Chapter 15- Properties of Stars Flashcards
properties of stars
-power source
-density
-age
-size
-temperature
-composition
-distance
-motion
-mass
-luminosity
PDASTCDMML
spectroscopy
measuring spectral lines
how could we go about proving that stars are like our sun, only farther away
confirm that the luminosity is similar to the suns
how do we determine luminosity
- with brightness and distance
- measured in watts
solving for brightness
the inverse square law
parallax
- apparent movement of foreground object relative to some background due to change in the observers location
- best way to measure distance
stellar brightness
lower numbers are brighter and higher numbers dimmer
apparent magnitude
based on how bright object appears from earth
absolute magnitude
how bright the object would be if it were 10 parsecs away
is the suns absolute magnitude higher or lower than its apparent magnitude
higher
how can we determine temp
temp determined by where star “peaks” on electromagnetic spectrum
spectral classification chart
OBAFGKM
-hottest stars to coolest stars
what do absorption lines tell us
ionization and ionization tells us the temp
-therefore absorption lines tells just the temp
spectral type
each spectral class is broken down into 10 subclasses
size, volume, mass differences
size= how big(radius)
volume= how much space
Mass=How much stuff