Honors Program

University of Minnesota

Department of Astronomy

Description

The Honors Program in IT is designed to improve the educational experience for students with exceptional academic abilities and recognize this accomplishment with an honors degree. The honors program comes in two flavors, lower division and upper division. To obtain a degree from IT with honors, only the requirements of the upper division program must be met. The lower division honors program is separate in the sense that it is preparatory, but not necessary for the upper division program. The IT honors program is run out of rm 136 in Lind Hall. Most of the paper work involved with completing the honors degree will be handled by this office, not the Astronomy DUGS.

Within a broad scope established by IT as a whole, the requirements for an honors degree are the prerogative of the individual departments and their degree programs. To obtain an honors degree in Astrophysics, a student must meet the following criteria:

Degree Minimum U.D. GPA Honors Experiences Senior Thesis
Cum Laude 3.50 2 Normal
Magna Cum Laude 3.66 2 Normal
Summa Cum Laude 3.75 2 Honors


[top]Honors Experiences


[top]Honors Thesis

All Astrophysics majors must complete a Senior Thesis (Ast 4994). Students in the upper division honors program who plan to graduate Summa Cum Laude must complete an Honors Thesis. An honors thesis must involve more original research or greater depth and scope than required for a normal Senior Thesis. Be sure the faculty member you are working with understands this before starting.

Double majors in Physics and Astrophysics who are also in the Physics Honors program must do a Physics Honors Thesis in order to obtain an Honors degree in Physics. A double major does not have to do a separate Astrophysics Thesis (honors or otherwise) if there is some astronomical content in the Physics Honors Thesis. For example, one student measured the absorption of X-Rays by slabs of aluminum in a industrial laboratory. This student then used these results to predict the extinction of X-Rays from celestial sources due to aluminum in the interstellar medium.

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