Conjunction of Mars and Uranus

Dominic Ford, Editor
From the Conjunctions feed


Mars and Uranus will share the same right ascension, with Mars passing 11' to the north of Uranus.

From Jacksonville however, the pair will not be readily observable since they will be very close to the Sun, at a separation of only 21° from it.

Mars will be at mag 1.5, and Uranus at mag 5.8, both in the constellation Taurus.

The pair will be close enough to fit within the field of view of a telescope, but will also be visible through a pair of binoculars.

A graph of the angular separation between Mars and Uranus 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 04h37m40s 22°14'N Taurus 1.5 3"9
Uranus 04h37m40s 22°02'N Taurus 5.8 3"4

The coordinates above are given in J2000.0. The pair will be at an angular separation of 21° from the Sun, which is in Gemini at this time of year.

The sky on 23 Jun 2028

The sky on 23 June 2028
Sunrise
06:22
Sunset
20:31
Twilight ends
22:08
Twilight begins
04:45


Waxing Crescent

3%

1 day old

Planets
Rise Culm. Set
Mercury 05:08 11:56 18:43
Venus 04:38 11:23 18:08
Moon 07:11 14:24 21:31
Mars 04:56 11:54 18:52
Jupiter 12:24 18:39 00:54
Saturn 03:11 09:42 16:14
All times shown in EDT.

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

12 Feb 2028  –  Uranus ends retrograde motion
18 Sep 2028  –  Uranus enters retrograde motion
03 Dec 2028  –  Uranus at opposition
16 Feb 2029  –  Uranus ends retrograde motion

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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