| Cassini,
his initial steps
Cassini started his studies in Genoa at the
Jesuit College. He was a brilliant pupil,
well up in literary [he loved Latin,], and in scientific subjects.
At the Abbey of San Fruttuoso [near
Camogli], under the guidance of Abbot
Doria, he thoroughly studied the Rudolphine
Tables,
the Alfonsine Tables
and the Elements of Euclid.
Soon after, Senator Giambattista Baliani,
a man with broad views and very much open minded toward science, in
close relationship by letter with Galileo,
became an important teacher for Cassini,
who discovered how flexible this noble man was and how open his opinions
were, an attitude and an approach so much different to that of the Jesuits,
that, however, Cassini always remembered with pleasure during all his life.
The virtues of Cassini became known
and the support of many friends opened
to him the doors of the prestigious University of Bologna,
where he was given the chair of Astronomy
in 1651.
Cassini – observation of a
comet ...
In 1652, Cassini
was able to observe a comet that passed
over Bologna.
Its position was nearly vertical over
the city, an event that favoured the quality of the observation.
He assumed the orbit was too much eccentric
and far away to compute the parallax.
Moreover, he assumed it had the same type
of motion of other celestial bodies [confirming
some of Tycho’s assumptions].
The Heliometer and the motion
of the Sun
Urgent and important problems
were related to the accuracy of the motion
of the Sun, i.e. the dates
of the Liturgical Calendar.
An unexpected opportunity arose all of a sudden:
in Bologna, San Petronio, was undergoing
great restoration works and the old Danti’s Sun-dial was to be done away
with..
Cassini aware of this happening,
understood there was enough space for a new instrument, which he called
"heliometrum":
it had gigantic proportions. The local meridian line was traced on the
floor. The opening cerimony took place
on 21 June 1655,
the Summer solstice.
With the Heliometer he proved
Kepler was right
Measuring the diameter of the Sun at the two solstices,
Cassini could measure the eccentricity
of the Solar orbit around the Earth, coinciding with that "bisected",
foreseen by Kepler.
Undoubtedly, the validity of Kepler’s theories, at times so much criticized,
was "scientifically"
confirmed.
The obliquity of the ecliptic
was measured with the Heliometer
The obliquity of the ecliptic is given by the
angles the Sun traces at the two solstices.
Its measurement was not difficult to take, but the
nearly 67 metres
long heliometer allowed an accuracy never reached before.
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Cassini established the period
of revolution of the Medicean’s planets and determined the rotation periods
of Jupiter and Mars
Cassini measured with extreme accuracy the apparition
and the disappearance of the Medicean planets. The observation of their
reciprocal eclipses allowed him to precisely determine the longitude, thus
solving one of the biggest problems of his time.
The Medicean planets are an "unparalleled
watch", visible
from Earth, from different positions that can also be far away from each
other: indeed, we can use them as an astronomical Harrison chronometer.
Cassini, also, observed that the
transit of the shadow of the satellite "Io"
is delayed when the Earth is moving away
from Jupiter and anticipated
when the Earth is approaching Jupiter.
At first, Cassini assumed this phenomenon was
due to the "finite"
velocity of light, but abandoned this hypothesis, because
with the other three satellites he was not able to observe a similar situation.
Cassini’s
assumption was not correct, as he did not understand that the reason was
not the absence of the phenomenon, but the intrinsic difficulty required
by the measurement, due to the slowness at which these satellites passed
by.
His assistant Roemer,
on the contrary, in no time, availed himself of this opportunity and determined
the speed of light with good accuracy.
These careful observations allowed Cassini to
discover Jupiter’s
superficial formations and to determine Jupiter’s
rotation period.
Cassini also determined the
rotation of Mars.
The picture shows some of the Cassini’s drawings of the Martian formations.
Blood transfusions
" In 1667
Cassini
gave news of his experiments on blood transfusion and on the observations
he had carried out on insects.
In two letters, both published in the Summer
of year 1667, one addressed to Berlingiero
Gessi, Ambassador in Rome of the Bolognese
Government, and the other one addressed to Michele
Giustiniani, a historian, Cassini announced
the success of his experiments on two lambs
and described in detail all the steps of the experiment and the innovative
techniques he had followed, i.e. the use he made of the hen’s
feather quill, in place of the metal cannula , which allowed, due to its
transparence, to visualize the flow of the blood,
and to regulate it accordingly" (*).
