Lecture 13 - Star Patterns Flashcards
what are the axes of the HR diagram?
X: temp (increasing right to left)
Y: luminosity
what are the 3 types of stars on the HR diagram and their properties?
- main sequence (most)
- supergiants, giants –> cooler, brighter, larger
- white dwarfs –> hotter dimmer, smaller
what is the magnitude scale?
LOWER magnitude = BRIGHTER star
why is the magnitude calibrated to the response of the human eye?
our eyes detect brightness better than size –> i.e. if we zoom in on a star, its size doesn’t change much
what is apparent magnitude? and its equation?
what happens to apparent brightness if there is a larger apparent magnitude?
describes how bright a star appears in the sky
equation: (m_1 - m_ref) = -2.5log_10 * (I_1/I_ref)
larger apparent magnitude = dimmer apparent brightness (I)
what is m_ref?
magnitude of the star Vega = 0
if apparent magnitude (m) changes by 5, how does apparent brightness change?
changes by a factor of 100
what is absolute magnitude? and its equation?
what do we need to consider?
describes the intrinsic brightness of a star
m - M = 2.5 log_10 (d/10)^2 = 5(log_10*d - 1)
must consider the distance from earth in parsecs!
if apparent magnitude changes by 5, how does distance change?
distance changes by a factor of 10
if star A has an apparent magnitude of 0 and star B has an apparent magnitude of 5, how much brighter is star A than star B?
if star A and B have the same absolute magnitude, how much further away is star B than star A?
Star A: 100x brighter
Star B: 10x further away (100x dimmer)
what do stellar luminosity classes indicate?
indicate radius and luminosity of a star
what does stellar luminosity classes indicate vs spectral type?
stellar luminosity classes –> radius and luminosity
spectral type –> surface temp and colour
what are the 5 stellar luminosity classes and how does size and luminosity change between them?
I –> supergiant
II –> bright giant
III –> giant
IV –> subgiant
V –> main-sequence star
size and luminosity decrease from I - V
what 3 properties of stars can we infer from HR diagrams that display temp and luminosity?
- colour
- spectral type
- radius
why are red stars usually large?
they emit light with lower energy (red) so to reach a high luminosity, they need to increase their size
what size of star emits blue light vs red light? why?
blue light is high energy so the star is small
red light is low energy so the star is large
what are stars doing when they are in the main sequence? how much of their lifetime is spent in the main sequence?
actively fusing H –> He
stay in main sequence for most of their lifetime in a fixed position on the main sequence
do high mass stars have long or short lifetime? describe why?
high mass stars have shorter lifetime
they have more H so they fuse H –> He very quickly and use it up more quickly, therefore shorter lifetime