The Moon and Uranus will make a close approach, passing within 1°23' of each other. The Moon will be 19 days old.
From Cambridge , the pair will be visible in the morning sky, becoming accessible around 23:03, when they reach an altitude of 21° above your eastern horizon. They will then reach their highest point in the sky at 04:31, 70° above your southern horizon. They will be lost to dawn twilight around 05:48, 65° above your south-western horizon.
The Moon will be at mag -12.2; and Uranus will be at mag 5.6. Both objects will lie in the constellation Taurus.
They 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 the Moon 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 |
| The Moon | 05h26m10s | 21°54'N | Taurus | -12.2 | 29'29"1 |
| Uranus | 05h26m30s | 23°17'N | Taurus | 5.6 | 3"7 |
The coordinates above are given in J2000.0. The pair will be at an angular separation of 120° from the Sun, which is in Virgo at this time of year.
The sky on 16 Oct 2030
| The sky on 16 October 2030 | ||||||||||||||||||||||||||||||||||
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71% 19 days old |
All times shown in EDT.
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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
| 28 Sep 2030 | – Uranus enters retrograde motion |
| 12 Dec 2030 | – Uranus at opposition |
| 25 Feb 2031 | – Uranus ends retrograde motion |
| 02 Oct 2031 | – Uranus enters 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.