Conjunction of Mars and Eris

Dominic Ford, Editor
From the Conjunctions feed


Mars and 136199 Eris will share the same right ascension, with Mars passing 9°56' to the north of 136199 Eris.

From South El Monte , the pair will become visible at around 18:16 (PDT), 55° above your south-western horizon, as dusk fades to darkness. They will then sink towards the horizon, setting at 23:27.

Mars will be at mag 0.5 in the constellation Aries, and 136199 Eris at mag 18.7 in the neighbouring constellation of Cetus.

A graph of the angular separation between Mars and 136199 Eris 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 01h50m20s 12°12'N Aries 0.5 7"3
136199 Eris 01h50m20s 2°15'N Cetus 18.7 0"0

The coordinates above are given in J2000.0. The pair will be at an angular separation of 83° from the Sun, which is in Capricornus at this time of year.

The sky on 2 Jun 2025

The sky on 2 June 2025
Sunrise
05:38
Sunset
19:58
Twilight ends
21:41
Twilight begins
03:56


Waxing Gibbous

54%

6 days old

Planets
Rise Culm. Set
Mercury 05:54 13:07 20:20
Venus 03:22 09:47 16:12
Moon 12:24 18:58 01:23
Mars 10:56 17:43 00:29
Jupiter 06:46 13:57 21:07
Saturn 02:13 08:11 14:08
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

20 Oct 2035  –  136199 Eris at opposition
20 Oct 2036  –  136199 Eris at opposition
20 Oct 2037  –  136199 Eris at opposition
21 Oct 2038  –  136199 Eris 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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