Conjunction of Mars and Saturn

Dominic Ford, Editor
From the Conjunctions feed


Mars and Saturn will share the same right ascension, with Mars passing 5'37" to the south of Saturn.

At around the same time, the two objects will also make a close approach, technically called an appulse.

From South El Monte , the pair will be visible in the dawn sky, rising at 01:32 (PDT) and reaching an altitude of 39° above the south-eastern horizon before fading from view as dawn breaks at around 04:55.

Mars will be at mag 0.2, and Saturn at mag 0.8, both in the constellation Pisces.

The pair 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.

A graph of the angular separation between Mars and Saturn 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
Mars 00h11m30s 1°13'S Pisces 0.2 8"2
Saturn 00h11m30s 1°08'S Pisces 0.8 17"1

The coordinates above are given in J2000.0. The pair will be at an angular separation of 80° from the Sun, which is in Taurus at this time of year.

The sky on 3 May 2026

The sky on 3 May 2026
Sunrise
05:58
Sunset
19:37
Twilight ends
21:10
Twilight begins
04:25


Waning Gibbous

92%

17 days old

Planets
Rise Culm. Set
Mercury 05:31 12:02 18:33
Venus 07:33 14:43 21:53
Moon 21:04 01:57 06:45
Mars 04:53 11:13 17:33
Jupiter 10:18 17:26 00:34
Saturn 04:35 10:42 16:49
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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