Eppure si muove        
                                         ...despite tidal braking


Léo DUBAL

dubal  @  archaeometry.org

Abstract: 

The pearled solar eclipse of 1912.04.17  

occurred 60 hours after the TITANIC disaster 
had cast its shadow upon this exciting event. 
The data collected during this most elusive eclipse,
as well as those of dozen of other solar eclipses spread over
the last 4'000 years
, are compared to those generated by Xavier JUBIER's 5MCSE,
the most up-to date ergonomical solar eclipse simulation freeware,
which allows the choice of the DeltaT parameter, as well as the exact GPS coordinates of the observation site. 
For the last 4'000 years, the Earth's spin slowdown key-parameter D T(t) will be assumed to behave as
                             D
T(t)  =  30.65 * t2  [s],
where t is expressed in centuries. 
An appropriate
ephemeris SI day, as origin of the time axis, has been chosen as Julian Day 2'398'000.5.
Excellent agreement has been found between our Geo-Chronological Model and
the records described in World Annals of all reliable candidates of ancient solar eclipses. 
One might speculate if the seconds in excess of this Model compared to actual DeltaT values
is the consequence of  recent global warming.
 

                                              Content

                                        1.  Time Scale

                                        2.  Slowdown of Earth' Spin

                                         3VLA' Canon of Solar Eclipses

                                        4.  Geo-Chronological Model vs. Solar Eclipses

                                        5.  Conclusion

                                       

1. Time Scale

 The accuracy in retrodiction of  past Solar Eclipses is bound to 
an adequate Modelling of the slowing-down of the Earth's spin.
The central parameter is the Length of the Day.
The secular length of the day λ is defined as:
  λ = (36524.24)-1 [cy]
while the circadian length of the day L(D) :
 
L(D) =  24[h] x 60[m/h] x 60[s/m] = 86'400 [s]

Since the introduction of Atomic clocks and of the SI seconds,
one has to introduce an ideal 
Do Day  which length is 
Lo( Do) = 86'400 [s SI]
In obvious divergence with commonly accepted timing for D
o 
we suggest to choose
for the ephemeris SI day
D= JD 2'398'000.5 
i.e.
1853.05.27 / 00:00 UT
JD meaning Julian Day.
In 1583, the year Galileo GALILEI
observed that a pendulum could be used for keeping time reliably,
Joseph-Juste  SCALIGER, the chronologist born in Agen, 
published in Lutecia
 
"De emendatione temporum"  [On the Correction of Chronology],
the
genial dating system he conceived after his lucky escape to Geneva
from the St Bartholomew' 
massacre.
 SCALIGER named this first linear time scale Julian Day 
 in honour to his father Julius Caesar de L'ESCALLE.
The introduction of such a Reform for Chronology
 represents a deep paradigmatic change.
Let us underline that our empirical choice for the
origin of the time-axis differs by half a century from,
 e.g.:  1800.01.01, the origin picked-up by
Kevin D. PANG, K.K. YAU & H.H. CHOU
 in Geo.Res.For. 3-4, 1998, pp. 459-488
for their analysis of Ancient Chinese Solar Eclipses


The time of occurrence of a solar eclipse will hereafter be referred as :
t  =  λ . (JD - Do[cy]

From the cumulative Geophysical difference D T
DT(t)  = UT - AT  [s] ,
between the Atomic Time defining Lo ,and
 Universal Time defining L = L(t)
follows the difference in
" LOD",  the length of the day:
D LL(t) - Lo  =  λ . dDT / dt   [s]
The rate of change of L(t) is therefore :
dL/dt =  λ d2DT/dt2  [s . cy-1]
The
average, fortnightly rate of change of secular lod  is, as expected, 
minute (ppm) compared to
 the rate of change of the fortnightly lod up and downs due to lunar tidal

2. Slow-down of Earth' Spin

The secular Earth's rotation rate
ω
= 47.34 . 109  [" / cy]
might be expressed in terms of the L(t)
ω
= 2.π  / L   [ rad . s-1]
and its time variation, as: 
dω/dt
= - . L-2 . dL/dt  [rad . s-1 .cy-1]
whence:
  = 
- L-1 . λ d2D
T/dt  [cy-1]

Our Geo-Chronological Model assumes a parabolic time dependence for DT(t):
D T(t)  =   c . t2  [s] 
whence

