The Moon and Venus will share the same right ascension, with the Moon passing 10' to the north of Venus. The Moon will be 27 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 dawn sky, rising at 05:19 (EST) – 1 hour and 56 minutes before the Sun – and reaching an altitude of 13° above the south-eastern horizon before fading from view as dawn breaks at around 06:55.
The Moon will be at mag -9.4, and Venus at mag -4.0, both in the constellation Ophiuchus.
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 Venus 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 | 16h47m00s | 21°08'S | Ophiuchus | -9.4 | 30'08"1 |
| Venus | 16h47m00s | 21°18'S | Ophiuchus | -4.0 | 11"3 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 25° from the Sun, which is in Sagittarius at this time of year.
The sky on 23 Nov 2024
| The sky on 23 November 2024 | ||||||||||||||||||||||||||||||||||
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39% 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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| 18 Nov 1957 | – Venus at greatest elongation east |
| 24 Dec 1957 | – Venus at highest altitude in evening sky |
| 08 Apr 1958 | – Venus at greatest elongation west |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.