Space Station >> Observing Mercury

Observing Mercury

Mercury's Caloris Basin is one of the largest impact features in the Solar System.

Observation of Mercury is complicated by its proximity to the Sun, as it is lost in the Sun's glare for much of the time, and at most other times can be observed for only a brief period during either morning or evening twilight.

Like Venus, Mercury exhibits moon-like phases as seen from Earth, being "new" at inferior conjunction and "full" at superior conjunction, rendered invisible on both of these occasions by virtue of its rising and setting in concert with the Sun in each case. The half-moon phase occurs at greatest elongation, when Mercury rises earliest before the Sun when at greatest elongation west, and setting latest after the Sun when at greatest elongation east (its separation from the Sun ranging from 18.5° if it is at perihelion at the time of the greatest elongation to 28.3° if at aphelion).


Unlike Venus, which is brightest when it is between new and half full, Mercury is brightest as seen from Earth when it is at a "gibbous" phase, between half full and full. This is because Venus is much closer to the Earth when in its crescent phase than it is in its gibbous phase, while Mercury's smaller orbit means it is not much further away and the fuller phase more than outweighs its greater distance from Earth.

Mercury attains inferior conjunction every 116 days on average, but this interval can range from 111 days to 121 days due to the planet's eccentric orbit. Its period of retrograde motion as seen from Earth can vary from 8 to 15 days on either side of inferior conjunction, this large range also arising from the planet's high degree of orbital eccentricity.

Mercury is more often easily visible from the Earth's Southern Hemisphere than from its Northern Hemisphere; this is due to the fact that its maximum possible elongations west of the Sun always occur when it is early autumn in the Southern Hemisphere, while its maximum possible eastern elongations happen when the Southern Hemisphere is having its late winter season. In both of these cases, the angle Mercury strikes with the ecliptic is maximized, allowing it to rise several hours before the Sun in the former instance and not set until several hours after sundown in the latter in countries located at South Temperate Zone latitudes, such as Argentina and New Zealand. At northern temperate latitudes, by contrast, Mercury is never above the horizon of a more-or-less fully dark night sky.

Mercury can, like several other planets and the brightest stars, be seen during a total solar eclipse.