First, read this page! That's what it's here for! The answers to nearly all of the questions people email to me are on this page, and that makes me very angry... very angry indeed! But, if after reading this page, you still have a question, send it to me!
How does a clock measure the time of day on Mars?
Does Mars have seasons like we do on Earth?
How does the eccentricity of Mars' orbit affect the seasonal variations?
What is an analemma, and what do the analemmas of Earth and Mars look like?
Would an Earth calendar work on Mars? What would be the problems of working with an Earth calendar?
Is there a generally accepted standard Martian calendar?
What factors would need to be considered to develop a Martian calendar?
What advantages would a Martian calendar have over an Earth calendar?
Would weeks contain seven sols or some other number?
Does a Martian calendar need months, or other units between day and year?
If you kept the same number of Earth months, what would you have to do?
If you gave the calendar more months, how would you determine the number of months?
How do the lopsided seasons on Mars affect choices for dividing the year into months?
What are some ideas for naming months?
Acknowledgements
Some of the following questions appear on the Martian Calendar Lesson Plan developed by the Center for Educational Resources (CERES) Project at Montana State University. Other contributors are Lance Latham, Alan Hensel, Anton Sherwood, Mike Kretsch, and Chris Hirata.
How long is a day on Mars?
Just about any astronomy book will tell you that the rotational period of Mars is 24.6229 hours, or 24 hours, 37 minutes. However, note that the same table also gives Earth’s rotational period as 23 hours 56 minutes. But isn’t Earth’s day 24 hours long? What happened to the missing four minutes? The difference is that the 23 hours 56 minute figure is a sidereal day, i.e., Earth’s rotation is measured from the point of view of a fixed reference angle. But as Earth turns once on its axis, it also moves along its orbit around the sun, and the direction from the Earth to the sun changes slightly. It takes Earth an extra four minutes to rotate through this additional angle, and so Earth’s solar day, measured from the point of view of the sun, is 24 hours.
The same principle applies to Mars. Although the sidereal day is 24 hours, 37 minutes, the solar day (known as the "sol") is 24 hours, 39 minutes, 35.24409 seconds (88775.24409 seconds).
However, this is the mean length of the sol. The actual length of the sol varies throughout the Martian due to the combined effects of the axial inclination and the orbital eccentricity. A sol can be as short as 88752.33 seconds and as long as 88818.89 seconds (see figure), difference of just over a minute.
See also "What is an analemma, and what do the analemmas of Earth and Mars look like?"
How does a clock measure the time of day on Mars?
Several ideas have been put forth regarding Martian clocks. Since a Martian sol is only three percent longer than an Earth day, the most straightforward approach is to simply stretch Earth’s units of time into slightly longer hours, minutes, and seconds (this system is used by NASA and JPL). Another approach is to add 39 minutes, 35.2 seconds at the end of 24 hours. Still another idea is to have a "metric" clock based on powers of ten.
How long is a year on Mars?
Just about any astronomy book will tell you that the orbital period of Mars is 686.9726 days. But this measurement is in 24-hour Earth days, not Martian sols, which are almost forty minutes longer. If you lived on Mars, you would count 668.5921 sols from one vernal equinox to the next.
The axis of Mars precesses through one complete cycle over a period of 93,000 Martian years (175,000 Terran years). This causes the tropical year to be longer than the sidereal year by 0.0072 Martian day (0.0074 Earth day).
There is also a 43,000 Martian year (81,000 Terran year) precession of the Martian orbit. The perihelion advances due to the gravity of Venus, Earth, and Jupiter. Thus the anomalistic year is 0.016 days longer than the sidereal year.
Does Mars have seasons like we do on Earth?
Seasons are caused by the inclination of a planet’s rotational axis relative to the plane of its orbit around the sun. Earth’s axis is inclined 23.5 degrees. On the first day of summer in the northern hemisphere, Earth’s north pole is tilted 23.5 degrees toward the sun, so the northern hemisphere receives more sunlight. Half a year later, on the first day of winter, Earth’s north pole is tilted away from the sun, so the northern hemisphere receives less sunlight.
The rotational axis of Mars is inclined 25.192 degrees relative to the plane of its orbit around the sun, so like Earth, Mars experiences seasons.
How does the eccentricity of Mars' orbit affect the seasonal variations?
Earth’s orbit is very nearly circular, and so the four seasons last approximately the same number of days. The orbit of Mars, however, is a bit more eccentric (0.0934). In accordance with Kepler’s laws of orbital motion, Mars travels more slowly in its orbit when it is further from the sun, and more quickly when it is nearer to the sun. Mars reaches its furthest point from the sun (called "aphelion") when it is spring in the northern hemisphere. This has the effect of making spring the longest season (193.30 sols), and summer the second longest (178.64 sols). Mars reaches its closest point to the sun (called "perihelion") when it is autumn in the northern hemisphere, and consequently autumn is the shortest season (142.70 sols), and winter is the second shortest (153.94 sols). Take a look at this figure. Notice that on a calendar containing 24-months of equal duration, spring (green) contains seven months, while autumn (orange) contains a little more than five. Summer (yellow) has a little more than six months, and winter (blue) has a little less.
What is an analemma, and what do the analemmas of Earth and Mars look like?