Conjunction of Mercury and Neptune

Dominic Ford, Editor
From the Conjunctions feed


Mercury and Neptune will share the same right ascension, with Mercury passing 9" to the north of Neptune.

From South El Monte however, the pair will not be readily observable since they will be very close to the Sun, at a separation of only 18° from it.

Mercury will be at mag -0.6, and Neptune at mag 8.0, both in the constellation Gemini.

The pair 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 Mercury and Neptune 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
Mercury 06h16m10s 22°19'N Gemini -0.6 6"3
Neptune 06h16m10s 22°18'N Gemini 8.0 2"2

The coordinates above are given in J2000.0. The pair will be at an angular separation of 18° from the Sun, which is in Gemini at this time of year.

The sky on 18 Jun 2026

The sky on 18 June 2026
Sunrise
05:37
Sunset
20:05
Twilight ends
21:50
Twilight begins
03:52


Waxing Crescent

18%

3 days old

Planets
Rise Culm. Set
Mercury 07:29 14:36 21:43
Venus 08:35 15:38 22:40
Moon 09:40 16:37 23:25
Mars 03:31 10:24 17:18
Jupiter 07:57 15:01 22:04
Saturn 01:45 07:56 14:07
All times shown in PDT.

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 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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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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