Mars and M22 will make a close approach, passing within a mere 22.9 arcminutes of each other.
From Cambridge however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 17° above the horizon at dawn.
Mars will be at mag 0.9; and M22 will be at mag 5.2. Both objects will lie in the constellation Sagittarius.
They will be close enough to fit within the field of view of a telescope, but will also be visible through a pair of binoculars.
A graph of the angular separation between Mars and M22 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 | 18h36m20s | 23°31'S | Sagittarius | 0.9 | 6"2 |
| M22 | 18h36m20s | 23°54'S | Sagittarius | 5.2 | 0"0 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 71° from the Sun, which is in Aquarius at this time of year.
The sky on 11 Mar 2035
| The sky on 11 March 2035 | ||||||||||||||||||||||||||||||||||
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4% 2 days old |
All times shown in EDT.
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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.
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.