Astrophotography by Anthony Ayiomamitis

Solar System Image Gallery - Mercury

Aside from being the closest planet to the Sun, Mercury is only second to distant Pluto in being the smallest planet of our solar system. It rotates completely around the Sun once every 88 days and has such a slow rotation about its axis that a day on Mercury is greater in length than its year (ie. time required to orbit the Sun). The proximity of Mercury to the Sun is responsible for its characteristic surface which is completely covered with craters, for the immense gravitational force of the Sun attracts many comets and asteroids which inevitably also crash into Mercury due its close proximity to the Sun. At aphelion, Mercury reaches a temperature of 285C whereas during perihelion it surpasses 430C (7.5x the greatest temperature ever recorded on the surface of the Earth: 57.7C, Lybia, Sept 1922). In contrast, the temperature at night reaches -180C due to the absence of any atmosphere. The only satellite mission to Mercury was Mariner 10 which made three fly-bys between March 1974 and March 1975 when it photographed half its surface. One of the most dominant features encountered by Mariner 10 is a plateau measuring 1300 km in diameter and is most probably due to an impact from a 100-km wide asteroid travelling at 500,000 km per hour.

2003 Transit: I was most fortunate on May 7th, 2003 to be perfectly located for the Mercury transit against the sun. This event is relatively rare as it occurs, on average, about thirteen times each century. The transiting Mercury had an apparent diameter of only 12.0 arc-seconds or approximately 1/160th that of the sun. Table 1 below describes the various key stages of the transit (UT+3) whereas Table 2 provides a visual representation of these same events as well as a sequence of the complete 5-hr and 20-minute transit. Complete ingress, maximum and egress are based on integrations 60 seconds apart whereas the complete transit is based on 33 integrations spaced at ten-minute intervals and (very painfully) digitally processed and assembled. Clicking on any of the images below will permit for the assessment of the corresponding image in a larger format with complete imaging details.

Table 1
Key Events and Stages
External Ingress
Internal Ingress
Internal Egress
External Egress

Table 2
Transit Images in H-alpha
Ingress Sequence
Maximum Sequence
Egress Sequence

Copyright 2001-2005, Anthony Ayiomamitis. All rights reserved.