Close approach of the Moon and M44

Dominic Ford, Editor
From the Appulses feed

Tags: Appulse

The Moon and M44 will make a close approach, passing within a mere 42.0 arcminutes of each other. The Moon will be 27 days old.

From Cambridge , the pair will be visible in the dawn sky, rising at 02:54 (EST) – 3 hours and 20 minutes before the Sun – and reaching an altitude of 23° above the eastern horizon before fading from view as dawn breaks at around 05:10.

The Moon will be at mag -10.3; and M44 will be at mag 3.1. Both objects will lie in the constellation Cancer.

They will be a little too widely separated to fit comfortably within the field of view of a telescope, but will be visible through a pair of binoculars.

A graph of the angular separation between the Moon and M44 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 08h41m20s 20°19'N Cancer -10.3 32'21"5
M44 08h40m20s 19°40'N Cancer 3.1 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 37° from the Sun, which is in Leo at this time of year.

The sky on 8 Sep 2026

The sky on 8 September 2026
Sunrise
06:14
Sunset
19:06
Twilight ends
20:44
Twilight begins
04:36


Waning Crescent

7%

27 days old

Planets
Rise Culm. Set
Mercury 07:08 13:20 19:32
Venus 10:05 15:12 20:19
Moon 03:06 10:35 17:49
Mars 01:17 08:51 16:25
Jupiter 03:36 10:43 17:51
Saturn 20:13 02:26 08:39
All times shown in EDT.

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.

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