Close approach of Mars and Uranus

Dominic Ford, Editor
From the Appulses feed

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The planets Mars and Uranus will make a close approach, passing within a mere 55.5 arcminutes of each other.

From Fairfield however, the pair will not be observable – they will reach their highest point in the sky during daytime and will be no higher than 17° above the horizon at dusk.

Mars will be at mag 1.7; and Uranus will be at mag 5.7. Both objects will lie in the constellation Gemini.

They will be a little too widely separated to fit comfortably within the field of view of a telescope, but will be visible through a pair of binoculars.

At around the same time, the pair will also share the same right ascension – called a conjunction.

A graph of the angular separation between Mars and Uranus around the time of closest approach is available here.

The positions of the pair at the moment of closest approach will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Mars 06h53m30s 24°10'N Gemini 1.7 4"1
Uranus 06h53m10s 23°15'N Gemini 5.7 3"6

The coordinates above are given in J2000.0. The pair will be at an angular separation of 40° from the Sun, which is in Taurus at this time of year.

The sky on 19 Jul 2024

The sky on 19 July 2024
Sunrise
05:34
Sunset
20:21
Twilight ends
22:20
Twilight begins
03:34


Waxing Gibbous

98%

14 days old

Planets
Rise Culm. Set
Mercury 07:54 14:45 21:35
Venus 06:35 13:50 21:04
Moon 19:29 23:48 04:09
Mars 01:34 08:48 16:02
Jupiter 02:18 09:42 17:06
Saturn 22:43 04:24 10:05
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.

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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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