Close approach of Mars and Uranus

Dominic Ford, Editor
From the Appulses feed

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The planets Mars and Uranus will make a close approach, passing within a mere 33.1 arcminutes of each other.

From South El Monte , the pair will be visible in the dawn sky, rising at 01:51 (PDT) and reaching an altitude of 33° above the southern horizon before fading from view as dawn breaks at around 05:44.

Mars will be at mag 1.1; and Uranus will be at mag 5.6. Both objects will lie in the constellation Libra.

They 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.

At around the same time, the pair will also share the same right ascension – called a conjunction.

A graph of the angular separation between Mars and Uranus 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
Mars 15h51m20s 19°21'S Libra 1.1 5"7
Uranus 15h50m50s 19°54'S Libra 5.6 3"6

The coordinates above are given in J2000.0. The pair will be at an angular separation of 71° from the Sun, which is in Capricornus at this time of year.

The sky on 10 Apr 2026

The sky on 10 April 2026
Sunrise
06:25
Sunset
19:19
Twilight ends
20:46
Twilight begins
04:58


Waning Crescent

40%

23 days old

Planets
Rise Culm. Set
Mercury 05:27 11:17 17:07
Venus 07:32 14:19 21:06
Moon 02:36 07:26 12:21
Mars 05:38 11:39 17:39
Jupiter 11:36 18:45 01:54
Saturn 05:58 12:02 18:07
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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