The Moon and Mars will share the same right ascension, with the Moon passing 30' to the north of Mars. The Moon will be 26 days old.
At around the same time, the two objects will also make a close approach, technically called an appulse.
From Fairfield however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 10° above the horizon at dawn.
The Moon will be at mag -10.8, and Mars at mag 1.1, both in the constellation Aquarius.
The pair will be a little too widely separated to fit comfortably 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 | 22h32m20s | 10°06'S | Aquarius | -10.8 | 32'37"4 |
| Mars | 22h32m20s | 10°37'S | Aquarius | 1.1 | 5"0 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 47° from the Sun, which is in Pisces at this time of year.
The sky on 23 Nov 2024
| The sky on 23 November 2024 | ||||||||||||||||||||||||||||||||||
|
39% 22 days old |
All times shown in EST.
|
|||||||||||||||||||||||||||||||||
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
| 09 Dec 2005 | – Mars ends retrograde motion |
| 15 Nov 2007 | – Mars enters retrograde motion |
| 18 Dec 2007 | – Mars at perigee |
| 24 Dec 2007 | – 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.