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 1°56' to the north of 1 Ceres.

From Cambridge however, the pair will not be readily observable since they will lie so far south that they will never rise more than 20° above the horizon.

Venus will be at mag -3.9, and 1 Ceres at mag 9.1, both in the constellation Sagittarius.

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 18h23m30s 24°46'S Sagittarius -3.9 11"5
1 Ceres 18h23m30s 26°43'S Sagittarius 9.1 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 27° from the Sun, which is in Ophiuchus at this time of year.

The sky on 30 Nov 2019

The sky on 30 November 2019
Sunrise
06:50
Sunset
16:12
Twilight ends
17:53
Twilight begins
05:10


Waxing Crescent

20%

4 days old

Planets
Rise Culm. Set
Mercury 05:06 10:12 15:19
Venus 09:07 13:31 17:55
Moon 10:40 15:15 19:54
Mars 04:14 09:28 14:41
Jupiter 08:32 13:03 17:35
Saturn 09:47 14:23 18:59
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.

Related news

28 May 2019  –  1 Ceres at opposition
28 Aug 2020  –  1 Ceres at opposition
26 Nov 2021  –  1 Ceres at opposition
21 Mar 2023  –  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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