Conjunction of Venus and Ceres

Dominic Ford, Editor
From the Conjunctions feed


Venus and 1 Ceres will share the same right ascension, with Venus passing 2°41' to the south of 1 Ceres.

From South El Monte 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 -4.4, and 1 Ceres at mag 9.0, both in the constellation Taurus.

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

A graph of the angular separation between Venus and 1 Ceres 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 05h02m30s 18°06'N Taurus -4.4 47"2
1 Ceres 05h02m30s 20°48'N Taurus 9.0 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 28° from the Sun, which is in Gemini at this time of year.

The sky on 5 May 2026

The sky on 5 May 2026
Sunrise
05:56
Sunset
19:38
Twilight ends
21:12
Twilight begins
04:22


Waning Gibbous

83%

18 days old

Planets
Rise Culm. Set
Mercury 05:34 12:09 18:45
Venus 07:34 14:45 21:57
Moon 22:58 03:38 08:18
Mars 04:50 11:11 17:33
Jupiter 10:12 17:20 00:28
Saturn 04:28 10:35 16:42
All times shown in PDT.

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

03 Oct 1979  –  1 Ceres at opposition
08 Jan 1981  –  1 Ceres at opposition
08 May 1982  –  1 Ceres at opposition
12 Aug 1983  –  1 Ceres 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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