| 1 |
Aristarchus'
Method of Determining the Distance to the Moon
Aristarchus'
Method of Determining the Distance to the Sun
Problem
3
Problem
4
Problem
5
Problem
6
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(PDF) |
| 2 |
Copernicus' Method
of Finding the Distance to an Inferior Planet
Copernicus' Method of Finding
the Distance to a Superior Planet
Mass of Jupiter
Dynamical Timescale of the Earth
Geosynchronous Satellite
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(PDF) |
| 3 |
Eccentric Orbits
Doppler Effect
Determination of the AU from
Doppler Shifts
Determining the Mass of a Neutron
Star
Planetary Orbital Periods
Refraction
Optics Problem
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(PDF) |
| 4 |
Short Problems on
the Sensitivity and Angular Resolution of Telescopes
Three-Slit Diffraction Problem
Divergence of a Laser Beam
X-Ray Mirror
Semiclassical Derivation of the
Energy Levels of the Hydrogen Atom
Short Optics Problems
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(PDF) |
| 5 |
Derivation of the
Stefan-Boltzmann and Wien Radiation Laws
Short Answer Questions on Magnitudes
Moving Cluster Method - the Hyades
Cluster
Binary Orbit 1
Binary Orbit 2
Binary Orbit 3
Binary Orbit 4
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(PDF) |
| 6 |
Magnitudes
Planck Distribution
The Visual and Spectroscopic
Binary Sirius A and B
Short Binary Problems from Zeilik
& Gregory
Short Questions on Spectral Types
Eclipsing Binary
Binary Radio Pulsar
|
(PDF - 2.8 MB) |
| 7 |
Spectroscopic
Parallax
Orbiting
Globular Cluster
Spherical,
Uniform-Density Model of the Galaxy
Model
Galactic Rotation Curve
Absorption
in the Galactic Plane
Rotation
Curve
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(PDF) |
| 8 |
Constructing the
Galactic Rotation Curve
Oort Constants
Kinematic Distances
Simplified Model of a Star
Fueling the Sun
Main-Sequence Lifetimes
Nuclear Binding Energies
|
(PDF) |
| 9 |
Dimensional Analysis
of Equations of Stellar Structure
Spectroscopic Parallax for a
Globular Cluster
Ascending the Giant Branch
Mean Density of Collapsed Stars
Cooling White Dwarf
Maximum Rotation Rate for a Pulsar
Pulsar Spin-Down
Blackbody Radiation from a Neutron
Star
|
(PDF) |
| 10 |
Collapsing White
Dwarf
Maximum Distances for Applying
Standard Candles
Distance to a Nova
Optical Luminosity of a Supernova
at Maximum
Cepheid Variables as Distance
Indicators
Variations in the Radius of Cepheid
Variables
|
(PDF) |
| 11 |
X-Ray Burst Source
Accretion Powered X-Ray Source
Interstellar Extinction
21–cm Hydrogen Radiation
Distance to a Dark Cloud
Short Problems
Short Problems
Planetary Nebula
|
(PDF) |
| 12 |
Orbiting Galaxies
Distance Determinations
Galaxy Redshift from the Ca II
K Line
Measuring a Quasar Redshift
Identifying the Lines and Determining
the Redshift of a Quasar
A Simple Determination of the
Hubble Law
Free-Fall Time for a Cluster
of Galaxies
Luminosity Function of Galaxies
in Rich Clusters
|
(PDF) |
| 13 |
Relativistic Doppler
Effect
Cygnus A Radio Galaxy
Feeding a Black Hole
Distance–Redshift Relation
H0, τ0,
and ρcrit
Expanding Balloon Analogy
Scale Factor and Age vs. Redshift
Dust in the Universe
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(PDF) |