   =   - L-1 . λ .  2 . = - 0.63377 . 10-9 . c
  [ cy -1]  

According to  J.G. WILLIAMS
("Diurnal and semidiurnal tidal contribution to lunar secular acceleration" ,
 EOS Trans Am. Geoph.Un. 73,43,126, 1992 )

the LLR (lunar laser ranging) data indicates a secular acceleration of the Moon

= - 25.88 ± 0.5 [" / cy2]

According to K. LAMBECK
(The Earth's Variable Rotation", Oxford Univ. Press, 1980) 
the secular acceleration of the Moon induces a tidal braking of the Earth:

   =  + 1.07.10-9 .   =  - 27.7 . 10-9 [cy-1]
Over the last four
millennia, the sea-level around the Earth seems to have
not exceeded 1% in fluctuation;
ct , the tidal braking might therefore
be considered as constant, at least in 1st approximation.
   - 0.63377 . 10-9 . ct    [ cy -1]  , with
ct = - 27.7 . 10-9  /  - 0.63377 . 10-9 = 43.7 [ s . cy -2]  

Tidal Braking is NOT the only force in action. 
As established by
PANG et al. (op.cit.) for Ancient Chinese Solar Eclipses,
c
lies within two boundaries
 
27.5 <  c  < 32.5  [ s . cy -2]

As the results presented farther suggest,
for the time laps of the last 4'000 years, 
an unique c-value, well inside Pang's criterion,
suffices to retrodict satisfactorily all available data.
 This value is : 
c = 30.65 [s . cy  -2] .

The observed secular rate of change of the Earth's spin is therefore
   
=     - 19.4 . 10-9 [cy-1]
leading to an overall secular non-tidal acceleration
    =     -     =    + 8.3 . 10-9 [cy-1]
which could be accounted for 2/3 by the secular decrease
of the Earth's oblateness,
-2J2 dot  =   + 5.5 . 10-9 [cy-1]
 measured by Satellite Laser Ranging.
The combined effect
ctr of Tidal Braking and post-glacial Rebound 
(or change of oblatness) is 
ctr
= 35.0 [s . cy  -2] .
Those results are shown in the "de REYFF-Chart" for Delta T
(t = λ.[JD-Do])
for tidal braking alone, with post-glacial rebound and for Solar eclipses data 




Post-glacial Rebound is not the only Non-Tidal forces at work.
 For other smaller components, J.O. DICKEY listed, from core outwards:

 viscous torque,  topographic coupling of the mantle to the core,
electromagnetic coupling, continental drift, earth-quakes, sea level loading,
 tsunami, ocean currents, ground water, winds, and atmospheric loading.
For the last 4'000 years, one might suggest that,
  as 1st approximation, there has been, no change
 in the overall secular Non-Tidal acceleration of the Earth.
The limit of validity of this hypothesis is provided by the occurrence,
over the last decade of a decrease of the actual DeltaT, 
(possibly an effect of global warming ?).

 
The experimental values of  LOD measured since 1962 against extragalactic sources are
compared with the continuous slow-down Model.

The software used in the present analysis is 5MCSE of Xavier JUBIER.
To introduce into 5MCSE the DeltaT of our Model, one should
add into the url "&DdT=1"
e.g, for the Hipparchus eclipse
(see SAROS), of -128.11.20, the url is:

http://xjubier.free.fr/en/site_pages/solar_eclipses/xSE_GoogleMapFull.php?Ecl=-01281120&Acc=2&Umb=1&Lmt=1&Mag=0&DdT=1

back to content

3.  VLA Canon of Observed Solar Eclipses

Our Geo-Chronological Model has been applied to both,
more recent and older solar eclipses, resulting in a new
Canon of Solar Eclipses.

On click, on Table SAROS will be downloaded
(PDF 63 ko)
 the output data generated by 5MCSE
for dozen of  relevant solar eclipses:
 timed according to the Geo-Chronological Model and
precisely located thanks to GoogleEarth.

"Relevant" means here for which Annals Records are not
- at least too obviously - apocryphal, and provide
sufficient information to make a qualified guess :
i)
a fair estimate of the location of the observation site,
ii)  a convincing date for the eclipse,
iii) a plausible order of magnitude of the eclipse at the observation site.
Such criteria have not been used in the other CANONS available on the web,
such as the monumental
 
Ancient & Medieval Eclipses in European Sources.
of F.K.GINZEL, originally published in Berlin, in 1899.

