© NASA/JPL/MESSENGER

Mercury at greatest elongation east

Thu, 23 Nov 2017 at21:22 EST(14 hours ago)
02:22 UTC

Dominic Ford, Editor
From the Inner Planets feed

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Ashburn
The sky at

In the southern hemisphere Mercury will be well placed for observation in the evening sky, shining brightly at mag -0.4.

From Ashburn (click to change) however, it will not be observable – it will reach its highest point in the sky during daytime and will be no higher than 6° above the horizon at dusk.

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.

These apparitions take place alternately in the morning and evening skies, depending whether Mercury lies to the east of the Sun or to the west.

When it lies to the east, it rises and sets a short time after the Sun and is visible in early evening twilight. When it lies to the west of the Sun, it rises and sets a short time before the Sun and is visible shortly before sunrise.

On this occasion, it lies 21° to the Sun's east.

Mercury in coming weeks

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

22 Nov 2017 13:20 EST – Mercury at greatest brightness
23 Nov 2017 21:22 EST – Mercury at greatest elongation east
28 Nov 2017 04:03 EST – Mercury at dichotomy
12 Dec 2017 20:43 EST – Mercury at inferior solar conjunction

After greatest elongation, 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 Mercury will remain up after sunset each night; all times are given in Ashburn local time.

Date Sun
sets at
Mercury
sets at
Altitude of Mercury
at sunset
Direction of Mercury
at sunset
17 Nov 201716:5117:53south-west
24 Nov 201716:4617:5910°south-west
01 Dec 201716:4417:5710°south-west
08 Dec 201716:4217:32south-west
15 Dec 201716:4316:39south-west
22 Dec 201716:4615:52-10°west
29 Dec 201716:5015:30-15°west
05 Jan 201816:5515:24-17°west
12 Jan 201817:0215:30-16°west
19 Jan 201817:0915:43-16°west
26 Jan 201817:1716:02-14°west

A graph of the angular separation of Mercury from the Sun around the time of greatest elongation is available here.

Mercury's position

The position of Mercury when it reaches greatest elongation will be:

Object Right Ascension Declination Constellation Magnitude Angular Size
Mercury 17h31m30s -25°45' Ophiuchus -0.4 6.6"
Sun 15h58m -20°30' Scorpius -26.7 32'23"

The coordinates above are given in J2000.0.

Seasonal effects

At each apparition, Mercury reaches a similar separation from the Sun – around 18–28°. This distance is set by the geometry of how big Mercury's orbit is, and how far away it is from the Earth.

Nonetheless, some times of the year are more favourable for viewing Mercury than others.

It appears most favourably in the evening sky around the time of the local spring equinox, and most favourably in the morning sky around the local autumn equinox.

These dates are reversed in the northern and southern hemispheres, such that a good apparition in one hemisphere will not be easily observable from the other.

This is comes about because Mercury always lies close to the line of the ecliptic, shown in yellow in the planetarium above. This is the line through the zodiacal constellations that the Sun follows through the year, and marks the flat plane in space in which all of the planets circle the Sun.

When Mercury remains in the sky for a few hours after the Sun has set, its altitude above the horizon depends on two factors.

One is its angular separation from the Sun. But equally important is how steeply the line of the ecliptic is inclined to the horizon.

If Mercury is widely separated from the Sun along the ecliptic, this may not translate into a high altitude if the ecliptic meets the horizon at a very shallow angle, running almost parallel to it.

Conversely, if the ecliptic is almost perpendicular to the horizon, a much smaller separation from the Sun may place Mercury higher in the sky.

The inclination of the ecliptic plane to the horizon at Ashburn varies between 74° (sunset at the spring equinox) and 27° (sunset at the autumn equinox). On November 23, the ecliptic is inclined at 36° to the western sunset horizon, as shown by the yellow line in the planetarium view above, meaning that on this occasion Mercury is poorly placed for viewing from Ashburn.

The sky on 23 November 2017
Sunrise 07:00
Sunset 16:49
Twilight ends
18:23
Twilight begins
05:27

5-day old moon
Age of Moon
5 days

All times shown in EST.
Rise Culm. Set
Mercury 08:56 13:28 17:59
Venus 06:03 11:10 16:16
Moon 11:05 16:05 21:05
Mars 03:32 09:13 14:54
Jupiter 05:09 10:27 15:45
Saturn 08:58 13:44 18:29

Source

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

23 Nov 2017, 21:22 EST  –  Mercury at greatest elongation east
01 Jan 2018, 19:40 EST  –  Mercury at greatest elongation west
15 Mar 2018, 06:18 EDT  –  Mercury at greatest elongation east
29 Apr 2018, 11:06 EDT  –  Mercury at greatest elongation west

Image credit

© NASA/JPL/MESSENGER

Ashburn

Latitude:
Longitude:
Timezone:

39.04°N
77.49°W
EST

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