Close approach of Venus and Jupiter

Dominic Ford, Editor
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The planets Venus and Jupiter will make a close approach, passing within a mere 30.0 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 5° above the horizon at dawn.

Venus will be at mag -3.9; and Jupiter will be at mag -2.1. Both objects will lie in the constellation Aries.

They will be close enough to fit within the field of view of a telescope, but will also be visible to the naked eye or 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 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
Venus 02h08m10s 11°19'N Aries -3.9 10"7
Jupiter 02h07m30s 11°47'N Aries -2.1 32"7

The coordinates above are given in J2000.0. The pair will be at an angular separation of 22° from the Sun, which is in Taurus at this time of year.

The sky on 17 May 2035

The sky on 17 May 2035
Sunrise
05:30
Sunset
20:05
Twilight ends
22:00
Twilight begins
03:35


Waxing Gibbous

86%

10 days old

Planets
Rise Culm. Set
Mercury 06:05 13:31 20:58
Venus 04:36 11:19 18:02
Moon 15:48 21:52 03:48
Mars 01:47 06:51 11:55
Jupiter 04:34 11:19 18:04
Saturn 10:00 17:20 00:40
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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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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