Emily LakdawallaMar 09, 2011

Martian timekeeping

While scanning through the talks scheduled for this week's Lunar and Planetary Science Conference I came across the following talk title: "Interannual and Seasonal Variability in the North Polar Region of Mars: Observations in Mars Years 29 and 30 by MARCI, CTX, and CRISM." My first thought was "hey, cool research spanning a long time period and across data sets." But my second was "Mars years 29 and 30? What does that mean?"

Mars 3 arrives to a dust-shrouded planet
Mars 3 arrives to a dust-shrouded planet When the Russian orbiter Mars 3 arrived at Mars late in 1971, it found the surface of the planet to be almost completely obscured by an enormous global dust event. Several months later, the sky was finally clear enough to reveal surface features. The image on the left was captured on December 12, 1971, and the one on the right on February 28, 1972. Russian Academy of Sciences / Ted Stryk

Clearly it's a way of marking the passage of time on Mars, but I didn't recall seeing such a thing used in an academic paper before. The agreed-upon method (where "agreed-upon" means "used by scientists publishing peer-reviewed papers") of marking time within a single Mars year is something called "Ls," read "ell sub ess," which is short for "solar longitude." Ls marks Mars' position in its orbit around the Sun, measured in degrees, from 0 to 360. As I explained on this webpage, Ls is 0° at the vernal equinox (beginning of northern spring), 90° at summer solstice, 180° at autumnal equinox, and 270° at winter solstice. Dust activity tends to peak a bit before the northern winter solstice, around 260°, though it can happen any time of the Martian year.

But that calendar resets with each of Mars' elliptical orbits around the Sun. Clearly "Mars years 29 and 30" refers to a way to count up the orbits, and it doesn't take much effort to deduce that it's counting up from some point in time near the start of the Space Age. A little bit of digging led me to a 2000 paper by Todd Clancy and several coauthors: "An intercomparison of ground-based millimeter, MGS TES, and Viking atmospheric temperature measurements: Seasonal and interannual variability of temperatures and dust loading in the global Mars atmosphere," which states:

For the purpose of this comparison, we use the solar longitude range 0°-360° to define a Mars year and adopt April 11, 1955 (Ls=0°) as the beginning of year 1. In this arbitrary convention, the Mariner 9, Viking, Phobos, and Pathfinder missions occurred in years 9-10, 12-15, 19-20, and 23, respectively. By comparison, the 1992-1999 [Earth-based] millimeter observations extend over years 21-24, and the 1997-1999 [Mars Global Surveyor] TES observations extend over years 23 and 24.

The convention is described again in a 2010 paper by Bruce Cantor, Philip James, and Wendy Calvin: "MARCI and MOC observations of the atmosphere and surface cap in the north polar region of Mars," which includes a handy-dandy lookup table for Earth dates corresponding to Mars' seasons:

Martian years and start dates of northern hemisphere seasons
Mars yearSpring equinox
Ls = 0°)
Summer solstice
Ls = 90°)
Autumnal equinox
Ls = 180°)
Winter solstice
Ls = 270°)
0104-11-195510-27-195504-27-195609-21-1956
0202-26-195709-13-195703-15-195808-09-1958
0301-14-195908-01-195901-31-196006-26-1960
0412-01-196006-18-196112-18-196105-14-1962
0510-19-196205-05-196311-05-196303-31-1964
0609-05-196403-22-196509-22-196502-15-1966
0707-24-196602-07-196708-10-196701-03-1968
0806-10-196812-25-196806-27-196911-20-1969
0904-28-197011-12-197005-15-197110-08-1971
1003-15-197209-29-197204-01-197308-25-1973
1101-31-197408-17-197402-17-197507-13-1975
1212-19-197507-04-197601-04-197705-30-1977
1311-05-197705-22-197811-22-197804-17-1979
1409-23-197904-08-198010-09-198003-04-1981
1508-10-198102-24-198208-27-198201-20-1983
1606-28-198301-12-198407-14-198412-07-1984
1705-15-198511-29-198506-01-198610-25-1986
1804-01-198710-17-198704-18-198809-11-1988
1902-16-198909-03-198903-06-199007-30-1990
2001-04-199107-22-199101-22-199206-16-1992
2111-21-199206-08-199312-08-199305-04-1994
2210-09-199404-26-199510-26-199503-21-1996
2308-26-199603-13-199709-12-199702-06-1998
2407-14-199801-29-199907-31-199912-25-1999
2505-31-200012-16-200006-17-200111-11-2001
2604-18-200211-03-200205-05-200309-29-2003
2703-05-200409-20-200403-22-200508-16-2005
2801-21-200608-08-200602-07-200707-04-2007
2912-09-200706-25-200812-25-200805-21-2009
3010-26-200905-13-201011-12-201004-08-2011
3109-13-201103-30-201209-29-201202-23-2013
3207-31-201302-15-201408-17-201401-11-2015
3306-18-201501-03-201607-04-201611-28-2016
3405-05-201711-20-201705-22-201810-16-2018
3503-23-201910-08-201904-08-202009-02-2020
3602-07-202108-25-202102-24-202207-21-2022
3712-26-202207-12-202301-12-202406-07-2024
3811-12-202405-29-202511-29-202504-25-2026
3909-30-202604-16-202710-17-202703-12-2028
4008-17-202803-03-202909-03-202901-28-2030

