Giovanni Domenico Cassini was born in Perinaldo in 1625,
and already as a student showed great talent
in mathematics and astronomy. He was trained in astronomy
by two able astronomers, G.B. Riccioli and F.M. Grimaldi.
Aged only 25, be was made Professor
of Astronomy at the University of Bologna. Invited by the
French King Louis XIV, to help in the design and construction
of the
forthcoming Observatoire de Paris, Cassini departed for France in 1669.
Although his visit was originally intented to be limited duration,
Cassini warmed up to France to the point of accepting the directorship
of the Observatory in 1671,
and never returned to Italy. He changed his name to
Jean Dominique, and became a French citizen in 1673. He died in Paris
on 14 September 1712.
Cassini established his reputation in Italy by careful and
accurate solar and planetary measurements, which allowed him
to produce improved planetary tables, as well as improved versions of
Galileo's
tables for the
moons of Jupiter,
then of great
interest because of their potential use for determining
longitudes at sea. He was also involved in numerous engineering
projects, including fortifications and hydraulics.
While in Bologna Cassini
also measured the rotation periods of Mars and Jupiter.
As director of the Observatoire de Paris, Cassini inaugurated,
among other projects,
a sustained solar observing program. Carried out primarily
by the Jesuit Jean Picard (1620-1682),
and later by Philippe de La Hire (1640-1718),
this program included sunspot observations as well as
measurements of the solar diameter.
Cassini's own interests remained in geodesy and planetary astronomy;
He carried out extensive observations of Earth's Moon, and
between 1671 and 1684 he discovered four Moons of Saturn
(Iapetus, Rhea, Tethys and Dione). In 1675 he also discovered
the main division of Saturn's ring, and correctly speculated on their
physical constitution as being a collection of small debris.
In 1672 Cassini effectively recomputed
the size of solar system from a determination
of the Martian parallax at opposition, from accurate measurements
of Mars' position carried out simultaneously by himself in Paris
and by fellow observer Jean Richer (1630-1696) in Cayenne, South America.
Cassini's resulting value for the astronomical unit (Sun-Earth distance)
was accurate to better than 90%, although the manner in which Cassini
decided which of his multiple data to retain for the calculation,
and which to throw out, has baffled science historians ever since.
Clearly an outstanding observer, Cassini was however quite conservative
on physical theories; he resisted both the Copernican model of the solar
system, as well as the concept of a finite speed of light put forth
by his collaborator Ole Römer (using Cassini's own data!).
By 1710 Cassini had turned blind, and his younger son Jacques
(1677-1756, a.k.a. "Cassini II") took over as
director of the Observatoire de Paris, himself succeeded by his
own son César-Francois (1714-1784, a.k.a. "Cassini III"),
followed in turn by his own son Dominique (1748-1845, a.k.a. "Cassini IV").
The Observatoire de Paris thus remained under the leadership of
the Cassini family for over 120 years, until Dominique
resigned his position in 1793 for political reasons.
Bibliography:
Porter, R. (ed.) 1994, The Biographical Dictionary of Scientists,
Oxford University Press.
van Helden, A., 1994, Measuring the Universe,
Galileo
Tycho
Hevelius
Janssen
Lyot
|