NOUVEAU
PHENOMENE RARE ET SINGULIER, D'une Lumière Celeste, qui a paru
au commencement du Printemps de cette année 1683 - par M. Cassini
.
Spring that year (1683)
started showing off a most unusual sight in the sky. Cassini described
it as follows:
a light, similar to that which whitens the
Milky Way, but brighter and more brilliant
at its centre and fainter at its ending tips, spread through the signs
the Sun crosses during this part of the season.
I started seeing it from the Royal Observatory
on the evening of 18 March, two
days before the equinox. Shortly, after
observing the changes that arose on the planet
Saturn, I recognized the
first star of the Ram. With the help of
lenses it can be seen as a twin star: each star is distant from the other
the length of both their diameters put together.
I saw this constellation and that of Taurus
much more luminous than ordinary around seven and three quarters, half
an hour after dusk ended.
On the Western side, only the rays at the horizon
retained such a luminescence up to a height of two, three degrees and the
brighter part extended for about eight, nine degrees.
It extended, along the Zodiac, almost obliquely,
reaching the Northern edge of the two most luminous stars of the Ram’s
head. It crossed the whole body of the
Ram, extended
towards Pleiades and vanished quietly and gently in Taurus’s
head.
Resemblance with the tail of a comet ...
This part of the sky was extremely clear; by
naked eye it was possible to see the stars with magnitude six and seven.
This luminescence, though similar to a mist floodlit by the Sun
rays, did not prevent the vision
of these small stars, even in its middle, which was thicker, in a similar
way as they could be seen through the tails of the comets. Its width, however,
was too extended to mistake it for a comet’s tail, as it was 3 or 4 times
the width of the biggest (tails) I ever saw up to now.
Except for its width, all other particulars were
very much similar to a tail, not only for its transparency, but also for
its colour and its position with respect to the Sun,
towards which it, more or less, pointed lengthways.
It was soon understood it followed the motion
of the sky towards West. Following this motion, it
always stationed within the same constellations
and, together with them, plunged into the fog at the horizon. I
doubted whether it slightly moved towards North,
as the two most brilliant stars of the Ram became a part of this
luminescence, which, at first, just touched the Northern side of this constellation.
This event was also confirmed by the observations carried out during the
following days.
There and then I was not completely sure, nor
was I days later. Everywhere the extreme
end of this luminescence was uncertain. It became more and more feeble.
It was extremely difficult to exactly determine its border lines through
the different shades of brightness the air showed at different distances.
At twilight, during the following days, it appeared more or less diffused.
Therefore, when the evening just started, an hour after sunset, that part
of luminescence, that was mostly visible, extended in breadth up to the
most brilliant stars of the Ram
and lengthways up to Pleiades.
Shortly after it modelled both. Its central part, however, as could be
ascertained by naked eye, seemed always motionless in the same point and
pointed towards the centre of the Ram.
Once this constellation and that of Taurus
waned, I tried to see if some trace of
this luminescence was still present where it had showed at first, at a
certain height and position, but nothing extraordinary could be seen there
anymore. This made me understand it followed the daily revolution of these
two constellations around the Earth:
it waned with them during the following days and appeared together with
them in the very same points where it had been seen during the previous
days. For the Copernicans this is alike being motionless in the sky, always
in the same point, during the daily revolution of the elementary sphere
about the Earth’s axis from West to East.
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Observation peculiarities ...
Samely, I observed it from 18
to 26 March,
whenever, in the evening, the sky was clear at West, without noticing
any further evident changes, except for those noticed during my last observation,
which I carried out on 26 March: this light did not seem to extend towards
the horns of Taurus, but more towards North, while the most brilliant star
of the Ram, that in the beginning just passed closed to its side plunged
more than one degree into this light.
During this last observation I could not discover
the first star of this constellation, because it was quite low and deep
amidst fogs, that at West diminished the extension of the light much more
than in previous observations.
Most probably without this obstacle and without
the twilight, it could have been seen more extended towards West and quite
near to the Sun that, in the beginning, was in the penultimate of Pisces.
It wandered away 30 degrees from the first of Ram and during the last observation,
carried out on 26 March, it moved away just slightly more than 22 degrees.
If this luminescence could have been seen conjoined with the Sun,
it would have shown up as a coma.
After this period, as the sky appeared cloudy
at West in the evening, I was not able to verify if such luminescence had
dissolved, except on 14, 22, 24 and 28 April. During these days, even if
after dawn, the constellation of the Ram
was hidden, the same luminescence could still be seen in Taurus,
extended up to its Northern horn. Northerly, it neared the head of Medusa
and the Southern knee of Perseus,
while its Southern foot was immersed into this light.