With the solar eclipse SAROS 26/40 (-1301.06.05) which, we

supposed
somewhere else to be described on a SHANG turtle bone oracle,
 excavated in Xiaotun near Anyang (Henan),
one has an interesting example how, a Geo-Chronological Model,
could comfort a linguistic interpretation or another.
Instead of adjusting Delta T in order to produce a 6
[m] long totality
over Xiaotun, the Magnitude retrodicted is a mere Magnitude of 0.83...
i.e.:  does not qualify to be listed in Table SAROS.

SAROS 118/43 (1560.08.21), discussed in the next Chapter, is another example
 not qualifying for the Table, due to the partial unreliability of the Annals.

One should notice that,  prior to year 840 Common Era,
solar eclipses have been used to date Annals,
with the uncertainty associated to such a guess-work.
Those proto-historical eclipses are marked in the
Table SAROS with grey background.
A graphical presentation of those results is given in the
de Reyff' - Chart.
 

back to content

4Geo-Chronological Model vs. Solar Eclipses

Table SAROS
presents a formatted, compact version of the data studied so far.
One will note the surprisingly high degree of coherence
 between the available records of all those solar eclipses and their retrodicted values.
So far the classical empirical approach has been to attempt best-fitting of the solar eclipses records, 
at the cost of assuming reliability of the available, often dubious, information.
With our Model, one has a tool to
pin-point deviant behaviour of the Earth, if any...
For completeness, about the wide range of interpretation of  solar eclipses,
let us remember that, in 1929, N.A.MOROZOV suggested that the
 "THUCYDIDES Triad" was the "contribution" of  J. KEPLER,
to proof scientifically the date of the Peloponnesus war...
a topic to be discussed somewhere else.
 

To demonstrate the interest of this Geo-Chronological Model,
let us cross-examine
both retrodictions, and Annals reports for
a few dozen
of solar eclipses,
 

1)    SAROS 134/43 on 2005.10.03

According to Bulletin de l'IERS, Delta T-value for this day was  65 seconds.
 The Geo-Chronological Model generates though a higher value, i.e. D T= 71 [s].
 If this rebound trend (induced by global warming ?) 
 would continue in the future, this might signal the end of the past "quiet" 4000 years long period.
 
 
 With the value given by the Model
D T= 71 [s],
 
5MCSE predicts @ E1.41887 / N38.7347 (Pitiüses Islands
.)
 
C2 at 09:02:08 UT 
Max at        09:03:47 UT         
C3 at   09:05:25 UT  
 with a magnitude of 0.960, a height of 34° and a duration 3m 17s.
In comparison, with the measured value (intergalactic Quasars),  D T= 65 [s], one predicts
C2 at   09:02:18
Max at 09:03:55
C3 at    09:05:31 
 with a magnitude of 0.960, a height of 34° and a duration 3m 14s.

 Those last results agree with VLA's photographical records (with filter 10-5)
The indicated UT-time is the one of the GPS-calibrated clock of the camera

09:02:27 photo VLAphoto VLA 09:03:43photo VLA 09:04:13

         09:02:27 UT          09:03:43 UT                09:04:13 UT         09:05:23
UT
        

As documented by VLA at 09:04:07 UT,
one can observe the maximum of an annular eclipse,
 
using, here, one Ø1mm & one Ø2 mm holes in a foil,

with a resulting four-fold intensity difference in the images projected onto a wall.

O
n 2005.10.03 @ E1.4 / N38.7 at 08:50 UT, we took another picture of this eclipse
 without any artificial filter in front of the camera,
the light of the solar crescent being 
naturally filtered by the clouds.



Those most exciting conditions of observation lasted for about 3 minutes.
Before the invention of protective glasses, the occurrence of such conditions have
 allowed quite optimal
naked eye observation of partial solar eclipses ...
 


