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.
1. Time Scale
2. Slowdown of Earth' Spin
3. VLA' 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


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)
According to Bulletin de l'IERS, Delta T-value for this day was 65 seconds.




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:

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 vi) On 12 km of
the road between Neauphle et Trappes, 380 school children
has been estimated to be 3.5 km wide.
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,

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
| 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.
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"


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
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 (RISTORO
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
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 solar corona
@ E29. / N41. is described
in Leo DEACONIS Historiae as:
a narrow headband, shining around the edge of the disk.
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,
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 DE-M, the Distance Earth-Moon, in terms of RE,
the Earth Radius.
Out of the eclipse @
E10.32 /N36.83 emerged,
in 1995, For this annular eclipse @ E23.38 / N38.36
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
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
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
23) SAROS 26/38
on -1337.05.14
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.
© Virtual Laboratory for Archaeometry / latest revision: 2008.06.12 21:01