Sol (day on Mars)
Sol (borrowed from the Latin word for sun) is a Mars solar day; that is, a Mars-day. A sol is the apparent interval between two successive returns of the Sun to the same meridian (sundial time) as seen by an observer on Mars. It is one of several units for timekeeping on Mars. The sol was originally adopted in 1976 during the Viking Lander missions and is a measure of time mainly used by NASA when, for example, scheduling the use of the Mars rover.
The sidereal rotational period of Mars—its rotation compared to the fixed stars—is only 24 hours, 37 minutes and 22.66 seconds. The solar day lasts slightly longer because of its orbit around the sun which requires it to turn slightly further on its axis.
Usage in Mars landersEdit
When a spacecraft lander begins operations on Mars, the passing Martian days (sols) are tracked using a simple numerical count. The two Viking missions, Mars Phoenix and the Mars Science Laboratory rover Curiosity count the sol on which each lander touched down as "Sol 0", as does the InSight mission. Mars Pathfinder and the two Mars Exploration Rovers instead defined touchdown as "Sol 1". Generally speaking, the choice between counting from Sol 0 or Sol 1 is made so that Sol 1 would be the first sol with "meaningful" or "useful" lander operations. Thus, landers that touched down late in the Martian day begin their sol count at 0, while those that touch down early in the day begin their count at 1.
Although lander missions have twice occurred in pairs, no effort was made to synchronize the sol counts of the two landers within each pair. Thus, for example, although Spirit and Opportunity were sent to operate simultaneously on Mars, each counted its landing date as "Sol 1", putting their calendars approximately 21 sols out of sync.
Mars Sol DateEdit
On Earth, astronomers often use Julian Dates—a simple sequential count of days—for timekeeping purposes. "For historical utility with respect to the Earth-based atmospheric, visual mapping, and polar-cap observations of Mars…, a sequential count of sol-numbers" the Mars Sol Date (MSD) was proposed starting "prior to the 1877 perihelic opposition." This Mars Sol Date (MSD), is a running count of sols since December 29, 1873 (coincidentally the birth date of astronomer Carl Otto Lampland). The Mars Sol Date is defined mathematically as MSD = (Julian Date using International Atomic Time - 2451549.5 + k)/1.02749125 + 44796.0, where k is a small correction of approximately 0.00014 d (or 12 s) due to uncertainty in the exact geographical position of the prime meridian at Airy-0 crater.
The word "yestersol" was coined by the NASA Mars operations team early during the MER mission to refer to the previous sol (the Mars version of "yesterday"), and came into fairly wide use within that organization during the Mars Exploration Rover Mission of 2003. It was eventually picked up and used by the press. Other neologisms include "tosol" (for "today" on Mars), as well as one of three Mars versions of "tomorrow": "nextersol", "morrowsol", or "solmorrow". NASA planners coined the term "soliday" at least as far back as 2012 to refer to days off due to time phasing or the synching of planetary schedules.
Considering a possible colonization of Mars, one question that arose was "how does one convert a Sol to standard Earth time?" In the science fiction series Mars trilogy by Kim Stanley Robinson, the Mars settlers use traditional Earth watches that stop ticking at midnight for 39 minutes and 40 seconds before resuming their timekeeping. This creates something like a "witching hour" which compensates for the time difference between a Sol and an Earth day. This follows the method previously given by Philip K. Dick in his novel Martian Time-Slip.
An alternative idea was suggested in 1988 by David Powell (the Davidian Mars calendar). In this case the clocks simply run slower than the ones on Earth so that their hour hands complete two cycles per one Sol. For example, 1 Mars-second is 1.027 Earth-seconds, 1 Mars-minute is 61.62 Earth-seconds, and 1 Mars-hour is 61 minutes and 36.968 Earth-seconds.
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