2)    SAROS 137/30
on 1912.04.17

In the Annals 1912 of the Société Astronomique Française, published by
Camille FLAMMARION, one finds precious data.on this  eclipse

i)   The Chronometer of the balloon "Globule"  has been tuned on
 Paris' Observatory by Paul TISSANDIER. It  indicated exactly
 12:11:51,
when Auguste NICOLLEAU took the following the picture:


 which suggests that the position of the balloon was very closed to the center line.
Its altitude was estimated to be 900 meters
over the Bridge of Rethondes,
 on the North bank of River Aisne, 100 meters West from the bridge.
With Google Earth one can estimate this location as: E2.937 / N49.414
,
 With a Delta T = 11 [s] given by our Geo-Chronoligical Model,
5MCSE retrodicts the occurrence of the maximum at 12:11:54,
a duration of 2.3 [s], and 51° for the height of the Sun

ii
)   At the FLAMMARION Observatory at Juvisy s/Orge @ E2.37° / N 48.69°
the maximum given by
5MCSE is at 12: 10: 19.with a magnitude of  0.992
C. FLAMMARION reported 12:10:20
, as the time of the picture taken by F. QUENISSET

It is of great interest: though slightly OFF centrality; protuberances were visible:.
we will refer to this effect as FLAMMARION's partial corona.
Concerning the timing of the maximum other pictures of QUENISSET indicate 
the occurrence of the maximum at about 12:10:15


 

iii)   The totality of the pearled eclipse on 1912.04.17 has been photographed 
at Saint-Nom-la-Bretêche, GPS E2.016° /N48.857°, by
 A. DANJON, at supposedly 12:09:53 

5MCSE retro-predicts for this site the maximum at 12:10:01 and a duration of 1.9 s.

iv)   Another interesting picture of this pearled eclipse is:

v)    From a captive balloon, the size of the Lunar shadow on the Earth
has been estimated to be 3.5 km wide.

vi)   On 12 km of the road between Neauphle et Trappes, 380 school children
 have been spaced by 100 m to monitor the width of the totality path
The central zone has been 4 km wide.
The minimum diameter of the Moon (bottom of the valleys) lasted 3 [s]
less than the one of the Sun, while the maximum diameter (mountain peaks)
was surpassing  by 2 [s] the diameter of the Sun.

vii)    At the crossing of la Grand'Croix,
Léon GAUMONT (1864-1946)
obtained a cinematographic record of the event.

viii)     In Ovar, observatory stations were spread along the road between Carregal to Cadaval
While 5MCSE retrodicts only 1.4 km of the road to have been in the totality zone,
 all the observers who were spread over 5 km to the West of station #10 
have believed to be in the central line !!! 

At station  #10, GPS W8.59757 / N40.85432

COSTA LOBO obtained 158 images in 14 [s]
showing Baily grains,
whose 40 with the grains only in the areas opposed to the Sun.
 The eclipse was therefore total
for a time laps of 4.4 [s],
only along the direction of the Moon,
what confirms the film of  Léon GAUMONT.
It has been interpreted, as the relative speed of the Moon
to the Earth is about 0.38 ["/s], i.e. 693 [m/s], as due to the shape of the Moon:
   a slight flattening along the axis of rotation,
The irregular profile of the Moon shows indeed,
 between valleys and peaks typically a 1["] difference..



Let us note though that Serge KOUTCHMY has shown evidence for an "ovalisation"
 (or polar lengthening) of the Solar Chromosphere, which,
in our opinion,
might well have also contributed to the direction dependant totality effect
recorded in 1912
The timing of the contacts recorded in observatory #10 
are compared to the retrodicted values with  5MCSE : 

  time measured time retropredicted
C1 10:21:12 10:20:50
C2 11:42:50 11:42:44
C3 11:43:04 11:42:45
C4 13:08:41 13:08:47

Those discrepancies demonstrate the major role of the profile of the Moon
on determining the timing of an eclipse.
Let us note here that the BIH
(Bureau international de l'heure) has been created in 1913.

ix)  
  At station #2  @ W8.6426 / N 40.8654,

  time measured time retropredicted
C2 11:42:52 11:42:41
C3 11:43:02 11:42:42
C4 13:08:37 13:08:44

x)    In observatory #3  @ W8.6376 /N 40.86317,
5MCSE retrodicts 1.6 s of totality, 10 times shorter than observed 

  time measured time retropredicted
C1 10:21:08 10:20:49
C2 11:42:47 11:42:42
C3 11:43:04 11:42:44
C4 13:08:38 13:08:44

xi)    In observatory #4  @ W8.6318 /N 40.8622,

  time measured time retropredicted
C2 11:42:50 11:42:56
C3 11:43:02
C4 13:08:37

Two interesting pictures of before and after totality have been taken.



xii)      In observatory #8 @ W8.6100 / N40.85677 the time of contacts were 

  time measured time retropredicted
C1 10:21:09 10:20:50
C2 11:42:55 11:42:43
C4 13:08:38 13:08:46


xiv) 
  To the East now... in Geneva @ E6.1526 / N46.200,  DUFOUR took this nice record:



5MCSE retrodicts the maximum at 12:12:59 (i.e. 1H13 Central Hour)

   of magnitude 0.889.
 

