Conjunction of Mercury and Ceres

Dominic Ford, Editor
From the Conjunctions feed


Mercury and 1 Ceres will share the same right ascension, with Mercury passing 2°38' to the south of 1 Ceres.

From South El Monte however, the pair will not be readily observable since they will be very close to the Sun, at a separation of only 20° from it.

Mercury will be at mag -0.6, and 1 Ceres at mag 8.8, both in the constellation Libra.

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 Mercury 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
Mercury 15h26m50s 16°44'S Libra -0.6 6"0
1 Ceres 15h26m50s 14°06'S Libra 8.8 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 19° from the Sun, which is in Ophiuchus at this time of year.

The sky on 30 Apr 2026

The sky on 30 April 2026
Sunrise
06:01
Sunset
19:34
Twilight ends
21:07
Twilight begins
04:29


Waxing Gibbous

99%

13 days old

Planets
Rise Culm. Set
Mercury 05:29 11:53 18:18
Venus 07:31 14:39 21:47
Moon 19:04 00:22 05:36
Mars 04:59 11:17 17:34
Jupiter 10:28 17:36 00:45
Saturn 04:46 10:53 16:59
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

25 Feb 2078  –  1 Ceres at opposition
18 Jun 2079  –  1 Ceres at opposition
15 Sep 2080  –  1 Ceres at opposition
17 Dec 2081  –  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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