Close approach of Mercury and Mars

Dominic Ford, Editor
From the Appulses feed

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The planets Mercury and Mars will make a close approach, passing within a mere 10.2 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 dusk.

Mercury will be at mag -0.1; and Mars will be at mag 1.8. Both objects will lie in the constellation Cancer.

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 Mercury and Mars 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
Mercury 08h14m00s 21°16'N Cancer -0.1 6"6
Mars 08h13m40s 21°07'N Cancer 1.8 3"6

The coordinates above are given in J2000.0. The pair will be at an angular separation of 23° from the Sun, which is in Gemini at this time of year.

The sky on 22 Mar 2026

The sky on 22 March 2026
Sunrise
06:50
Sunset
19:04
Twilight ends
20:28
Twilight begins
05:27


Waxing Crescent

21%

4 days old

Planets
Rise Culm. Set
Mercury 05:49 11:30 17:11
Venus 07:43 14:05 20:27
Moon 08:54 16:11 23:37
Mars 06:14 11:59 17:43
Jupiter 12:45 19:54 03:04
Saturn 07:07 13:08 19:10
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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