Conjunction of Venus and Mars

Dominic Ford, Editor
From the Conjunctions feed


Venus and Mars will share the same right ascension, with Venus passing 2°27' to the south of Mars.

From Columbus however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 10° above the horizon at dusk.

Venus will be at mag -4.4, and Mars at mag 1.5, both in the constellation Virgo.

The pair 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 two objects at the moment of conjunction will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Venus 12h57m00s 8°22'S Virgo -4.4 25"5
Mars 12h57m00s 5°55'S Virgo 1.5 4"4

The coordinates above are given in J2000.0. The pair will be at an angular separation of 45° from the Sun, which is in Leo at this time of year.

The sky on 16 Jul 2024

The sky on 16 July 2024
Sunrise
06:14
Sunset
20:58
Twilight ends
22:55
Twilight begins
04:17


Waxing Gibbous

80%

11 days old

Planets
Rise Culm. Set
Mercury 08:28 15:23 22:17
Venus 07:10 14:25 21:40
Moon 16:51 21:36 02:16
Mars 02:21 09:30 16:40
Jupiter 03:10 10:31 17:51
Saturn 23:33 05:15 10:57
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.

Related news

10 Mar 2010  –  Mars ends retrograde motion
23 Jan 2012  –  Mars enters retrograde motion
03 Mar 2012  –  Mars at opposition
05 Mar 2012  –  Mars at perigee

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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