The Master of Science in Astronomy and Astrophysics at the University of Michigan equips students with theoretical and observational skills to explore the universe—from nearby stars and exoplanets to the vast structure of the cosmos. The program fosters advanced research in stellar dynamics, cosmology, and galactic evolution.
Dark Matter Distribution in Spiral Galaxies Using Rotation Curves
Spectroscopic Analysis of Exoplanetary Atmospheres
Simulating Galaxy Mergers and Starburst Triggers
High-Resolution Mapping of the Cosmic Microwave Background
Gravitational Lensing as a Tool for Detecting Distant Galaxy Clusters
Radiative Transfer Modeling in Protoplanetary Disks
Pulsar Timing Arrays for Gravitational Wave Detection
Simulating Supernova Explosions Using Hydrodynamic Codes
Detection of Habitable Zone Planets Using Transit Photometry
AGN Feedback Mechanisms in Galaxy Evolution
Quantifying Metallicity Gradients in the Milky Way
Studying Stellar Oscillations with Asteroseismology Data
Measuring Hubble Constant with Standard Candles and Rulers
Multi-Wavelength Observations of Star-Forming Regions
Polarimetry of Interstellar Dust and Magnetic Fields
Investigating Quasar Variability Across Redshift
3D Mapping of Stellar Populations in Globular Clusters
X-Ray Emissions in Neutron Star Binaries
N-Body Simulations of Galaxy Cluster Dynamics
Radio Observations of Fast Radio Bursts
This program offers a rigorous pathway into academic and observational research careers in astrophysics and related space sciences, supported by world-class faculty and observatory collaborations.
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