Therefore, during these last observations I
was able to see this luminescence advancing slightly towards North, in
a better way than before. This, while
the Sun neared Taurus, prevented it to show so brilliant, due to the evening
twilight.
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Comparison between this
aspect and other similar ones,
together with something
very strange on this argument
In past Memories it was very difficult to find
something similar to this new light that,
for many days, was stationary in the same celestial signs (zodiac signs)
without showing any evident particular motion. Its extension, mainly in
width, was great and no comet that could have been the cause of its origin
was to be seen.
What may be considered nearer to this circumstance,
to its duration, consistency and direction towards the meeting with the
Sun, was an event I saw in Bologna during year 1668,
when I was invited over to France and where His Majesty, the King of France,
requested me to join the Academie Royale des Sciences (Royal Academy
of Sciences). It was a path of light similar to the tail of a comet: it
took up a space 30 degrees in length and a little more than 1 degree in
width.
On 10 March, I observed it at the horizon,
peeping out from the clouds that hid the constellation of Cetus
or Whale,
while on the Eastern side it pointed towards the foot of Orion and on the
Western side towards the Sun. Its longitude was in relation with the signs
of the Ram and of Taurus, but its latitude was manly Southerly. It changed
position among the fixed stars, following a particular motion towards East
and towards North, nearing Orion day after day. It remained visible up
to 19 March and, during these nine days, it passed opposite different stars
of Eridanus, never hiding any of them.
Others saw the same event
elsewhere ...
Chardin, while describing the coronation of
Suleiman, King of Persia, refers that in 1668 a similar event was observed
in the capital of one of the Persian
Provinces on 7 March,
the second day after its first apparition. Later on it showed up on 10
March, at 7 in the evening, at Ispahal, capital of the Kingdom.
It showed up in the Southern side, following
the celestial vault. It was 30 degrees and
32 minutes long.
Data meets with our observations. It was 6 degrees large almost everywhere,
4 times more than the one I observed in Bologna. Yet, some people saw it
larger. Its width, however, was difficult to estimate, as at its extreme
end it was feeble, dissolving little by little. Chardin added its upper
part pointed towards the Orion’s Belt and the river Eridanus.
From my point of view, longitude 72 degrees and
latitude of the ecliptic 3 degrees do not comply with this position, as
Eridanus and the Orion’s Belt are much more Northerly and Westerly.
He also added its lower end was Cetus
or the bend of Eridanus,
which exactly coincides with my observation that focuses it where the hollow
of Cetus touches the bend of Eridanus, without respect to the longitude
and the latitude he gives to this ending part, where numbers seem to be
incorrect. He says Persians called it Niazach, which means small spear
because of its appearance. He also reported they had never seen or heard
of a similar event. He said they thought it was a comet, its head hidden
in the West, so that it could not be seen at the horizon.
Cassini’s hypothesis ...
In that occasion, I was able to prove that
this event was quite similar to something else that had appeared two thousand
years before. An event Carimandrus
, as referred by Seneca in his work "Discussions
on Nature (Naturales
Quaestiones)" in
7 books, says had been observed by Anaxagoras:
it was a great unusual light visible for
many days and it had the size of a big log . The same author states
also Callisthenes
observed this light before the two great towns of Achaea,
Helix and Bure, disappeared into the sea
due to an earth-quake. It had the shape of a fire, quite extended in length.
According to Aristotle it was a comet that did not seem so at the beginning,
because of its great blaze. When time passed by, it showed its true nature
as soon as the Sun
started to set.
Seneca, in chapter 6th of book 1st
"on Meteors", writing about this event
that was observed in the sky during the time of the earth-quake and of
the floods that destroyed Achaea, called
it Great Comet, or Great Star. He said
it became visible at the Western equinoctial point, in the same way as
seen by Us. After many stories and notes on similar events, he added that
the Great Star, of which before, became manifest when the weather was frosty
and the evenings were very clear, in the year during which Aristaeus was
Archon of Athens. The first day it did not show up at all, as the Sun
set early. The next day it showed a little
more, as the Sun delayed a little, and set after this light had extended
up to the third part of the sky, taking the shape of a line. For this reason
it was called "Pathway": it extended upward to the Orion’s Belt and there
dissolved. Something very similar happened to the "Pathway" of light of
1668.
