 Nov 2024
| The sky on 22 November 2024 | ||||||||||||||||||||||||||||||||||
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46% 21 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 Mar 2042 | – Jupiter 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.