The zodiacal light
At the beginning of Spring,
in 1668, he
observed a luminescence, triangular in shape,
on the ecliptic plane, very much alike to the Milky Way. He called it "zodiacal
light". He
could not understand the phenomenon. Today
we know it is due to residual interplanetary dust stagnating on the ecliptic,
that, in particular conditions, becomes visible from Earth, when illuminated
by the Sun.
Cassini, cartographer of France
" It was a back-breaking
task, that on which Cassini
started to work since some years trying to improve
the determination of longitude, so as
to draw maps always more precise and detailed. His
method made use of the eclipses of Jupiter’s satellites. This
was the starting point onto which his great cartographical work was based.
It was developed, day after day, with the contribution of scientific groups:
many of them working far away from Paris; all of them, in a certain way,
"co-ordinated" by the "Observatoire". The
French King, and his Minister Colbert, attaching primary importance to
this problem, subsidized the project with great generosity. Cassini was
extremely meticulous and a ... great organizer ".
(*)
z (*) Bibliography: Anna
Cassini - "Un'avventura tra le stelle - Gio. Domenico Cassini da Perinaldo
alla corte del Re Sole",
published by: Comune di Perinaldo
Cassini - observation and
drawings of the Solar spots
Cassini discovered some of Saturn’s
satellites - the famous "division" between the rings
Japetus 1671
Rhea 1672
Cassini Division 1675
Dione 1684
Tethys 1684
Cassini determined the parallax
of Mars
The simultaneous
observation of Mars,
with respect to stars nearby, carried out by
Cassini in Paris
and by
Jean Richer at Cayenne
(French Guiana), allowed to compute the parallax.
Cassini studied the motion
and the orography of the Moon
Cassini measured the
oscillations of the Moon, called "librations"
and explained their origin. He also analyzed the particular motion of the
Moon in synchronous resonance with the Earth [the Moon always points
the same face toward the Earth, because its motions of rotation and revolution
are same]. These studies allowed the formulation
of significant statements in celestial mechanics, known as "the
three laws of Cassini".
In 1679, Cassini completed the great Map
of the Moon.
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A Map of the
Moon was put down by Cassini
between 14 Sept. 1671 (Barthalot, 1982,
p 48) and the beginning of 1679
On Sat. 18 Feb. 1679
the imprinting
was presented to the "Académie"
members
(i.e. during the weekly meeting of the
Physics group).
source:
http://www.leidenuniv.nl/fsw/verduin/
stathist/huygens/acad1666/index.html
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Map of the Moon by Cassini
2nd edition: the 1st edition is dated 1679. Imprinted
by Jean Patigny.
The second edition is dated 1787.
20 'Pouces de
Paris' (54 cm)
- diameter.
This second edition is same as the first one,
except for the text:
"Carte de la Lune
... de Jean
Dominique Cassini"
Imprinted on the back side.
source:
http://www.leidenuniv.nl/fsw/verduin/
stathist/huygens/acad1666/index.html
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Cassini presents the four
fundamental laws of celestial mechanics
These laws make reference to a body in resonance
(rotation – orbit) with its main body of reference [i.e.
Earth and Moon
or Sun and Mercury].
The laws are based on the hypothesis of a Keplerian orbit (reference is
made to Mercury), with a constant precession of the nodes and of the pericentre.
(a) The body has an uniform rotation about
the principal axis of inertia and the rotational angular velocity is equal
or very near to a 3/2 n.
(b) The direction
of the rotational axis of the body and the normal to the orbital plane
form a constant angle.
(c) The direction of the rotational axis
of the body, the normal to the orbital plane and the axis of the orbital
precession are coplanar.
This is trivial in the
case of simple Keplerian motion. It is true with precession, and can be
demonstrated algebraically.
(d) Whenever
a body passes at the pericentre of its orbit, the axe of minimum moment
of inertia is facing the Sun.
Cassini, today, would be a
"top manager"
The way he set up the "Observatoire", an astronomical
centre in continuous contact with other excellent organizations around
the world; the way he was able to co-ordinate simultaneous observations
such as that of Mars, emphasize his extraordinary
managerial qualities and his pragmatical
approach to matters. His
cartographical and hydrogeological commitment was an effort of titanic
dimention: measurements were taken in
very severe environmental conditions, both for men and instruments. For
the latter, Cassini developed special engineering techniques, an anticipation
of the so called "rugged",
made instruments for military use, resistant to ambient and mechanical
stress. A man of great intelligence that
honoured his Country: Liguria ...
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