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Latitude Geometry and Astronomy
2009.04.04 - I've
discussed geodetic geometry of monument latitudes, 4/5 atan at Monks Mound, 3/5 atan atop Ur Ziggurat, 3:4:5 at Harran,
cir/7 in Avebury,
cir/14 at Karnak, and other sites. One of the oldest known stone
circles, situated one-fourth the distance from equator to pole at Nabta
Playa, Egypt, infers intentional latitude placement originates at an
early date. In contrast to simple integer ratios of spatial geometry,
the latitudes at Newark and Marietta present solar and lunar motion
modules (Table 2). Marietta's latitude equals 40 times solar orbit per
day (40 SO). The same astronomy module relates to Ur Ziggurat:
"Divide earth's
circumference by days per solar orbit (0.98561° = SO),
multiply by 10 pi, and the result is the latitude of the Ur ziggurat,
or 30.9638° = 31.4159 SO."
Marietta and Ur latitudes
equate at 4 to pi. Marietta latitude presents a low integer ratio for
days to lunar orbit motion. The latitude transecting the site equals three times lunar orbit per rotation (3
R27) and 40 times solar orbit per day (40 SO). Figure
1 illustrates the relationships of the monument to these latitudes about 322 A.D. The 40 SO - 3 R27 latitude difference equals 0.00322° or
358.6 m (also the diameter of the Great Circle). In 322 A.D. earth's
rotation axis was inclined 3/5th's of Marietta latitude, an arc equal
to 24 days of solar orbit, = 24 SO. The 55 SO latitude at Thornborough
equals eleven-eights Marietta's latitude.
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Table 2. Solar Orbit
Nodes
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Solar orbit modules,
heliocentric angles
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motion
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module
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circumference
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degrees
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day
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SO
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0.0027378
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0.985609
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lunar nodal period
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S22
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0.0745017
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26.820613
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lunar anomalistic
period
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S25
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0.0754389
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27.158012
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lunar synodic period
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S29
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0.0808489
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29.105618
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The Quadranau and Octagon
colatitudes (angle to the pole) express the ratio of the lunar nodal
and anomalistic periods, 1.0 : 1.012580. Thornborough latitude
expresses the ratio of lunar synodic period in relation to Newark and
Marietta colatitudes representing the nodal and anomalistic periods,
expressing S29:S22:S25. Table 3 compares these monument latitudes and
colatitudes.
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Table 3.
Monument Latitudes
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site
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latitude
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colatitude
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Thornborough
South
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1.8623 S29
54.995 SO
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35.79614°
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Newark Octagon
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40.05314°
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1.86226 S22
49.94686°
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Marietta Quadranau
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3.0002 R27
39.999 SO
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1.86229 S25
50.57620°
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Marietta Capitoleum
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3.0001 R27
39.998 SO
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1.86234 S25
50.57736°
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322 A.D.
tropical year - eclipse nodal period difference = 18.62277 days
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In a previous article, Thornborough Henges and the
Ure-Swale Monuments Assessing Evidence of Geospatial
Intelligence in the Neolithic, I noted arc distance from Newark to
Thornborough South is 2.0 times solar orbit per nodal period (S22), and
that Thornborough's latitude
equals 1.8623 times solar orbit per lunar synodic period (S29). Eclipse
cycles are intercalations of two lunar periods, the synodic and nodal
periods (Table 2). The multiple "1.8623 times" presents an astronomical
number; eclipse nodal period is 18.62277 days less than a tropical
year. Newark Octagon colatitude equals 1.86226 S22. Capitoleum
colatitude equals 1.86234 times lunar orbit per anomalistic period
(S25). The modules are each 1.8623 multiples of the three lunar periods.

Newark Earthworks and
the Lunar Standstill Period

2011.01.24
- The lunar standstill period results from the turning
of the axis of lunar orbit. Inclination of the earth's axis
(obliquity) together with solar orbit results in the sun rising and
setting north and south of due east and due west during the course of
each year. In the case of the moon, lunar orbit inclination either adds
to or subtracts from the moon's swing back and forth across the
celestial equator. Unlike the sun, the moon shifts north and
south on the horizon every 27.22 days (the lunar nodal period).
The moon's maximum rise-set angle from east-west recurs in a mean
period of
18.613 years, one lunar standstill and just over one turn in
space of the direction of the lunar orbit axis.
