Close approach of Saturn and Neptune

Dominic Ford, Editor
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The planets Saturn and Neptune will make a close approach, passing within a mere 13.7 arcminutes of each other.

From Fairfield however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 16° above the horizon at dawn.

Saturn will be at mag 0.4; and Neptune will be at mag 8.0. Both objects will lie in the constellation Sagittarius.

They will be close enough to fit within the field of view of a telescope, but will also be visible through a pair of binoculars.

At around the same time, the pair will also share the same right ascension – called a conjunction.

A graph of the angular separation between Saturn and Neptune 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
Saturn 18h52m10s 22°12'S Sagittarius 0.4 15"8
Neptune 18h52m00s 21°59'S Sagittarius 8.0 2"2

The coordinates above are given in J2000.0. The pair will be at an angular separation of 60° from the Sun, which is in Aquarius at this time of year.

The sky on 9 Oct 2024

The sky on 9 October 2024
Sunrise
06:56
Sunset
18:20
Twilight ends
19:52
Twilight begins
05:24


Waxing Crescent

47%

7 days old

Planets
Rise Culm. Set
Mercury 07:30 13:03 18:36
Venus 09:50 14:46 19:41
Moon 13:49 18:05 22:21
Mars 23:31 07:01 14:31
Jupiter 21:32 05:00 12:28
Saturn 17:05 22:38 04:11
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.

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21 Sep 1989  –  Neptune 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.

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