The Moon and Venus will share the same right ascension, with the Moon passing 6°33' to the south of Venus. The Moon will be 26 days old.
At around the same time, the two objects will also make a close approach, technically called an appulse.
From Fairfield , the pair will be visible in the dawn sky, rising at 04:11 (EDT) – 2 hours and 50 minutes before the Sun – and reaching an altitude of 20° above the south-eastern horizon before fading from view as dawn breaks at around 06:43.
The Moon will be at mag -10.5, and Venus at mag -4.2, both in the constellation Sagittarius.
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 | 17h53m10s | 27°34'S | Sagittarius | -10.5 | 29'26"2 |
| Venus | 17h53m10s | 21°00'S | Sagittarius | -4.2 | 18"5 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 44° from the Sun, which is in Capricornus at this time of year.
The sky on 2 Feb 2027
| The sky on 2 February 2027 | ||||||||||||||||||||||||||||||||||
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11% 26 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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| 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.