The Moon and Neptune will make a close approach, passing within a mere 0.2 arcminutes of each other. The Moon will be 14 days old.
From South El Monte , the pair will be visible between 21:06 and 03:57. They will become accessible at around 21:06, when they rise to an altitude of 21° above your south-eastern horizon. They will reach their highest point in the sky at 00:32, 42° above your southern horizon. They will become inaccessible at around 03:57 when they sink below 21° above your south-western horizon.
The Moon will be at mag -12.8; and Neptune will be at mag 7.9. Both objects will lie in the constellation Libra.
They will be close enough to fit within the field of view of a telescope, but will also be visible through a pair of binoculars.
A graph of the angular separation between the Moon and Neptune 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 | 14h35m50s | 13°19'S | Libra | -12.8 | 32'58"0 |
| Neptune | 14h35m50s | 13°19'S | Libra | 7.9 | 2"3 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 176° from the Sun, which is in Aries at this time of year.
The sky on 8 Jul 2026
| The sky on 8 July 2026 | ||||||||||||||||||||||||||||||||||
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33% 24 days old |
All times shown in PDT.
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Source
The circumstances of this event were computed using the DE440 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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| 23 Jul 2126 | – Neptune ends retrograde motion |
| 16 Feb 2127 | – Neptune enters retrograde motion |
| 05 May 2127 | – Neptune at opposition |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.