Close approach of Jupiter and Mercury

Dominic Ford, Editor
From the Appulses feed

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The planets Jupiter and Mercury will make a close approach, passing within a mere 5.0 arcminutes of each other.

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 7° above the horizon at dawn.

Jupiter will be at mag -2.0; and Mercury will be at mag 0.2. Both objects will lie in the constellation Aquarius.

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 Jupiter and Mercury 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
Jupiter 22h22m30s 11°01'S Aquarius -2.0 32"7
Mercury 22h22m30s 11°06'S Aquarius 0.2 7"6

The coordinates above are given in J2000.0. The pair will be at an angular separation of 27° from the Sun, which is in Pisces at this time of year.

The sky on 30 Sep 2025

The sky on 30 September 2025
Sunrise
06:43
Sunset
18:37
Twilight ends
20:00
Twilight begins
05:20


Waxing Gibbous

59%

9 days old

Planets
Rise Culm. Set
Mercury 07:47 13:28 19:09
Venus 04:50 11:14 17:37
Moon 14:58 19:43 00:32
Mars 08:58 14:24 19:50
Jupiter 00:43 07:49 14:54
Saturn 18:15 00:09 06:03
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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