Seneca, misunderstanding
this event and considering it as a comet, treated Ephorus
as a liar and a swindler. Ephorus
stated this great light had divided into two stars. Nobody else made such
assertion, even if everybody witnessed it everywhere on earth and considered
it as an omen of the submersion of the two towns. Although
the apparition of this great light was certain and witnessed by all the
people that observed it, it was not possible to agree on its nature, similarly
as it was not possible for the present event of our days.
There are some further Memories of ambiguous comets,
which only showed a great light, same as that observed after 10 till 29
November 1618, in the Southern side of the sky, towards Hydra, before the
apparition of the great comet that showed up in the Northern side towards
the end of that same month and that lasted till the end of January 1619. |
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About the nature of this light
This extraordinary light able to shed rays
upon the Earth seemed to possess some particular material:
luminous itself or able to reflect or decompose the rays of the Sun or
the rays of some other luminous body, directly or with the help of a foreign
body. However the direction of its length from the Sun allowed to presume
it originated from the Sun itself.
In my Compendium of Observations no. 12 carried
out on the comet of year 1681, I said: in
the Upper Sky there may be a diffused substance able to reflect the light,
similar to what can be found in the air (atmosphere?) that surrounds the
Earth. This substance meeting the comets, where the Sky is more or less
clear, may favour the apparition of their tails and become the cause of
the changes that arise from them.
As this light is similar to that of the comets,
both in colour and brightness, in faintness and in the relation it has
with the rays of the Sun, it is possible to believe that the substance
that reflects this light has a similar nature,
whether it originates from a comet hidden among the rays of the Sun (an
argument I should not wish to foster, since its width is so dissimilar
from that of all the other comet tails observed up to now) or whether it
directly receives the rays of the Sun itself, in the same way as
we can see in the air (atmosphere?) events caused by refractions and by
the direct reflexes of the Sun or by similar reflexes due to the intrusion
of the Moon, such as the Iris and the Haloes of this or that Star.
No other inconvenience is there except for the
appearance that, in this substance spread out in the Upper Sky, is similar
whether originating from the Sun or self originating or originating from
the tail end of some comet. It could even
reflect the light of some Star. This happens
when certain fixed Stars show a coma, as
referred by Aristotle, in accordance with
the observations of the Egyptians and with what he emphasized, himself
having seen a coma around one of the Stars
in the Leg of the great Dog,
initially not brilliant, but still evident to those who carefully observed
it.
It must be remarked that our light seemed to originate
from the same place where many comets
passed by during this century, in years
1652, 1665, 1672, 1680
and where numerous other passed by in previous centuries and that, due
to their frequency, could be seen in that belt, I called "Comet’s
Zodiac" in my Treatise.
Hypothesis on the distance
of this luminous substance.
Regarding the distance
of such substance that originates this light or that is a medium through
which this light is reflected or refracted back to Earth, it
is not possible to determine this distance using the parallax, principally
because of the ambiguity of its ending (part), that, at different hours
during night-time and from different places around the Earth, does not
allow to accurately compare such distance with the fixed Stars. Anyway
it is possible to ascertain such distance is great from the circumference
of its 24 hour daily motion, next to the Stars.
Following a common thinking, could a raging wind
carry this substance for a whole month through the air without dispersing
it with its impetuosity, pushing it around the Earth in such uniform way
and allowing it to always match the same constellations? On the contrary,
if the Copernican hypothesis must be followed, with what kind of force
could it try to put up a resistance to the daily motion of the elementary
sphere from West to East, without being dispersed or diverted? It
then must be admitted that this substance is above the elementary sphere
and consequently is in the Upper Sky.
Considering that its particular motion is imperceptible, it must be assumed
that this substance is extremely noble and near to the region of the Stars.
Our ancestors were right when they deemed nearer
towards the fixed stars those stars that, among the planets, are nearer
to their universal motion and less to their particular motion. Only for
this precise reason they deemed Saturn
most noble among all other planets and placed Jupiter
above it. No astronomer in the last 20 or 30 centuries ever doubted
this convincement. They even confirmed (their
assumptions) with new hypothesis used to represent the motion of such events,
even though (such hypotheses) were diverse one from another and sometimes
even conflicting, as the Copernican theory was towards the Ptolemaic
theory and that of Tycho’s.
Each theory explained the order of the superior planets as ascertained
by our ancestors. Being impossible to explain such order without the aid
of a hypothesis, each single theory made use of particular conjectures.
These two planets have no definite parallax,
because the diameter of their circumferences and that of the Earth’s
is not proportioned. It is therefore a
good rule to establish the universal position of any new object, taking
into consideration its motion and that of other bodies known to us, which,
through astronomical observations, are found to be lined up at different
distances in accordance to their different apparent velocity. |