The Moon and Venus will make a close approach, passing within a mere 8.9 arcminutes of each other. From some parts of the world, the Moon will pass in front of Venus, creating a lunar occultation. The Moon will be 26 days old.
From Cambridge , the pair will be visible in the dawn sky, rising at 02:42 (EST) – 2 hours and 22 minutes before the Sun – and reaching an altitude of 21° above the eastern horizon before fading from view as dawn breaks at around 04:43.
The Moon will be at mag -10.6; and Venus will be at mag -4.1. Both objects will lie in the constellation Aries.
They 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.
At around the same time, the pair will also share the same right ascension – called a conjunction.
A graph of the angular separation between the Moon and Venus around the time of closest approach is available here.
The positions of the pair at the moment of closest approach will be as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| The Moon | 03h03m50s | 14°42'N | Aries | -10.6 | 32'09"8 |
| Venus | 03h04m00s | 14°33'N | Aries | -4.1 | 18"6 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 44° from the Sun, which is in Gemini at this time of year.
The sky on 23 Jun 2033
| The sky on 23 June 2033 | ||||||||||||||||||||||||||||||||||
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10% 26 days old |
All times shown in EDT.
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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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| 04 Jun 2034 | – Venus at highest altitude in evening sky |
| 12 Aug 2034 | – Venus at greatest elongation east |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.