3)    SAROS 126/41 on 1900.05.28

 The drawing of the corona due to Fr. MOREUX  at site @ W 0.72 / N 38.27
is particularly interesting : "..couronne tissées de fils...presque irréels"

1900.05.28  Drawing Moreux

it is corroborated  @ E3.1 / N 36.7
by the drawing of A.C. CROMMELIN

Algiers 1900.05.28 / Drawing Crommelin


and the one of  E.W. MAUNDER

Algiers 1900.05.28 / Drawing Maunder ?

4)    SAROS 133/29 on 1724.05.22

@ E2.107 / N48.81, in the Trianon from Versailles, Jacques CASSINI & LOUIS XV
proceeded to a first chronometric observation of a solar eclipse, comforted by the
measurements of DESLILE at the Observatory of Paris.
DE REYFF discussed the consequences of this important scientific event
(though optimistic concerning CASSINI's skill to accurately set the time of  his clock).  

5)    SAROS 133/25 on 1652
.04.08

@ W5.806 / N54.713, the duration of totality was 21 seconds. 
The observation of Dr WYBERG on the Northern border of the Belfast Lough
 are most precious, because Carrickfergus was also just at the Northern border of the totality path.
". . . [ the Sun was reduced to] a very slender crescent of light, 
the Moon all at once threw herself within the margin of the solar disc with such agility that she seemed to revolve
 like an upper millstone, affording a pleasant spectacle of rotatory motion."
This eclipse represents therefore a most important test of our Model.  

6)    SAROS 137/13 on 1605.10.12

The so-called "Noirceur" @ E5.37 / N43.29, over Marseille leads one to presume
 that, on an October afternoon, a magnitude of 0.985 looks particularly dark.
 For comparison, let us note that the pictures taken in Geneva on 1912.04.17 with a magnitude of 0.889
look  already pretty grim. 

7)    SAROS 112/58 on 1567.04.09

For this pearled eclipse @ E12.457 / N41.902,
5MCSE retrodicts a magnitude of 0.997.
The Vatican was slightly North of the narrow totality path.

CLAVIUS (1537-1612) claims to have witnessed two Eclipses of the Sun in the space of 7 years.
 CLAVIUS report
, dated 1593, a quarter of century after SAROS 112/58, in
Sphaeram Ioannis de Sacrobosco, Commentarius
, p 508, reads:

The other I saw at Rome in the year 1567 also about midday in which although the Moon was placed
 between my sight and the Sun it did not obscure the whole Sun as previously
(i.e. in Lusitania)
 but a narrow circle was left on the Sun, surrounding the whole Moon on all sides.

One might guess, that, he saw the FLAMMARION partial corona.

8)    SAROS 118/43 on 1560.08.21:

This eclipse was total over Granada and OPorto.
while in Coimbra, @ W8.412/N40.221, the retrodicted Magnitude was 0.996,
In the report previously quoted, CLAVIUS said:

  "One of these I observed about midday at Coimbra in Lusitania  in the year 1559,
 in which the Moon was placed between my sight and the Sun with the result that it covered
the whole Sun for a considerable length of time." 
Obviously, after such a long time he could not remember well the year,
 because in Portugal, around 1559, the only solar eclipse occurred a year later.
If he saw himself the eclipse
at all, did he remember his site of observation correctly ?

9)    SAROS 121/28 on 1431.02.12

This eclipse was total over Perugia @ E12.39/N43.11 at 14:38UT
Antonio dei Veghi, in Diario dall'anno 1423 al 1491. wrote:
"On February 12 at about the 21st or 22nd hour, the Sun was completely obscured
 and in front of the Sun was placed a black circle like a little wheel. 
It became
as dark as night and the sky revealed the stars.
 The birds went to roost as they usually do at night. 
Everyone was feeling ill at ease as a result of this event. 
It began half an hour before the Sun was covered over. 
It gradually lost its light even to the hour stated above. . ." 
Time here was obviously counted since sunset the day before.


