The Moon and Jupiter will make a close approach, passing within 5°36' of each other. The Moon will be 16 days old.
From San Diego , the pair will be visible in the morning sky, becoming accessible around 18:52, when they reach an altitude of 7° above your eastern horizon. They will then reach their highest point in the sky at 01:11, 79° above your southern horizon. They will be lost to dawn twilight around 06:02, 25° above your western horizon.
The Moon will be at mag -12.7; and Jupiter will be at mag -2.8. Both objects will lie in the constellation Taurus.
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 Jupiter 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 | 05h07m30s | 27°48'N | Taurus | -12.7 | 32'26"4 |
Jupiter | 05h10m20s | 22°14'N | Taurus | -2.8 | 46"5 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 156° from the Sun, which is in Libra at this time of year.
The sky on 17 Nov 2024
The sky on 17 November 2024 | ||||||||||||||||||||||||||||||||||
93% 16 days old |
All times shown in PST.
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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.
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08 Oct 2024 | – Jupiter enters retrograde motion |
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11 Nov 2025 | – Jupiter enters 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.