One long-standing interpretation of Newark Octagon is
intentional alignments to the lunar standstill rise and set
extrema. The hypothesis first appeared in John A. Eddy's article Archaeoastronomy of
North America: Cliffs, Mounds, and Medicine Wheels (in In Search of Ancient Astronomies,
1978, E.C. Krupp, editor). Eddy's map examination revealed the
alignment as
possible. Hively and Horn's survey (1982) determined
standstill rising and
setting positions coincide with the architecture of the
earthwork. Azimuth identifies horizontal direction, while
elevation
corresponds to vertical direction. The azimuths of the octagon sides
closely correlate with the lunar standstill horizon extrema as observed
in
the three-dimensional landscape surrounding the Octagon. Most
importantly, the
primary axis of the entire earthwork (octagon, circle, and connecting
parallel walls) aligns to the lunar major moonrise, the northern-most
moonrise position of each standstill (arrow in image above). I
discuss details and other
possible interpretations of the Octagon Earthwork primary
alignment in Temporal Epoch Calculations.
Recently, Google Earth updated some Andean areas with
high-resolution imagery. One of the important sites now visible
in
detail is a UNESCO
World
Heritage
site, the Chavin
Archaeological Site in Peru. The Google Earth illlustration below
incorporates an
image overlay of CyArk's
archaeology map. While ground-truthing with GPS
equipment needs to be accomplished
for precise coordinates, especially when rugged Andean terrain is
combined with oblique camera angles, reasonably accurate
coordinates can now be derived using Google Earth. The first
image below identifies newly-derived coordinates for specific site
features.
The Chavin latitude
arcsine
equals one-sixth (asin 0.1666... = 9.5941 degrees). A right
triangle at Chavin with sides extended to the pole star and to the
geodetic center expresses the ratio 1:6; the axis is the hypotenuse
equaling six and the geodetic radius equals one. Latitude
properties expressing integral number relationships to the pole and
equator reinforce astronomical observation interpretations of major
monuments. Today, a precise asin(1/6)
geodetic triangle intersects the latitude of Building F. Secular
polar motion has shifted local latitude slightly since
construction.
In the next image, a
tessellated line extending from Newark to Pachacamac, Peru, is
visible passing 2.5 km east of Chavin de Huantar. Newark, Chavin, and
Pachacamac form a nearly straight line spanning 5,826 km. The
Archaeological Complex of Pachacamac is on the UNESCO World
Heritage Centre's Tentative List.
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South
America Sites
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code
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site
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latitude
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longitude
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source
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Chavin de Huantar Huaca A Portal |
-9.594358 |
-77.177889 |
GE 2011-01
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| pachs |
Pachacamac
Huaca Sol |
-12.262789 |
-76.901822 |
GE 2011-01
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The Newark to Pachacamac arc distance equals four times the
angular motion of the moon per rotation (r27). The mean arc
distance from Pachacamac's Huaca Sol the two great circles at Newark
(pachs-nocc-nccm) equals 4.000014 r27, an excess of only 20m (1.0 :
1.000004 accuracy). This arc distance, if interpreted as an
intentional construct, implies
accurate knowledge of lunar motion per rotation along with the
geodetic capability
to situate monuments accurately.
The three sites
together may
also express
a more complex understanding of lunar astronomy, the
fundamental astronomical constants which determine lunar
standstills. The
arc distances from Pachacamac to Newark and to Chavin
(pachs-chhap and pachs-nocp) present the ratio 1.0 :
19.59995. From Chavin (chhap) the ratio of the arcs to Pachacamac
and
Newark is 1.0 : 18.59999. The lunar
standstill constants below for 900 BCE, the approximate epoch of Chavin
construction, precisely match these proportions.
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Lunar
Standstill
Period,
900
BCE values
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code
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term
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value
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et
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eclipse nodal
intervals per
lunar orbit turn
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19.600125
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ot
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orbits per lunar orbit
turn
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18.600125
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es
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eclipse nodal
intervals per
lunar standstill period
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19.61407
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ys
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years per
lunar
standstill period
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18.61407
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os
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orbits per lunar
standstill
period
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18.61339
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x - 1 = y
x
= 19.600125 eclipse nodal
intervals per lunar orbit turn
y = 18.600125
orbits per lunar orbit turn
x
= 19.61407
eclipse nodal intervals per lunar standstill period
y = 18.61407 years per lunar standstill
period
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Another set of numbers repeats the ratio of the
arcs. The astrogeodetic module s22 represents mean angular solar
orbit
of the moon and earth per lunar
nodal period. The arc distance from
Pachacamac to Chavin equals
one-tenth of s22 (pachs-chhap = 0.100004 s22).
The arc from Chavin to Newark Octagon (chhap-nocp) equals 1.86007 s22,
that
from Pachacamac to Newark (pachs-nocp) equals 1.96007 s22, one-tenth
multiples
of the values in the table above (et and ot). The difference
between these two
arcs is precisely 0.10000 s22. The mean arc from Pachacamac to
Octagon
centerpoint and to Observatory mound is 1.960012 s22 (pachs-nocp-noom),
precisely one-tenth the "et" value (19.600125).
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