The Moon and Venus will share the same right ascension, with the Moon passing 6°39' to the north of Venus. The Moon will be 28 days old.
From Los Angeles , the pair will be difficult to observe as they will appear no higher than 9° above the horizon. They will be visible in the dawn sky, rising at 04:52 (PDT) – 1 hour and 6 minutes before the Sun – and reaching an altitude of 9° above the eastern horizon before fading from view as dawn breaks at around 05:42.
The Moon will be at mag -9.3, and Venus at mag -3.9, both in the constellation Pisces.
The pair will be too widely separated to fit within the field of view of a telescope or pair of binoculars, but will be visible to the naked eye.
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 | 01h05m40s | 11°51'N | Pisces | -9.3 | 31'19"8 |
| Venus | 01h05m40s | 5°11'N | Pisces | -3.9 | 11"3 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 24° from the Sun, which is in Aries at this time of year.
The sky on 4 May 2027
| The sky on 4 May 2027 | ||||||||||||||||||||||||||||||||||
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2% 28 days old |
All times shown in PDT.
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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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| 03 Jan 2027 | – Venus at greatest elongation west |
| 21 Mar 2028 | – Venus at greatest elongation east |
| 23 Mar 2028 | – Venus at highest altitude in evening sky |
| 10 Aug 2028 | – 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.