Introduction to Astronomy
Overview
1. Classroom
- Discovering the night sky
- History of astronomy
- Properties of light
- Telescopes
- Earth-Moon-Sun system
- Solar system
- Birth, life and death of stars
- Galaxies
- Cosmology
- Alien Life
2. Laboratory
- Sky charts
- Night sky observations
- Ellipses
- Scale of the solar system
- Image formation via mirrors and lenses
- Light spectra/wavelength measurements
- Sunspots
- Photometry
- Planetarium/observatory field trip
This course will be presented using lectures, assigned readings and laboratory exercises, which will include outside observations. A variety of audio-visual materials, computer simulations, and internet searches will be used where appropriate.
Evaluation will be carried out in accordance with ºÚÁϱ¬ÁÏÍø policy. The instructor will present a written course outline with specific evaluation criteria at the beginning of the semester.
Evaluation will be based on the following:
- minimum of two tests administered during the semester 30-40% (15%-25% for each test)
- submitted laboratory reports 20-25%
- quizzes, assignments (possibly online), projects 10-20%
- final examination 30-40%
Upon completion of the course the student will be able to:
- describe the scientific method, and explain how it is applied to the study of the universe
- identify major paradigm shifts in the historical development of astronomy
- identify major stars, constellations, and commonly used coordinate systems for viewing the sky
- explain the cycles of the sky (Earth, Moon, and Sun system) including: seasons, eclipses, tides, phases of the Moon, and precession
- state Kepler’s Three Laws, Newton’s Three Laws and Newton’s universal law of gravitation and demonstrate understanding of these laws through the solution of problems
- identify and explain features and properties of light including: wave-particle duality, speed of light, reflection, refraction, scattering, and the Doppler effect
- explain the appearance of atomic spectra using the Bohr model of the atom
- explain the operation of telescopes
- explain the currently accepted model of the formation and evolution of the solar system
- discuss the characteristics of the various bodies in the solar system
- identify prominent features of the Sun including: sunspots, the solar cycle, solar flares, and coronal mass ejections
- explain how the spectrum from a star can be used to determine characteristics of the star such as: temperature, composition, size, radial velocity, and rotational speed
- explain the features of a Hertzsprung-Russell diagram including: luminosity, temperature, radius, apparent magnitude, spectral class and luminosity class
- explain how binary star systems are used to determine the diameter and mass of stars
- discuss and explain different methods used to determine distances to stars and galaxies including: stellar parallax, spectroscopic parallax, and standard candles (Cepheid Variables, Type I supernova)
- explain how stars are formed, the role of fusion in energy production, and the evolution of stars as they age
- discuss and explain the death of stars, and the formation of white dwarf stars, neutron stars, and black holes
- discuss the consequences of general relativity near a massive object such as: spaghettification, time dilation, gravitational redshift, and the event horizon of a black hole
- classify galaxies based on their appearance
- explain the currently accepted model of cosmology including: the Big Bang, dark matter, dark energy, and the acceleration of the rate of expansion of the universe
- explain the significance of Hubble’s Law
- discuss the likelihood of alien life, and the challenges involved with the Search for Extra-Terrestrial Intelligence (SETI)
Consult the ºÚÁϱ¬ÁÏÍø Bookstore for the latest required textbooks and materials. Example textbooks and materials include
Astronomy by Open Stax and
ºÚÁϱ¬ÁÏÍø, Astronomy 1105 Laboratory Experiments
Requisites
Prerequisites
BC Foundations of Math 11 (C or higher) or BC Pre-Calculus 11 (C or higher)
Corequisites
Courses listed here must be completed either prior to or simultaneously with this course:
- No corequisite courses
Equivalencies
Courses listed here are equivalent to this course and cannot be taken for further credit:
- No equivalency courses
Course Guidelines
Course Guidelines for previous years are viewable by selecting the version desired. If you took this course and do not see a listing for the starting semester / year of the course, consider the previous version as the applicable version.
Course Transfers
These are for current course guidelines only. For a full list of archived courses please see
Institution | Transfer details for ASTR 1105 |
---|---|
Camosun College (CAMO) | CAMO ASTR 101 (3) |
Capilano University (CAPU) | CAPU ASTR 107 (4) |
Kwantlen Polytechnic University (KPU) | KPU ASTR 1100 (4) |
Okanagan College (OC) | OC ASTR 111 (3) |
Simon Fraser University (SFU) | SFU PHYS 190 (3) |
Thompson Rivers University (TRU) | TRU ASTR 1140 (3) |
Trinity Western University (TWU) | TWU PHYS 215 (3) |
University of British Columbia - Okanagan (UBCO) | UBCO ASTR_O 122 (3) |
University of British Columbia - Vancouver (UBCV) | UBCV ASTR_V 1st (3) |
University of Northern BC (UNBC) | UNBC ASTR 120 (3) |
University of the Fraser Valley (UFV) | UFV PHYS 1XX (4) |
University of Victoria (UVIC) | UVIC ASTR 1XX (1.5) |