|Thu, 19 Jan 2017 at||08:45 EST||(2 days away)|
Dominic Ford, Editor
From the Inner Planets feed
Mercury will be well placed for observation in the dawn sky, shining brightly at mag -2.0.
From Newark (click to change), it will be difficult to observe as it will appear no higher than 10° above the horizon. It will rise at 05:40 (EST) – 1 hour and 36 minutes before the Sun – and reach an altitude of 10° above the south-eastern horizon before fading from view as dawn breaks at around 06:56.
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 24° to the Sun's west.
Mercury in coming weeks
The key moments in this apparition of Mercury are as follows:
|28 Dec 2016 13:41 EST||– Mercury at inferior solar conjunction|
|11 Jan 2017 06:29 EST||– Mercury at greatest brightness|
|13 Jan 2017 17:02 EST||– Mercury at dichotomy|
|19 Jan 2017 08:45 EST||– Mercury at greatest elongation west|
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 before sunrise Mercury will rise each night; all times are given in Newark local time.
|Altitude of Mercury
|Direction of Mercury
|12 Jan 2017||07:18||05:40||14°||west|
|19 Jan 2017||07:15||05:41||13°||west|
|26 Jan 2017||07:10||05:51||11°||west|
|02 Feb 2017||07:04||06:02||9°||west|
|09 Feb 2017||06:57||06:13||6°||west|
|16 Feb 2017||06:48||06:21||3°||west|
|23 Feb 2017||06:38||06:26||1°||west|
|02 Mar 2017||06:28||06:29||-1°||west|
|09 Mar 2017||06:17||06:30||-3°||west|
|16 Mar 2017||07:05||07:30||-5°||west|
|23 Mar 2017||06:54||07:26||-6°||west|
A graph of the angular separation of Mercury from the Sun around the time of greatest elongation is available here.
The position of Mercury when it reaches greatest elongation will be:
|Object||Right Ascension||Declination||Constellation||Magnitude||Angular Size|
The coordinates above are given in J2000.0.
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 rises a few hours ahead of the Sun, the altitude it reaches Mercury above the horizon before sunrise 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 Newark varies between 72° (sunrise at the autumn equinox) and 25° (sunrise at the spring equinox). On January 19, the ecliptic is inclined at 33° to the eastern dawn horizon, as shown by the yellow line in the planetarium view above, meaning that on this occasion Mercury is poorly placed for viewing from Newark.
|The sky on 19 January 2017|
All times shown in EST.
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.
|19 Jan 2017, 08:45 EST||– Mercury at greatest elongation west|
|07 Mar 2017, 19:15 EST||– Mercury at superior solar conjunction|
|23 Mar 2017, 02:37 EDT||– Mercury at greatest brightness|
|30 Mar 2017, 01:32 EDT||– Mercury at dichotomy|