10)    SAROS 115/33 on 1239.06.03:
In Arrezzo 250 paces long
In Mende, totality with  98%....

At least nine different Annals, relate the event, i.e: 
Coimbra (Chronicon Conimbricensis) 
 Toledo (Anales Toledanos)
Mende (Arch. Gévaudaises, 1913)
 Montpellier (Zurita, Anales de la Corona de Aragon)
Firenze (Storie Fiorentina)
 Siena (Archivo de Duomo di Siena)
 Arezzo (R
ISTORO d'Arezzo: Della composizione del mondo )
Cesena (Annales Caesenates)
Split  (Thomae Historia Pontificum Salonitanorum et Spalatinorum)
RISTORO d'Arezzo wrote the most interesting report , the totality there was the longest, i.e. 350 seconds:
“while I was in the city of Arezzo, where I was born, and in which I am writing this book,
in our monastery, a building which is situated towards the
 end of the fifth latitude zone, whose latitude from the equator is 42 and a quarter degrees
(vs GPS N43.46), 
and whose westerly longitude is 32 and a third
(vs GPS E11.87),

 one Friday, at the 6 th hour of the day (vs 12:15UT), when the Sun was 20 deg in Gemini
 and the weather was calm and clear, the sky began to turn yellow and 
I saw the whole body of the Sun covered step by step and it became night.
  I saw Mercury close to the Sun, and all the animals and birds were terrified; 
and the wild beasts could easily by caught.
  There were some people who caught birds and animals, because they were bewildered.

    The air and the ground began to become cold; and it  began to be covered and uncovered from the west.”
  
I saw the Sun entirely covered for the space of time in which a man could walk fully 250 paces.
This early chronometry exercise reveals that the paces in a  monastery are twice slower than mine... 

This first multi-site solar eclipse observation represents
 a unique opportunity to represents a unique opportunity to
audit medieval Annals: 

Translating Arch. Gévaudaises, 1913 gives:
"A.D. 1239,...the 3rd of nones of June,...between nones (i.e.:3 p.m.)
and noon,...there was a total solar eclipse"
.
 While at the 8 other observation sites, totality lasted between 3 to 6 minutes,
in Mende, the magnitude did not reached 98%.

11)    SAROS 121/14 on
1178.09.13

The information given in Arch. Gévaudaises, 1913,  is minimal. It is based on
 "Chronicle and custom of Bishop GUILLAUME IV de Peyre" (1194), 
quoting ADELBERT III, his predecessor in Mende, 
The site is therefore supposed to be @ E 3.50 / N44.52  
The report reads:
"Eleven hundred after seventy eight, the Moon hid the Sun in its 21st day". 
Only the year is mentioned, what is already most precious,
but "its 21st day"  is a weird way of describing the new Moon.

12)   SAROS 102/43 on 1133.08.02 : 

Honorii Augustodunensis: Summa Totius et Imagine Mundi. 
"Duke Frederick . . . set fire to the town of Augsburg and killed many of its citizens . . . 
An eclipse of the Sun occurred on the 4th day before the Nones of August at midday for about an hour,
such as is not seen in a thousand years. Eventually the whole sky was dark like night,
 and stars were seen over almost the whole sky. 
At length the Sun, emerging from the darkness, appeared like a star, 
afterwards in the form of a new Moon; finally it assumed its original form
."  
Distinguished
researchers have confused Honoré d'Autun, with the city of Augsburg !
Our Model restores the truth...
The totality over Regensburg, @E12.0886/ N49.0188 , 
the residence of the
famous author of Imagine Mundi,  lasted 2m 45s

13)    SAROS 111/29 on 1033.06.29

For the eclipse  @ E 4.659 / N 46.434:
with a retrodicted magnitude 0.985 over Cluny,
the Annals mention the appreciation:... "truly frightening".
La même année, la millième après la Passion du Seigneur,
le troisième jour des calendes de juillet, un vendredi vingt-huitième jour de la lune,
 se produisit une éclipse ou obscurcissement du soleil, qui dura
depuis la sixième heure de ce jour jusqu'à la huitième et fut vraiment terrible.
Le soleil prit la couleur du saphir, et il portait à sa partie supérieure l'image de la lune à son premier quartier.
Les hommes, en se regardant entre eux, se voyaient pâles comme des morts...»
.

