Angelo Secchi was
born on 18 June 1818 in Reggio, Italy. He joined the Jesuit at age 15,
began his theological studies in 1844, and was ordained priest in
1847. In 1839 he began
lecturing on physics and mathematics at the Jesuits'
Collegio Romano. In 1848, due to the political unrest in Italy that led to
the general expulsion of the Jesuit order, he traveled to England, then
to Georgetown University, near Washington, where he taught the natural
sciences. He was back in Europe within a year,
and in 1852 returned to Rome,
founding a new observatory at the Collegio Romano. He remained
based in Rome until his death, on 26 February 1878.
Secchi made many important contributions to the astronomy of
his days, in particular on stellar spectral classification. He was the first
to make systematic use of spectroscopy in stellar classification. His
four class scheme prevailed throughout much of the second
half of the nineteenth century, and paved the way for all later
classification schemes.
Secchi was also extremely active in
solar physics, an area he became interested in during his stay in
America. He studied prominences during eclipses, both visually
and spectroscopically, and provided the first demonstrations that prominences
are features belonging to the Sun. He wrote a number of astronomical
books in Italian, some quite technical, others aimed at the general public,
and one for children.
His influential solar monograph Le Soleil
was first published in Paris in 1870, with a German translation appearing in
18XX and the second French edition in 1875.
Secchi was the first astrophysicist to suggest that the solar core is in
a gaseous state, with the temperature steadily decreasing from the
center to the surface. Some of his theories on
sunspots, granulation and prominences would
today be considered obsolete, but their influence on nineteenth
century astronomy and solar physics was considerable.
He was elected to England's Royal Society and Royal Astronomical
Society, of the French Académie des Sciences, and of Russia's Imperial
Academy of St. Petersburg. In Italy he presided for many years over the
Accademia dei Nuovi Lincei, and founded the Societa degli Spettroscopisti
Italiani, devoted to spectroscopic studies of the Sun.
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