Close approach of Venus and Neptune

Dominic Ford, Editor
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The planets Venus and Neptune will make a close approach, passing within a mere 6.4 arcminutes of each other.

From South El Monte , the pair will be visible in the dawn sky, rising at 03:45 (PDT) – 2 hours and 53 minutes before the Sun – and reaching an altitude of 22° above the eastern horizon before fading from view as dawn breaks at around 05:39.

Venus will be at mag -4.0; and Neptune will be at mag 8.0. Both objects will lie in the constellation Leo.

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.

At around the same time, the pair will also share the same right ascension – called a conjunction.

A graph of the angular separation between Venus 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
Venus 10h07m30s 12°11'N Leo -4.0 13"8
Neptune 10h07m20s 12°05'N Leo 8.0 2"2

The coordinates above are given in J2000.0. The pair will be at an angular separation of 36° from the Sun, which is in Virgo at this time of year.

The sky on 13 May 2026

The sky on 13 May 2026
Sunrise
05:49
Sunset
19:44
Twilight ends
21:21
Twilight begins
04:13


Waning Crescent

6%

27 days old

Planets
Rise Culm. Set
Mercury 05:48 12:42 19:37
Venus 07:40 14:56 22:11
Moon 03:36 09:56 16:26
Mars 04:34 11:02 17:30
Jupiter 09:46 16:54 00:01
Saturn 03:58 10:07 16:15
All times shown in PDT.

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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Image credit

The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.

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