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अंतर – विश्वविद्यालय केंद्र : खगोलविज्ञान और खगोलभौतिकी                                                                                                          Inter-University Centre for Astronomy and Astrophysics

अंतर – विश्वविद्यालय केंद्र : खगोलविज्ञान और खगोलभौतिकी Inter-University Centre for Astronomy and Astrophysics

An Autonomous Institution of the University Grants Commission

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M.Sc. Courses at Savitribai Phule Pune University

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M.Sc. Courses at Savitribai Phule Pune University (SPPU)



IUCAA M.Sc. Teaching
IUCAA offers neither a B.Sc. in Astronomy nor an M.Sc. in Astronomy. However, IUCAA faculty are involved in teaching the Astronomy and Astrophysics, Papers I and II of the third and fourth semesters of the M.Sc. programme in Physics at the University of Pune. Astronomy and Astrophysics is an optional course for M.Sc. (Physics) students. Normally, about 10 students are admitted to this course. (Admission to the course is done by the Department of Physics, University of Pune) The syllabus for these courses is given below.
Astronomy and Astrophysics I
Module 1: 3 credits (30 lectures, 15 T/S/D) Overview of the universe
Physics of astrophysics gravity
adiative processe
gas dynamic
Module 2: 1 credit (10 lectures, 5 T/S/D) Stellar physics
Module 3: 1 credit (10 lectures, 5 T/S/D) Galactic physics
Astronomy and Astrophysics II
Module 1: 3 credits (30 lectures, 15 T/S/D) General relativity principles of relativity
geometrical framework of general relativity
solutions to Einstein’s equations and their properties
Module 2: 2 credits (20 lectures, 10 T/S/D) Cosmology cosmological models
physical cosmology and the early universe
Experiments for Astronomy and Astrophysics I and II
(total 5 credits, 120 lab hours)
Temperature of artificial star by photometry
Characteristics of a CCD camera
Solar limb darkening effect
Polar alignment of an astronomical telescope
Estimating the relative magnitude of a group of stars by a CCD camera
Atmospheric extinction for different colours
Differential photometry of a programme star versus a standard star
Effective temperature of a star by B-V photometry
Night sky brightness with a photometer
Distance to the moon by parallax
Calibration of a 1420 MHz radio receiver and spectrometer
Detection of the 21-cm line of neutral hydrogen from our galaxy
Distance to a Cepheid variable
Variability of delta Scuti type stars
Variability of RS CVn binaries
Polarization of day/moon light
Any 10 of these experiments will be covered (5 each in semesters III and IV)
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Last Updated: 12 December 2022

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