Conjunction of Jupiter and Neptune

Dominic Ford, Editor
From the Conjunctions feed


Jupiter and Neptune will share the same right ascension, with Jupiter passing 29' to the north of Neptune.

At around the same time, the two objects will also make a close approach, technically called an appulse.

From South El Monte , the pair will be visible in the dawn sky, rising at 00:35 (PDT) and reaching an altitude of 64° above the south-eastern horizon before fading from view as dawn breaks at around 06:03.

Jupiter will be at mag -2.1, and Neptune at mag 7.9, both in the constellation Cancer.

The pair 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 Jupiter and Neptune 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
Jupiter 09h10m40s 16°48'N Cancer -2.1 36"1
Neptune 09h10m40s 16°18'N Cancer 7.9 2"2

The coordinates above are given in J2000.0. The pair will be at an angular separation of 81° from the Sun, which is in Virgo at this time of year.

The sky on 4 May 2026

The sky on 4 May 2026
Sunrise
05:57
Sunset
19:37
Twilight ends
21:11
Twilight begins
04:24


Waning Gibbous

89%

17 days old

Planets
Rise Culm. Set
Mercury 05:32 12:06 18:39
Venus 07:33 14:44 21:55
Moon 22:03 02:47 07:28
Mars 04:51 11:12 17:33
Jupiter 10:15 17:23 00:31
Saturn 04:31 10:38 16:46
All times shown in PDT.

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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