- PAGE F 24, 46-50, /D 24-29/ ... PAGE F 24, 46-50, /D 24-29/ A/ 9.9.16.0.0 4 Ahau 8 ...
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PAGE F 24,
46-50, /D 24-29/
A/
9.9.16.0.0 4 Ahau 8 Cumuku
1,366,560 days
- 6.2.0 - 2,200 days
B/ 9.9.9.16.0 1 Ahau 18 Kayab
1,364,360 days
C/
/9.14.2.6.0/ 1 Ahau 18 Uo
1,397,640 days
A/ J.D.
1,988,821 February
4, 733
B/ J.D.
1,986,621 January
27, 727
C/ J.D.
2,019,901 March
10,818
The rounded length of Venus synodic circulation of 584
days multiplied by five are added to the dates B and C 5-65 times and 130; 195
and 260 times. The real length of synodic circulation of Venus is 583.921
394 days. Time intervals of 185,120; 68,900; 33,280 and 9,100 days are added to
the number B. And again the upper mentioned multiplies of 584 days. The total
of B and interval of 33.280 days is the same as the date C, in the Dresden
Codex mentioned only by the dates of calendar circle – 1 Ahau 18 Uo.
The total of B and 68,900 or B and 9,100 days is forming
next dates D and E. Their last day always falls on 1 Ahau from 260 day tzolkin,
as stressed in the Codex table.
B/ 9.9.9.16.0 1 Ahau 18 Kayab 1,364,360 days
9.11.7.0
68,900 days
D/
/9.19.1.5.0/ 1 Ahau 1,433,260
days
B/ 9.9.9.16.0 1 Ahau 18 Kayab 1,364,360 days
1.5.5.0
9,100 days
E/
/9.10.15.3.0/ 1 Ahau
1,373,460 days
D/
J.D.
2,055,521
September 17, 915
E/ J.D.
1,995,721 December 27, 751
The rounded length
of synodic circulation of Venus multiplied by five is 2,920 days. They
contain:
5 times the length
of synodic circulation of Venus
13 times the length of siderialal circulation of Venus
8 times the length
of tropical year
2,920 days is the typical period when the
siderialal and sinodical circulation of Venus meet the tropical year. In
this time the planet sets or rises in the same place in the sky after 8 years.
Venus
visibility ephemerides are mentioned in the next Codex tables. Its synodic
circulation length is written like five times /236 and 90 and 250 and 8 days/. These are comprehensible
approximate values, because of the synodic circulation length of this planet is
moving between 577 and 592 days.
236 days - Venus is in the eastern sky as a morning star
90 days - Venus
is around the upper conjunction with the Sun and not visible
250 days - Venus is in the western sky as an evening
star
8 days - the
Venus is around the lower conjunction with the Sun and not visible
This specification is added to dates B and D five times.
Dates B, C and D
are concerning the moment of Venus first observation as a morning star
after its lower conjunction with the Sun.
Date E is
concerning the moment of Venus first observation as an evening star after
tens of days of invisibility because of its upper conjunction with the Sun.
B/ January 27, 727
The
Venus is 8 days after the lower conjunction with the Sun. For first time observed as a morning star in the eastern sky.
The
Venus rose at 5.39 am
The
Sun rose at 6.34 am
C/ March 10, 818
The
Venus is five days after its lower conjunction with the Sun. For the first time
observed as a morning star in the eastern sky.
Venus rose at 5.36 am
The Sun rose at 6.11 am
D/
September 17, 915
Venus is
six days after its lower conjunction with the Sun. For the first time observed as a morning star in the eastern
sky.
Venus rose at 4.54 am
The Sun rose at 5.49 am
E/ December 27, 751
Venus is 63 days after upper conjunction with the Sun. For the first
time observed as an evening star in the
western sky.
The Sun set at 5.42 p.m.
The
Venus set at 6.46 p.m.
There is a time
interval of 2,200 days marked between dates A and B. It contains:
19 times
the Mercury synodic circulation length
/115.877 484 days/
25 times
the Mercury siderialal circulation length /87.968 581 days/
6 times the tropical year /365.242 199 days/
2,200
days is the typical period when the siderialal and sinodical circulation
of the Mercury meet the tropical year. In this time the planet sets or rises in
the same place in the sky after 6 years. The similar cyclical regularity was
observed by the Mayan astronomers about Venus, with a period of 2,920 days.
The dates A and B are marking the moments when the Mercury was to be found in a
close approach of the maximal western elongations from the Sun. The D date
concerns the maximal eastern elongation. Only in those positions around the
maximal elongations is the planet visible not long before the sunrise or
shortly after the sunset.
A/ February 4, 733
The
Mercury is to be found in western elongation with angle distance 26.47 degrees
from the Sun.
The
Mercury rose at 4.53 am
The
Sun rose at 6.32 am
The
maximal western elongation of 26.73 degrees was on January 31, 733. The
difference between determined and real elongation is 0.26 degrees.
B/ January 27, 727
The
Mercury was in western elongation with angle distance 25.5 degrees from the Sun.
The
Mercury rose at 4.55 am
The
Sun rose at 6.34 am
The
maximal western elongation of 26.07 degrees was on January 21, 727. The
difference between determined and real elongation is 0.57 degrees.
D/ September 17, 915
The
Mercury was in eastern elongation with angle distance 25.05 degrees from the Sun.
The
Mercury set at 7.10 p.m.
The
Sun set at 5.57 p.m.
The
maximal eastern elongation 25.12 degrees occurred just few hours later.
The
autumn equinox.
In all three determined elongations the Mayan astronomers have made an
average mistake 0.3 degrees less than reality. It is so slight difference that
it can’t have been
discovered.
E/ December 27, 751 The conjunction of Venus, Mercury and
Jupiter. The position of planets is expressed in degrees of geocentrical
ecliptical coordinates:
The
Mercury 295.489
The
Venus 294.289
The
Jupiter 294.987
The time interval 2,200 days between A and
B dates contains 74.5 times the length of synodic circulation of the Moon /29.530 588 days/.
A/
February 4, 733 The fullmoon
B/
January 27, 727 The newmoon