The time mentioned between the 6 and 8th hours after dawn is consistent
with the retrodicted time of the first & last penumbra contacts, i.e.09:42 & 12:45 UT
The date, mentioned as the 3rd day before the July Calendars,
according to
http://www.louisg.net/C_julien.htm is indeed June 29th. The depiction of
 the maximum: i.e. the Sun was carrying on his upper part the image of the Moon
 at its 1st quarter, is also consistent with
 
5MCSE retrodiction at 11:13 UT 

14)    SAROS 115/18 on 968.12.22

The solar corona @ E29. / N41. is described in  Leo DEACONIS Historiae as:
 a narrow headband, shining around the edge of the disk
.

15 )    SAROS 90/55 on 840.05.05

With the description of this eclipse @ E9.37 /N47.42, in the
 Annales Sangallenses, one has the very first Chronicle description of an eclipse.
Previous annals’ reports were themselves dated on the basis of eclipses!
Year 840  is, in this sense, the beginning of modern History of solar eclipses.




The year, here, is explicitly given: ω.xl.  with the abbreviation ω standing for 800
This Chronicle is most important because it is corroborated by  the "Chronicon" of ANDREAS Bergomatis  
Indictione tertia sic fuit sol obscuratus in hoc mundo, et stellas in celo apparebant,
3.Nonas Magias, ora nona, in laetanias Domini,
quasi media ora. Facta est tribulatio magna. Cumque hoc populus intenderent,
multi extimabant, quod iam amplius hoc seculum non staret
sed dum haec angustia contemplarent, refulsit sol et
quasi tremidus in antea umbraculam fugire cepit.
Ipsa vero nocte sequenti prope matutino facta est lux quasi in die.
Haec signa in celo conperta, doctores in suorum monitiones dixerunt
Estote, fratres, parati; quia adimpletum est quod in evangelio Dominus dixit:
cum haec signa videritis, scitote, quia prope est die Domini magnus et manifestus?
Sequenti autem mense Iunio Hludowicus imperator defunctus est, suosque dies finivit in pace. 

The death of LOUIS I, just mentioned in CSG, is usually assumed to occur on 840.06.20.
It is described in ANDREAS B. Chronicon in relation to
this long eclipse over Bergamo, and the 3rd year of indiction:
May 840 matches the 3rd year of the 35th indiction,
 the 15 years long ecclesiastical fiscal period  introduced by CONSTANTIN on 312.09.01. 
For the precise day in May, both Chronicles indicate 3 days before the None's of May,
which, according to http://www.louisg.net/C_julien.htm is indeed May 5th, and for the hour, 
St-Gallen mentions between the 8th and 9th hour (of the day).
  For St-Gallen, GPS gives 03:17 UT for sunrise, 8h30 added to it gives 12:47 UT
 while 5MCSE retrodicts 12:38 UT....
click for a more in-depth discussion (in French)
 
16)    SAROS 79/29 on 71.03.20

This eclipse was total for half a minute over the city of Athens,
while it is believed that
 the poet PLUTARCH spent most of his life in his city of Chaeronea.
In De facie in orbe lunae, PLUTARCH  lets an Athenian
 (friend of his ?) called Lucius, describe a solar eclipse:
...beginning  just after noonday 
 Later, Lucius described  
"...a kind of light visible about the rim,
 keeping the shadow from being profound.."
what corresponds well to
the partial corona, as coined by FLAMMARION

17)    SAROS 62/54 on 65.12.16
For the eclipse over the Kingdom of CHU,  
with magnitude of 0.997 over the capital Xuzhou
@ E117.15/ N34.25
one might ask if it has not been instrumental in enforcing Buddhism.

18)    SAROS 79/18 on -128.11.29

The totality path crossed over the Hellespont,  e.g. 17 s duration @ E26.398/N40.146 
while 1/5 of the sun disk was still visible in Alexandria @E29.9 /N31.2: 
this matches exactly with the description
 given by PAPPUS and CLEOMEDRE of the characteristics
 of the eclipse used by the Greek astronomer HIPPARCHUS in his
  evaluation of D
E-M, the Distance Earth-Moon, in terms of RE, the Earth Radius. 
We do not know how HIPPARCHUS actually proceeded.  
A qualified guess has been  90 Earth Radii. Another approach is:
as the height of the sun was only 12° over the horizon,
 it must have been easy to remember its
 position over the landscape and then to estimate the azimuths of the 
two observation sites, i.e. 233° and 239° as retrodicted by 5MCSE.
The ratio R
E / DE-M equals the ratio of a 1/5 of the sun apparent angle 0.5°/5 
and of the 6° difference in azimuth, i.e. 0.1° / 6° = 1/60, 
The distance from Alexandria to the Moon is then 60 Earth Radii.
As expected, there exist other opinions on HIPPARCHUS...
 e.g.: On the web-site of the School of Mathematics, Uni. St Andrews,
 forwarding the claims of G J TOOMER, HIPPARCHUS on the distances
of the Sun and Moon, Arch. History Exact Sci. 14 (1974), 126-142
it is boldly stated that HIPPARCHUS used the eclipse on -189.03.14,
on his birthday so to speak...  

