Mercury will reach half phase in its Feb–Mar 1995 morning apparition. It will be shining brightly at mag 0.1.
Feb–Mar 1995 morning apparition of Mercury
|03 Feb 1995||–||Mercury at inferior solar conjunction|
|22 Feb 1995||–||Mercury at highest altitude in morning sky|
|24 Feb 1995||–||Mercury at dichotomy|
|01 Mar 1995||–||Mercury at greatest elongation west|
A graph of the phase of Mercury is available here.
Apparitions of Mercury
|26 Sep 1994||–||Evening apparition|
|05 Nov 1994||–||Morning apparition|
|19 Jan 1995||–||Evening apparition|
|01 Mar 1995||–||Morning apparition|
|11 May 1995||–||Evening apparition|
|29 Jun 1995||–||Morning apparition|
|08 Sep 1995||–||Evening apparition|
Mercury's orbit lies closer to the Sun than the Earth's, meaning that it always appears close to the Sun and is lost in the Sun's glare much of the time.
It is observable for only a few weeks each time it reaches greatest separation from the Sun – moments referred to as greatest elongation. These apparitions repeat roughly once every 3–4 months.
Mercury's 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 shows an intermediate half phase – called dichotomy – at roughly the same moment that it appears furthest from the Sun, at greatest elongation. The exact times of the two events may differ by a few days, only because Mercury's orbit is not quite perfectly aligned with the ecliptic.
The coordinates of Mercury when it reaches dichotomy will be:
|Object||Right Ascension||Declination||Constellation||Angular Size|
The coordinates above are given in J2000.0.
|The sky on 28 January 2022|
26 days old
All times shown in EST.
The circumstances of this event were computed using the DE430 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.
|22 Feb 1995||– Mercury at highest altitude in morning sky|
|01 Mar 1995||– Mercury at greatest elongation west|
|09 May 1995||– Mercury at highest altitude in evening sky|
|11 May 1995||– Mercury at greatest elongation east|