The Moon and Jupiter will share the same right ascension, with the Moon passing 5°28' to the south of Jupiter. The Moon will be 2 days old.
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 7° above the horizon at dusk.
The Moon will be at mag -8.8, and Jupiter at mag -1.8, both in the constellation Gemini.
The pair 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.
A graph of the angular separation between the Moon and Jupiter 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 | 07h52m10s | 15°49'N | Gemini | -8.8 | 29'30"4 |
Jupiter | 07h52m10s | 21°18'N | Gemini | -1.8 | 31"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 Gemini at this time of year.
The sky on 23 Nov 2024
The sky on 23 November 2024 | ||||||||||||||||||||||||||||||||||
38% 22 days old |
All times shown in EST.
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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
06 Mar 2014 | – Jupiter ends retrograde motion |
08 Dec 2014 | – Jupiter enters retrograde motion |
06 Feb 2015 | – Jupiter at opposition |
08 Apr 2015 | – Jupiter ends retrograde motion |
Image credit
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.