The Moon and Venus will share the same right ascension, with the Moon passing 6°19' to the north of Venus. The Moon will be 28 days old.
From Columbus however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 5° above the horizon at dawn.
The Moon will be at mag -8.7 in the constellation Aries, and Venus at mag -3.9 in the neighbouring constellation of Taurus.
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 | 03h25m50s | 23°51'N | Aries | -8.7 | 32'22"3 |
| Venus | 03h25m50s | 17°31'N | Taurus | -3.9 | 10"3 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 17° from the Sun, which is in Taurus at this time of year.
The sky on 3 Jun 2027
| The sky on 3 June 2027 | ||||||||||||||||||||||||||||||||||
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0% 28 days old |
All times shown in EDT.
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Warning
Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.
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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| 21 Mar 2028 | – Venus at greatest elongation east |
| 24 Mar 2028 | – Venus at highest altitude in evening sky |
| 11 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.