Dominic Ford, Editor
From the Conjunctions feed
The Moon and Venus will share the same right ascension, with the Moon passing 5°41' to the south of Venus. The Moon will be 29 days old.
From Ashburn, the pair will be difficult to observe as they will appear no higher than 11° above the horizon. They will be visible in the dawn sky, rising at 05:05 (EDT) – 1 hour and 24 minutes before the Sun – and reaching an altitude of 11° above the eastern horizon before fading from view as dawn breaks at around 06:11.
The Moon will be at mag -8.2, and Venus at mag -3.9, both in the constellation Cancer.
The pair will be too widely separated to fit within the field of view of a telescope or pair of binoculars, but will be visible to the naked eye.
A graph of the angular separation between the Moon and Venus 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|
The coordinates above are given in J2000.0. The pair will be at an angular separation of 15° from the Sun, which is in Leo at this time of year.
|The sky on 24 August 2014|
29 days old
All times shown in EDT.
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.
|23 Mar 2014||– Venus at greatest elongation west|
|09 May 2015||– Venus reaches highest point in evening sky|
|06 Jun 2015||– Venus at greatest elongation east|
|21 Oct 2015||– Venus 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.