ESSAYS FROM ARCHAEOASTRONOMY & ETHNOASTRONOMY NEWS, THE QUARTERLY BULLETIN OF THE CENTER FOR ARCHAEOASTRONOMY
Number 3 March Equinox 1992
To the Limits
by David Dearborn
Few would doubt that Native American groups employed lunar calenders
recognizing that some years contained 12 full moons while others had 13. This
requires a recognition of the synodic month, 29.5 days, and the length of the
year, 365 days. The Maya, with their interest in astronomy, determined a great
deal more. The eclipse table of the Dresden Codex contains the number 177 in a
long series, with an occasional 148 and 178. Simply averaging this series
results in a value of 173.31, the number of days between eclipse seasons, or
half the Eclipse year. As eclipses occur only at new or full moon, the 177's
(and occasional 178) are easily understood as the number of days between 6 full
(or new) moons, or the time between a pair of eclipses. As this period is 4
days longer than the 173 days separating the eclipse seasons, a series of
eclipses beginning near the start of an eclipse season will advance through
subsequent seasons until it occurs near the end. When this happens, the next
eclipse will occur after only 5 synodic months (148 days), at the beginning of
the next eclipse season.
The time between eclipse seasons results from the 18.61 year precession
of the moon's orbit. This precession advances the locations where the moon's
orbit crosses the ecliptic (the nodes). Eclipses will occur on the new or full
moon nearest the time that the sun passes one of the nodes. Because of
precession, the time for the sun to move from one node to another is only
173.31 days.
One must consider how the Maya determined this 173.31 day period. It
can be derived from a long-term record of eclipse data, but such data would
certainly be incomplete, as not all eclipses would have been visible to the
Maya. A directly related observation that could have provided the Maya with a
clue to the precession of the moon's orbit is the dramatic change in the moon's
monthly rise (or set) point. As the moon's orbit precesses, its monthly
declination range changes from +/- 18 degrees at minor standstill to +/- 28
degrees at major standstill, 9.3 years later. This causes a variation in the
azimuth limits of moon rises (and sets) of about 10 degrees in tropical regions
(more in temperate ones).
Evidence is accumulating that Native Americans living in what is now
the United States monitored this 18.61 year precession period of the moon.
Foremost among this is the work of J. McKim Malville at Chimney Rock published
in Archaeoastronomy, no 16 (JHA, xxii(1991). The Chimney Rock Pueblo, 5AA83,
is a Chaco outlier located such that the major northern standstill of the moon
was observable between the prominent double chimney feature on the horizon.
Dendro-dates show occupation and construction activity coincident with
standstill dates in 1076 and 1093. This supports the suggestion by Anna
Sofaer, Rolf Sinclair, and LeRoy Doggett for a lunar standstill marker at
Fajada Butte (in Archaeoastronomy in the New World, 1981, ed. Aveni), and
recent work by Anna on the orientation of major Chacoan structures reported at
Oxford 3, and as yet unpublished. There would be little question of the
significance of these alignments if they were corroborated with ethnographic
data from Pueblo cultures. Such ethnographic evidence has been sought, but not
found. Steve Mclusky (in World Archaeoastronomy, p. 362) has noted that
certain irregularities in the Zuni scheduling of Shalako can be understood if
they were influenced by the position of moon rise, but this data do not resolve
the question of whether or not they were aware of lunar standstills.
Additional evidence suggesting Native American interest in lunar
standstills has been gathered by Bill Romain (see articles listed in new
publications). He proposes alignments to lunar standstills in a number of
Hopewell earthworks. Unfortunately the current state of most Hopewell sites
does not permit great accuracy for individual measurements, but perhaps the
growing data base on these sites will permit a statistical investigation to
test the hypothesis that the alignments are intentional.
While the present evidence that Native American cultures of the United
States were monitoring the 18.61 year cycle of the moon by means of the lunar
standstills is not compelling, it is reasonably suggestive. The existence of
contact between the Southwest and Mexico adds plausibility to the hypothesis
that Southwestern groups knew of lunar standstills, or at least the existence
of long-term cycles of the moon. This appears to be a developing area of
inquery, that could benefit from a survey of Mexican and Mayan sites to
determine the nature of the lunar observations that they must have made.