Conjunction of Mercury and Neptune

Dominic Ford, Editor
From the Conjunctions feed


Mercury and Neptune will share the same right ascension, with Mercury passing 45' to the north of Neptune.

From South El Monte however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 4° above the horizon at dawn.

Mercury will be at mag -0.1, and Neptune at mag 8.0, both in the constellation Sagittarius.

The pair will be a little too widely separated to fit comfortably within the field of view of a telescope, but will 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 18h56m40s 21°11'S Sagittarius -0.1 7"2
Neptune 18h56m40s 21°56'S Sagittarius 8.0 2"1

The coordinates above are given in J2000.0. The pair will be at an angular separation of 24° from the Sun, which is in Capricornus at this time of year.

The sky on 23 Aug 2025

The sky on 23 August 2025
Sunrise
06:16
Sunset
19:29
Twilight ends
20:58
Twilight begins
04:47


Waxing Crescent

0%

30 days old

Planets
Rise Culm. Set
Mercury 04:53 11:44 18:35
Venus 03:39 10:40 17:41
Moon 06:42 13:21 19:50
Mars 09:27 15:20 21:13
Jupiter 02:44 09:52 17:00
Saturn 20:52 02:49 08:45
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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16 Apr 1990  –  Neptune enters retrograde motion
05 Jul 1990  –  Neptune at opposition
23 Sep 1990  –  Neptune ends retrograde motion

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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