The Moon and Mars will share the same right ascension, with the Moon passing 4°08' to the south of Mars. The Moon will be 28 days old.
From Los Angeles however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 0° above the horizon at dawn.
The Moon will be at mag -9.0, and Mars at mag 1.2, both in the constellation Capricornus.
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 | 21h40m20s | 19°14'S | Capricornus | -9.0 | 33'20"1 |
| Mars | 21h40m20s | 15°05'S | Capricornus | 1.2 | 4"0 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 20° from the Sun, which is in Aquarius at this time of year.
The sky on 2 Jul 2024
| The sky on 2 July 2024 | ||||||||||||||||||||||||||||||||||
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6% 26 days old |
All times shown in PDT.
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Warning
Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.
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 Feb 2040 | – Mars ends retrograde motion |
| 27 Dec 2041 | – Mars enters retrograde motion |
| 04 Feb 2042 | – Mars at perigee |
| 06 Feb 2042 | – 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.