Close approach of Venus and Neptune

Dominic Ford, Editor
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The planets Venus and Neptune will make a close approach, passing within a mere 8.8 arcminutes of each other.

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 1° above the horizon at dawn.

Venus will be at mag -4.0; and Neptune will be at mag 8.0. Both objects will lie in the constellation Aquarius.

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 Venus 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
Venus 22h07m30s 12°13'S Aquarius -4.0 13"5
Neptune 22h07m20s 12°05'S Aquarius 8.0 2"2

The coordinates above are given in J2000.0. The pair will be at an angular separation of 36° from the Sun, which is in Pisces at this time of year.

The sky on 29 Nov 2024

The sky on 29 November 2024
Sunrise
06:49
Sunset
16:12
Twilight ends
17:52
Twilight begins
05:09


Waning Crescent

0%

28 days old

Planets
Rise Culm. Set
Mercury 08:01 12:29 16:58
Venus 10:12 14:39 19:06
Moon 05:25 10:10 14:48
Mars 20:16 03:43 11:10
Jupiter 16:43 00:13 07:44
Saturn 12:35 18:05 23:36
All times shown in EST.

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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22 Aug 2011  –  Neptune at opposition
09 Nov 2011  –  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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