Dominic Ford, Editor
From the Appulses feed
The Moon and Mercury will make a close approach, passing within 0°25' of each other. The Moon will be 28 days old.
From Fairfield, the pair will be difficult to observe as they will appear no higher than 8° above the horizon. They will be visible in the dawn sky, rising at 05:44 (EDT) – 1 hour and 17 minutes before the Sun – and reaching an altitude of 8° above the south-eastern horizon before fading from view as dawn breaks around 06:40.
The Moon will be at mag -8.4, and Mercury at mag -0.6, both in the constellation Libra.
The pair will be close enough to fit within the field of view of a telescope, but will also be visible to the naked eye or through a pair of binoculars.
A graph of the angular separation between the Moon and Mercury around the time of closest approach is available here.
The positions of the two objects at the moment of closest approach will be as follows:
|Object||Right Ascension||Declination||Constellation||Magnitude||Angular Size|
The coordinates above are given in J2000.0. The pair will be at an angular separation of 14° from the Sun, which is in Ophiuchus at this time of year.
|The sky on 01 December 2013|
28 days old
All times shown in EST.
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.
The circumstances of this event were computed using the DE405 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.
|17 Nov 2013||– Mercury at greatest elongation west|
|31 Jan 2014||– Mercury at greatest elongation east|
|03 Feb 2014||– Mercury reaches highest point in evening sky|
|04 Mar 2014||– Mercury reaches highest point in morning sky|
The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.