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Astronomy Test 1
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Distance Modulus
Luminosity
Energy per time
Flux
Apparent brightness
Luminostiy per unit area
Energy per unit time per unit area
Equation for Flux
Apparent magnetudes
Absolute magnetudes
Bolometric Magnetude
Temperature approximation using color index
Radii of stars
Luminosity and Temperature
Masses
Radii, Luminosities, and Temperatures
Types of Bianaries
Apparent
Visual
Spectroscopic
Eclipsing
Astronomic
Hydrostatic Equilibrium
Opacity
Mean Free Path
HR Diagram axis
Absolute magnitudes or Luminosity
Spectral types or Effective temperature
Spectroscopic Parallax
After finding a stars classification (from absorbtion lines) compare on HR Diagram to similar stars to find approximate absolute magnitute. Use the distance modulus to find distance.
Equations of Steller interrior
Hydrostatic Equilibrium
Mass Continuity
Energy Transport (radiative and convective)
Energy Generation
Mass Continuity
Equation of Radiative Energy Transport
Equation of Convective Energy Transport
Equation of Energy Generation
Gravitational Potential Energy
Nuclear Fussion in the Sun
Random Walk Motion
Bianary Mass-Orbital Radius Relationship
Boltzmann's Equation
Ratio increases as T goes to infinity
Mass Function
Wien's Law
Population I stars
Young
High metal content
Formed from dead stars
All O and B are PopI
Population II stars
Old
Low Metal content
First stars to form
Low mass
Author
Robertfoster
ID
132493
Card Set
Astronomy Test 1
Description
Review
Updated
2012-02-03T00:20:15Z
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