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Apr 23, 2024
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Undergraduate Calendar 2015-2016 [-ARCHIVED CALENDAR-]
Honours Astrophysics (B.Sc.)
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Admission Notes
- Completion of ASTRON 1F03 is required by the end of Level II and is strongly recommended in Level I.
- Completion of MATH 1B03 is required by the end of Level II and is strongly recommended in Level I.
Admission
Enrolment in this program is limited and possession of the published minimum admission requirements does not guarantee admission. Selection is based on academic achievement but requires, as a minimum, completion of any Level I program with a Grade Point Average of at least 6.0 including:
9 units
from the Science I Course List (See Admission Notes 1 and 2 above.)
Note:
Students who have satisfied all above admission criteria and have a Cumulative Average between 5.5 and 5.9 will be admitted to the program, on Program Probation. Students may be on program probation only once. Eligibility to continue in the program will require a Cumulative Average of at least 6.0 at the next academic review. Admission (Effective September 2016)
Enrolment in this program is limited and possession of the published minimum admission requirements does not guarantee admission. Selection is based on academic achievement but requires, as a minimum, completion of any Level I program with a Cumulative Average of at least 6.0 including:
9 units
from
- the Science I Course List (See Admission Notes 1 and 2 above.)
Note:
Students who have satisfied all above admission criteria and have a Cumulative Average between 5.5 and 5.9 will be admitted to the program, on Program Probation. Students may be on Program Probation only once. Eligibility to continue in the program will require a Cumulative Average of at least 6.0 at the next academic review. Requirements
121 units total (Levels I to IV), of which no more than 48 units may be Level I 30 units
(See Admission above.) 0-6 units
- Electives (See Program Note 3 above.)
3 units
- Electives (See Program Note 1 above.)
6 units
from
- Level IV Astronomy, Physics
9 units
- Electives (See Program Note 2 above.)
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