Interactive Demonstrations
GENERAL EDUCATION COURSES
Demonstration
Description
Applies to
Text-only Summary
Kepler's
Laws
Examine Kepler's Laws of planetary motion by picking orbit sizes and shapes and viewing the resultant motion.
ASTR 10
Kepler's Laws Text
Planetary
Spectra
See how the visible and IR spectra of airless planets vary with star temperature and brightness, planet distance and albedo
ASTR 10
Planet Spectra Text
Build a
Planet
Watch an animated display of the formation and evolution of a terrestrial planet based on your choices of mass and orbit distance
ASTR 10
Planet Evolution Text
Visual Spectra
of Objects
View visual and graphical representations of the visible spectra of various objects
ASTR 10
ASTR 101
Spectra Text
Planck
Spectrum
Change the temperature and see how the spectrum and visual color impression of a star change
ASTR 101
Planck Spectrum Text
Energy
Levels
See how transitions within the energy level structure of an atom produce a unique line spectrum
ASTR 101
Energy Levels Text
Evolution of
a Star Cluster
See how the HR diagram and visual appearance of a star cluster change with time
ASTR 101
Cluster Evolution Text
Lunar
Phases
Select a month and year to produce a monthly lunar phase calendar for some of the author's favorite cities
ASTR 102
Lunar Phases Text
Coordinate
Conversions
Convert the astrolabe Azimuth and Altitude values to RA and Dec for ASTR 102 Lab #5 (Plotting the Moon's Orbit)
ASTR 102
Coordinate Conversion Text
Spectral Classes
& H-R Diagram
A lab exercise in which spectral classes and magnitudes of stars in a cluster are estimated and an H-R Diagram is produced and analyzed
ASTR 102
On-Line Lab Text
ASTROPHYSICS COURSES
Demonstration
Description
Applies to
Text-only Summary
Effective Potential and Integrated Motion
Explore the effective potential and integrated motion for various force laws
ASTR 117A
Effective Potential Text
Planet Stability in Binary Star Systems
Determine which planetary orbits are stable in various binary star systems
ASTR 117A
Planet Stability Text
Stellar Models and Spectra
See how the strength and shape of spectral lines change as stellar physical parameters (T, g & abundances) are varied
ASTR 117B
Stellar Models and Spectra Text
Disk Galaxy Simulation
Examine the development of structure in a two-dimensional, collisionless-particle disk galaxy
ASTR 117B
Galaxy Simulation Text
Nuclear Isotope Stability
Examine the stability of nuclear isotopes as precicted by the semi-empirical mass formula
ASTR 117B
Nuclear Stability Text
[
Astro Philes Home Page
] [
SJSU Home Page
]