Conjunction of Venus and Pluto

Dominic Ford, Editor
From the Conjunctions feed


Venus and 134340 Pluto will share the same right ascension, with Venus passing 7°27' to the south of 134340 Pluto.

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 7° above the horizon at dawn.

Venus will be at mag -3.9 in the constellation Ophiuchus, and 134340 Pluto at mag 14.6 in the neighbouring constellation of Serpens Cauda.

A graph of the angular separation between Venus and 134340 Pluto 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 17h30m40s 22°40'S Ophiuchus -3.9 10"7
134340 Pluto 17h30m40s 15°13'S Serpens Cauda 14.6 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 20° from the Sun, which is in Sagittarius at this time of year.

The sky on 3 Oct 2024

The sky on 3 October 2024
Sunrise
06:49
Sunset
18:30
Twilight ends
20:02
Twilight begins
05:17


Waxing Crescent

1%

1 day old

Planets
Rise Culm. Set
Mercury 07:01 12:49 18:38
Venus 09:35 14:40 19:46
Moon 07:34 13:15 18:47
Mars 23:40 07:11 14:42
Jupiter 21:55 05:23 12:51
Saturn 17:30 23:03 04:37
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

11 Jun 2004  –  134340 Pluto at opposition
14 Jun 2005  –  134340 Pluto at opposition
16 Jun 2006  –  134340 Pluto at opposition
19 Jun 2007  –  134340 Pluto at opposition

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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