Conjunction of Mars and Ceres

Dominic Ford, Editor
From the Conjunctions feed


Mars and 1 Ceres will share the same right ascension, with Mars passing 6°04' 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 15° from it.

Mars will be at mag 1.6, and 1 Ceres at mag 8.7, both in the constellation Virgo.

A graph of the angular separation between Mars 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
Mars 13h44m20s 10°34'S Virgo 1.6 3"7
1 Ceres 13h44m20s 4°29'S Virgo 8.7 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 16° from the Sun, which is in Virgo at this time of year.

The sky on 6 Jul 2026

The sky on 6 July 2026
Sunrise
05:44
Sunset
20:06
Twilight ends
21:50
Twilight begins
04:00


Waning Gibbous

58%

21 days old

Planets
Rise Culm. Set
Mercury 06:41 13:33 20:25
Venus 09:06 15:49 22:31
Moon 23:37 05:44 11:59
Mars 03:03 10:07 17:10
Jupiter 07:05 14:06 21:07
Saturn 00:37 06:49 13:01
All times shown in PDT.

Warning

Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.

Source

The circumstances of this event were computed using the DE440 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

24 Feb 2055  –  1 Ceres at opposition
17 Jun 2056  –  1 Ceres at opposition
15 Sep 2057  –  1 Ceres at opposition
17 Dec 2058  –  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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