Close approach of the Moon and Mars

Dominic Ford, Editor
From the Appulses feed

Tags: Appulse

The Moon and Mars will make a close approach, passing within 5°16' of each other. The Moon will be 4 days old.

From Cambridge , the pair will become visible at around 17:20 (EST), 30° above your south-western horizon, as dusk fades to darkness. They will then sink towards the horizon, setting at 20:36.

The Moon will be at mag -10.9 in Pisces; and Mars will be at mag 1.1 in Aquarius.

They will be too widely separated to fit within the field of view of a telescope or pair of binoculars, but will be visible to the naked eye.

At around the same time, the pair 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 pair at the moment of closest approach will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
The Moon 22h51m40s 2°25'S Pisces -10.9 32'44"4
Mars 22h58m50s 7°22'S Aquarius 1.1 5"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 48° from the Sun, which is in Sagittarius at this time of year.

The sky on 16 Jan 2032

The sky on 16 January 2032
Sunrise
07:08
Sunset
16:36
Twilight ends
18:15
Twilight begins
05:28


Waxing Crescent

21%

4 days old

Planets
Rise Culm. Set
Mercury 06:40 11:08 15:37
Venus 04:49 09:27 14:04
Moon 09:19 15:24 21:39
Mars 09:24 15:01 20:37
Jupiter 06:27 11:00 15:34
Saturn 13:35 21:01 04:28
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.

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Image credit

The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.

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