19)    SAROS 69/24 on -309.08.15

 The totality zone with its southern border at the bay of Syracusa @  E15.29 / N37.07,
makes the story of the escape of AGATHOCLES  to sounds plausible.

20)    SAROS 50/42 on -462.04.30

Out of the eclipse  @ E10.32 /N36.83 emerged, in 1995,
the hypothesis that this event might have been instrumental in the institution of the cult of the 
Goddess TANIT  in Carthage. 5MCSE retrodicts  M=0.985 at 12:39 UT

21)    SAROS 42/62 on -477.02.17

For this annular eclipse @ E23.38 / N38.36
the Theban poet PINDAR, while 40 years, old, wrote an Ode (Paens, IX)
 to the citizens of his city, evoking the long annular eclipse:
.
...star supreme, reft from us in the daytime !
and the threats of the Theban winter:
...an unspeakably violent snow-storm

2
2)    SAROS 44/42 on -708.07.17

This eclipse  @ E116.576 /N35.401 is the first eclipse reported in Chinese Annals.
This stele, photographied by Liu Ciyuan, is now at Xian.
It is a later copy of earlier Annals from Jining @E116.576/ N35.401,
what became 150 years later the native place of Confucius 
 
Renchen, the 29th day of the Jiazi, the"60 days Chinese week", 
associated with the name of LU HUANGgong, the chief of the kingdom of Lu 
provides unmistakably the date of this nearly 2 minutes long solar eclipse,

i.e., a very strong argument for the Geo-Chronological Model.

23)    SAROS 26/38 on -1337.05.14

During the eclipse  @ E30.90 /N27.67 the totality over the site,
where two years later AKHENATEN will inaugurate his capital  Akhet-Aten,

24)    SAROS 23/14 on -1911.09.24  

For the annular eclipse @E111.7° / N27.67, 
one deals with the oldest solar eclipse ever mentioned.
This "Double Sunset" which took place at sun dawn over Chande, in western part of the San Miao Kingdom, 
has first been described by PANG et al in GeoRes Forum pp 479-481.

back to content

6.  Conclusion

The solar eclipse of  +840.05.05 described in the
 Codices Electronici Sangallenses 915 confirms
 the validity of both Common Chronology and the Geo-Chronological Model.
The excellent agreement between our solar eclipses retrodictions with Xavier JUBIER's 5MCSE 
& World Annals strongly advocates for the use of
  DT given by the Geo-Chronological Model as input data to 5MCSE.
 Keeping in mind that, at the decade level, deviations from a strict parabolic decrease
 might reach up to 30 sec, those small oscillations, mainly harmonic O1,

invalidate wild oscillating behaviour used previously as default values.

The solar eclipse of  -1301.06.05, previously boldly assumed to have been
described on an oracle bone of the Shang Dynasty,
 as well as 
the solar eclipse of +1133.08.02,
reported in Regensburg by Honorii  Augustodunensis
the famous author of Imagine Mundi, 
misleadingly assumed by previous researchers to have been in Augsburg, 
or
the solar eclipse of  +1239.06.03 misleadingly
described as "total" in Mende Archbishopric Annals
cast more than a doubt
upon the classical approach of "Best-fitting Delta T".

The retrodicted parameters of solar eclipses are consistent
 with a mean non-tidal acceleration of the Earth
   =   + 8.3 .10-9 [cy-1],
constant over the last 4'000 years.




Acknowledgment:  Our thanks to Serge KOUTCHMY, Xavier JUBIER and Christophe de REYFF
   for their stimulating discussions and continuous support..

Back

© Virtual Laboratory for Archaeometry latest revision:    2008.06.12 21:01