I haven't seen this convention used very often, but then there are not very many people who publish research that requires referring to years beyond the span of a given mission. Really it's just people who care about Mars' year-to-year weather who actually need to apply this convention. But it's not just climatologists who care about interannual weather variability; those of us who follow the adventures of landed Mars missions care about variations in weather, too. So, adopting this convention for naming the Martian years, and using solar longitude as the most accepted method of marking time within a year, here's a Martian timeline of interesting events in Mars exploration. And thanks to Aymeric Spiga for pointing out this handy online Earth-to-Mars date converter.

Earth DateMars
ear/Ls
Event
July 14, 19656.143Mariner 4 flyby
August 19698.200Mariner 6 and 7 flybys
November 19719.284Mariner 9, Mars 2, and Mars 3 enter orbit
August 197210.64Mars 2 and 3 shut down
October 27, 197210.102Mariner 9 shuts down
February 197411.0Mars 4 and 5 enter orbit
July 197612.88Viking 1 Orbiter & Lander arrive
September 197612.116Viking 2 Orbiter & Lander arrive
July 25, 197813.118Viking 2 Orbiter shuts down
April 11, 198014.91Viking 2 Lander shuts down
August 17, 198014.151Viking 1 Orbiter shuts down
November 13, 198215.226Viking 1 Lander shuts down
January 29, 198919.350Phobos 2 enters orbit
March 27, 198920.18Phobos 2 shuts down
July 4, 199723.142Mars Pathfinder lands
September 199723.173Mars Global Surveyor enters orbit; Mars Pathfinder shuts down
October 24, 200125.258Mars Odyssey enters orbit
December 14, 200326.315Nozomi flies past Mars
January 200426.325Mars Express, Spirit, and Opportunity arrive
March 10, 200628.22Mars Reconnaisance Orbiter arrives
November 5, 200628.130Mars Global Surveyor shuts down
May 25, 200829.76Phoenix lands
November 2, 200829.151Phoenix shuts down
March 22, 201030.67Last contact with Spirit
March 9, 201130.251Today

So Mariner 4's images came from year 6, late in the northern summer. Mariner 6 and 7's images came a little more than two Mars years later, a little after the equinox had brought sunlight to the south pole and darkened the north. Mariner 9 and Mars 2 and 3 all arrived another Mars year later, year 9, right around the southern summer solstice; Mars 2 and 3 lasted through the next equinox, and Mariner 9 through the next solstice. Mars 4 and 5 arrived right at the northern vernal equinox in year 11.

The Vikings came in year 12, around the northern summer solstice, so they saw a very differently lit Mars to what Mariner 9 imaged, at least at first. Of course those missions also lasted a long time. Viking 2 Orbiter lasted almost exactly one Mars year; Viking 2 Lander and Orbiter about two Mars years; and Viking 1 lander an amazing three and a half Mars years, most of the way through year 15.

There followed a long drought in the Mars program. Phobos 2's brief mission came around the equinox beginning year 20, but that was the only mission at Mars in the period from year 16 through year 22.

The resurgence of Mars science began midway through year 23, very late in northern summer, when Mars Pathfinder landed. It survived until close to the northern autumnal equinox, when Mars Global Surveyor arrived. That orbiter was still active near the southern summer solstice in year 25, when Odyssey joined the party; and both were active late in the southern summer of year 26 when a flotilla of spacecraft (Nozomi, Mars Express, and the Mars Exploration Rovers) flew past, entered orbit, or landed. Spirit lasted through at least three and a half Mars years. All the rest of the orbiters except Mars Global Surveyor are still operating now, late in the southern spring of Mars year 30.

What do you think? Is this a valuable way of looking at Mars time?

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