Last modified 8/22/06. This document is not yet complete.
| Name | Abbreviation | Value |
| ............................ | ............................ | ............................ |
| nano | n | 10^-9 |
| micro | greek mu | 10^-6 |
| milli | m | 10^-3 |
| centi | c | 10^-2 |
| kilo | k | 10^3 |
| mega | M | 10^6 |
| giga | G | 10^9 |
| ............................ | ............................ | ............................ |
| Name | Formula | Notes | Text Page | |
| ............................ | ............................ | ............................ | ............................ | |
| Wien's law | lambda_max is 0.29 cm / T | lambda_max is the wavelength of peak blackbody radiation; T is the temperature in K | 76 | |
| Doppler effect | apparent wavelength / true wavelength is 1 + v/c | v is the velocity of the object; c is the wave speed - the speed of light for the Doppler effect in astronomy | 77 | |
| small angle formula | see Angle Measurement Lab | |||
| apparent brightness | apparent brightness is proportional to L/D^2 | L is luminosity, D is distance | 443 | |
| Kepler's 3rd law | M=R^3/P^2 | M is the mass enclosed by the orbit (in solar masses), R is the orbit radius (in AU), P is the orbit period (in yr) | 622 | |
| ............................ | ............................ | ............................ | ............................ | |
| stellar magnitude | m1-m2= -2.5 * log_10(b1/b2) | m1 & m2 are the apparent magnitudes of object 1 & 2, b1 & b2 are their brightnesses | 445 | |
| apparent magnitude | m=M+5log_10(D/10 pc) | m is apparent mag, M is absolute mag, D is distance | 445 | |
| ............................ | ............................ | ............................ | ............................ |
The absolute magnitude of the Sun: 4.83
AU (astronomical unit): 1.5E8 km
ly (lightyear): 9.5E12 km
pc (parsec): 3.3 ly which is 3.1E13 km
More are given on the back of the front cover of the text.