Mercury at greatest brightness

Wed, 06 Jul 2016 at17:37 EDT(561 days ago)
21:37 UTC

Dominic Ford, Editor
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The sky at

In the southern hemisphere Mercury will be well placed for observation in the dawn sky, shining brightly at mag -2.3.

From Ashburn (click to change) however, it will not be readily observable since it will be very close to the Sun, at a separation of only 1° from it.

Mercury's orbit lies closer to the Sun than the Earth's, meaning that it always appears close to the Sun and is very difficult to observe most of the time.

It is observable only for a few days each time it reaches greatest separation from the Sun – moments referred to as greatest elongation.

Mercury's brightness

Mercury's brightness depends on two factors: its closeness to the Earth, and its phase. Its phase varies depending on its position relative to the Earth. When it passes between the Earth and Sun, for example, the side that is turned towards the Earth is entirely unilluminated, like a new moon.

Conversely, when it lies opposite to the Earth in its orbit, passing almost behind the Sun, it appears fully illuminated, like a full moon. However, at this time it is also at its most distant from the Earth, so it is actually fainter than at other times.

Mercury reaches its brightest when it is still a crescent – with less than half of its disk illuminated. This is because it is much closer to the Earth during its crescent phases than at other times.

As a result, during evening apparitions, Mercury reaches maximum brightness a few days after it is at greatest separation from the Sun, which always coincides with it showing half-phase (dichotomy).

Conversely, during morning apparitions, Mercury reaches maximum brightness a few days before it is at greatest separation from the Sun.

Mercury in coming weeks

The key moments in this apparition of Mercury are as follows:

11 Jun 2016 06:01 EDT – Mercury at dichotomy
06 Jul 2016 17:37 EDT – Mercury at greatest brightness
06 Jul 2016 23:11 EDT – Mercury at superior solar conjunction

Over coming weeks, the distance between Mercury and the Sun will decrease each night as it sinks back into the Sun's glare. The table below lists how long before sunrise Mercury will rise each night; all times are given in Ashburn local time.

Date Sun
sets at
rises at
Altitude of Mercury
at sunrise
Direction of Mercury
at sunrise
29 Jun 201605:4505:06north-west
06 Jul 201605:4905:44north-west
13 Jul 201605:5306:28-5°north-west
20 Jul 201605:5907:10-12°west
27 Jul 201606:0407:46-17°west
03 Aug 201606:1108:14-22°west
10 Aug 201606:1708:34-25°west
17 Aug 201606:2308:45-27°west
24 Aug 201606:3008:44-26°west
31 Aug 201606:3608:25-21°west
07 Sep 201606:4207:41-13°west

A graph of the brightness of Mercury is available here.

Mercury's position

The coordinates of Mercury when it reaches greatest brightness will be:

Object Right Ascension Declination Constellation Angular Size
Mercury 07h04m30s +23°58' Gemini 5.1"
Sun 07h05m +22°35' Gemini 31'27"

The coordinates above are given in J2000.0.

The sky on 06 July 2016
Sunrise 05:49
Sunset 20:37
Twilight ends
Twilight begins

2-day old moon
Age of Moon
2 days

All times shown in EDT.
Rise Culm. Set
Mercury 05:44 13:12 20:40
Venus 06:27 13:49 21:11
Moon 08:24 15:15 22:05
Mars 16:38 21:28 02:22
Jupiter 11:02 17:25 23:47
Saturn 17:51 22:45 03:42


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.

Related news

05 Jun 2016, 08:43 EDT  –  Mercury at greatest elongation west
16 Aug 2016, 11:19 EDT  –  Mercury at greatest elongation east
28 Sep 2016, 13:07 EDT  –  Mercury at greatest elongation west
11 Dec 2016, 02:45 EST  –  Mercury at greatest elongation east

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