Close approach of Venus and Mars

Dominic Ford, Editor
From the Appulses feed

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The planets Venus and Mars will make a close approach, passing within 2°36' of each other.

From Fairfield , the pair will be difficult to observe as they will appear no higher than 17° above the horizon. They will be visible in the dawn sky, rising at 04:03 (EST) – 2 hours and 32 minutes before the Sun – and reaching an altitude of 17° above the south-eastern horizon before fading from view as dawn breaks at around 05:45.

Venus will be at mag -4.6; and Mars will be at mag 1.8. Both objects will lie in the constellation Virgo.

They will be too widely separated to fit within the field of view of a telescope, but will be visible to the naked eye or through a pair of binoculars.

A graph of the angular separation between Venus and Mars 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 13h11m40s 9°15'S Virgo -4.6 49"6
Mars 13h19m00s 7°22'S Virgo 1.8 3"8

The coordinates above are given in J2000.0. The pair will be at an angular separation of 30° from the Sun, which is in Libra at this time of year.

The sky on 13 Nov 2034

The sky on 13 November 2034
Sunrise
06:35
Sunset
16:34
Twilight ends
18:10
Twilight begins
04:59


Waxing Crescent

7%

2 days old

Planets
Rise Culm. Set
Mercury 05:38 10:53 16:07
Venus 04:03 09:33 15:04
Moon 08:42 13:41 18:39
Mars 04:04 09:41 15:18
Jupiter 14:33 20:36 02:40
Saturn 21:37 04:51 12:06
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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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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