A Possible Solution of the Number Series on Pages 51 to 58 of the Dresden CodexGuthe, Carl E. (Carl Eugen)
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A Possible Solution of the Number Series on Pages 51 to 58 of the Dresden Codex
Guthe, Carl E. (Carl Eugen)
Codex Dresdensis Maya
Upper Month
number number Interval Groups
502 17
59 \
2244 76 | 94(47 + 47)
35 /
3278 111
41 41
4488 152
59 \
6230 211 | 94(47 + 47)
35 /
7264 246
41 41
8474 287
53 \
10039 340 | 94(47 + 47)
41 /
11250 381
The next logical step is a comparison between the theoretical calendars
just described and the manuscript. A study of the manuscript reveals
that: (1) the series recorded represents 405 lunar months or three times
135 months, and that the series naturally falls into three great
subdivisions of 3986 days each; (2) each third consists of 23 columns
or unequal subdivisions; (3) the intervals between the 178-day groups
are 47 and 88 months; (4) the 148-day groups fall approximately at 47
and 41 month intervals (see Table X); (5) the first 178-day group in
each third occurs between the 30th and 35th month inclusive, and the
other 178-day group of the third comes 47 months later. Since the number
178 is composed of four 30-and two 29-day months, an extra day must have
been added, that is, a 30-day month was substituted for one of the
29-day months, if the manuscript represents a regular alternating
series.
The obvious conclusions to be drawn from these facts are: (1) that the
series was divided into three groups of 3986 days each in order to
associate the lunar calendar closely with the ecliptic cycle of the same
length; (2) that the 23 columns in each third may represent the
twenty-three eclipse seasons in each eclipse period of 3986 days; (3)
that groups of 47 and 41 months were used in some way in the series, for
the 178-day groups are separated by 47 and 88 months and 88 is composed
of 47 and 41, the two periods so closely associated with the recurrence
of eclipses; (4) that the six months period was changed to one of five
months of 148 days approximately every 47 and 41 months, which is the
method already advanced in the theoretical ecliptic lunar series for
keeping the synodical months and ecliptic seasons together; (5) that one
extra day was added to the alternating 29-and 30-day months, between the
30th and 35th month inclusive of each third, in accordance with the
theoretical necessity for so doing already brought out, and that another
of the three extra days was added 47 months later.
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