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SCHOOL OF PRACTICAL ASTRONOMY.
Professor Stone.
B. A.
General Astronomy.—The primary aim of this course is to give such
a knowledge of the facts, principles, and methods of Astronomy
as every well-educated person should possess.
The preparation required is a good working knowledge of Arithmetic,
Algebra through Quadratics, Plane and Solid Synthetic Geometry,
and Plane Trigonometry through the Solutions of Triangles. In
this preparation thoroughness is of more importance than extent.
The instruction is given by oral examinations, by lectures, and by
the assignment of problems. The mental discipline of the student is
kept constantly in view, and an earnest effort is made to create a habit
of clear and logical thinking.
Text-Books.—Young's General Astronomy; Berry's A Short History of
Astronomy.
GRADUATE COURSES.
M. A.
The courses mentioned in the paragraph following this, although
primarily designed to meet the wants of candidates for the degree of
Doctor of Philosophy, are also open to candidates for the degree of
Master of Arts, who are required to satisfactorily complete, in addition
to the work of the B. A. course, a year's work in the more
advanced courses.
PH. D.
Theoretical Astronomy.—The courses offered vary from year to year.
During the year 1899-1900 lectures introductory to Celestial Mechanics
will be offered, special attention being given to the Problem of Two
Bodies.
Practical Astronomy.—Laboratory courses are offered each year, in
which systematic training is given in numerical computation, and in
the use of Astronomical instruments. Students are also encouraged to
engage in such original work as their time and attainments may
permit.
A Seminar is held twice a week, at which lectures are given on
assigned subjects by the more advanced students.
Completion of the M. A. course in the School of Mathematics or that
of Natural Philosophy may be substituted, if desired, for the equivalent
work in Astronomy as a qualification for candidacy for the degree
of Doctor of Philosophy by those who elect Astronomy as one of their
subjects.
For information in regard to Fellowships in Astronomy, application
should be made to the professor in charge of the School.
The Astronomical Observatory is situated upon an elevation known
as Mount Jefferson which furnishes an unobstructed horizon. The
principal building is a rotunda forty-five feet in diameter, and contains
the great Clark refractor of twenty-six inches aperture. The building
and instrument are the gift of Leander J. McCormick, Esq., of
Chicago. The computing rooms are adjoining, and contain clock,
chronograph, etc., and a working library. In a smaller building are a
three-inch Fauth transit and a four-inch Kahler equatorial.
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