The Moon and Mars will share the same right ascension, with the Moon passing 2°03' to the north of Mars. The Moon will be 23 days old.
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 01:02 (PDT) and reaching an altitude of 47° above the south-eastern horizon before fading from view as dawn breaks at around 05:12.
The Moon will be at mag -11.8 in the constellation Pisces, and Mars at mag -0.0 in the neighbouring constellation of Cetus.
The pair 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.
A graph of the angular separation between the Moon and Mars 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 |
| The Moon | 00h46m30s | 4°19'N | Pisces | -11.8 | 31'30"2 |
| Mars | 00h46m30s | 2°16'N | Cetus | -0.0 | 9"2 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 85° from the Sun, which is in Gemini at this time of year.
The sky on 27 Aug 2025
| The sky on 27 August 2025 | ||||||||||||||||||||||||||||||||||
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24% 4 days old |
All times shown in PDT.
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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
| 27 Sep 2003 | – Mars ends retrograde motion |
| 01 Oct 2005 | – Mars enters retrograde motion |
| 29 Oct 2005 | – Mars at perigee |
| 06 Nov 2005 | – Mars at opposition |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.