The Moon, Mars and Uranus will make a close approach, passing within 4°37' of each other. The Moon will be 3 days old.
From South El Monte however, the trio will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 11° above the horizon at dusk.
The Moon will be at mag -10.3; Mars will be at mag 1.6; and Uranus will be at mag 5.3. The trio will lie in the constellation Virgo.
They will be too widely separated to fit within the field of view of a telescope, but will be visible to the naked eye or through a pair of binoculars.
At around the same time, the trio will also share the same right ascension – called a conjunction.
A graph of the angular separation between the Moon and Mars around the time of closest approach is available here.
The positions of the trio at the moment of closest approach will be as follows:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| The Moon | 13h18m40s | 3°11'S | Virgo | -10.3 | 31'28"7 |
| Mars | 13h11m10s | 7°24'S | Virgo | 1.6 | 4"2 |
| Uranus | 13h19m50s | 7°43'S | Virgo | 5.3 | 4"0 |
The coordinates above are given in J2000.0. The trio will be at an angular separation of 39° from the Sun, which is in Leo at this time of year.
The sky on 18 May 2026
| The sky on 18 May 2026 | ||||||||||||||||||||||||||||||||||
|
6% 2 days old |
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.
Related news
| 04 Mar 2057 | – Mars ends retrograde motion |
| 17 Jan 2059 | – Mars enters retrograde motion |
| 26 Feb 2059 | – Mars at opposition |
| 28 Feb 2059 | – Mars at perigee |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.