SkyEye

The upper chart shows the path of Mercury across the background stars over the course of the year. Stars to magnitude +4.5 are shown with some fainter objects included to complete constellation patterns. The white circles represent the planet on the first day of the month and are scaled according to apparent magnitude. The faint paths before the first circle and after the last circle represent the planet's positions in December of last year and January of next. In general, the planet moves from right to left except when it's in retrograde and proceding in the opposite direction. As an inferior planet, Mercury never strays far from the Sun so it always begins and ends the year near the constellation of Sagittarius, located about one quarter of the way in from the left side of the chart.

The lower charts show how the appearance of Mercury changes over the year. Below each image is listed the date, the apparent magnitude, the apparent diameter of the disk (in arc-seconds), the geocentric distance (in au), the elongation from the Sun (in degrees) and the percentage of the disk which is illuminated. Like the Moon, Mercury exhibits a complete range of phases, from new to crescent to gibbous to full and back again. Because its synodic period is around four months, Mercury completes this phase cycle three times each year. Note how Mercury's magnitude varies widely, ranging (approximately) from −2.0 to +6.0 between conjunctions.

Mercury's first appearance in 2023 is in the west after sunset but it soon vanishes from the scene, to reappear in the morning sky. There are three more complete evening apparitions, with mid-March through May favouring northern temperate latitudes and July–September bringing the best viewing opportunities in tropical and southern regions. The first morning apparition (mid-January to mid-March) is slightly better than the following morning appearance (May–June) for equatorial regions, but the May–June apparition favours the southern hemisphere whilst the September to mid-October appearance is the best one for northern observers. The final morning apparition gets underway just as the year ends.

• Apparitions of the Inferior Planets from Latitude 50° North
• Apparitions of the Inferior Planets from Latitude 10° North
• Apparitions of the Inferior Planets from Latitude 30° South

Sources

The dates, times and circumstances of all planetary and lunar phenomena were calculated from the JPL DE406 solar system ephemeris using the same rigorous methods that are employed in the compilation of publications such as The Astronomical Almanac.