Astronomy Immersion

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The astronomy immersion provides students with the opportunity for additional study in astronomy in order to build a secondary area of expertise in support of their major or other areas of interest. The immersion offers a broad background in astronomy with courses providing a broad survey of modern astrophysics and the techniques and technologies used to investigate astronomical phenomena. 

Notes about this immersion:

  • This immersion is closed to students majoring in imaging science and physics.

The program code for Astronomy Immersion is ASTRO-IM.

Curriculum for Astronomy Immersion

   University Physics I
This is a course in calculus-based physics for science and engineering majors. Topics include kinematics, planar motion, Newton's Laws, gravitation, work and energy, momentum and impulse, conservation laws, systems of particles, rotational motion, static equilibrium, mechanical oscillations and waves, and data presentation/analysis. The course is taught in a workshop format that integrates the material traditionally found in separate lecture and laboratory courses.
   University Physics II
This course is a continuation of PHYS-211, University Physics I. Topics include electrostatics, Gauss' law, electric field and potential, capacitance, resistance, DC circuits, magnetic field, Ampere's law, inductance, and geometrical and physical optics. The course is taught in a lecture/workshop format that integrates the material traditionally found in separate lecture and laboratory courses.
Required course
   University Astronomy
This course is an introduction to the basic concepts of astronomy and astrophysics for scientists and engineers. Topics include the celestial sphere, celestial mechanics, methods of data acquisition, planetary systems, stars and stellar systems, cosmology, and life in the universe.
Choose two of the following:
   Stellar Astrophysics
This course presents concepts of stars and stellar systems at an intermediate level. Topics include the observed characteristics of stars, stellar atmospheres, stellar structure and evolution, interaction of stars with the interstellar medium, and the populations of stars within the Milky Way Galaxy.
   Galactic Astrophysics
This course describes the structure and dynamics of the Milky Way galaxy. It provides an overview of the major constituents of the Milky Way, their interactions, and the methods by which astronomers study them.
   Extragalactic Astrophysics and Cosmology
This course provides a survey of the structure of the universe on the largest scales, including galaxies and clusters of galaxies. The course also provides an overview of the history of the universe from the Big Bang to the current day, and describes the observational evidence for our current values of the cosmological parameters.
   Observational Astronomy
This course provides a practical, hands-on introduction to optical astronomy. Students will use the RIT Observatory's telescopes and CCD cameras to take images of celestial objects, reduce the data, and analyze the results. The course will emphasize the details of image processing required to remove instrumental effects from CCD images.