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Transcript
Hot
•
OBeAFineGirlKissMe.
Hottest stars on left
Absolute magnitude measures
brightness with all stars
placed at same distance
–
–
Giants
Brightest stars on top
An increase of 2.5
magnitudes ⇒ star is a factor
of 10 fainter.
Model
–
–
1.
2.
White
dwarfs
Dwarfs
Temperature
Size (therefore names dwarfs
& giants)
Faint
•
The Hot-plate Model of a Star
Spectral Class
–
–
Absolute Magnitude
•
Luminous
Model of Stars—
3 Oct
Spectral Class
3.
How does the energy from the
hot-plate get to my hand?
What are two ways to make a
hot plate produce more
energy per second? (The same
question applies to a star:
What are two ways to make a
star brighter or more
luminous?)
What can I do to make the
same hot-plate at the same
setting burn my hand and not
burn my hand?
Astrophysics and twentieth-century astronomy to 1950,
O Gingerich, ed., Cambridge, 1984
Model of a Star: Temperature
• Thermal radiation, also called blackbody radiation
– Emitted by anything warm
– Brighter for hotter objects
– Wavelength changes with
temperature
• λpeak ×T=2.9mm K (Wien’s Law)
• For the sun, T=5700K and λpeak
=2.9mm/5700K=.0005mm=500nm
• For a person, T=273+37=310K.
λpeak =2.9mm/310K=.01mm
(infrared)
• A star or hot plate emits radiation.
Energy emitted per second depends
on Area×T4.
http://www.acemart.com/graphics/00000001/products/WELLh70_01.jpg
Luminosity & Flux of Stars
• Luminosity = amount
of energy per second
produced by the star
– L=R2T4
• Flux = energy per
second received by a
detector on earth
– F=L/D2
Supernova 1987a in the Magellanic Cloud
What quantity or quantities have changed?
1
Magnitudes of Stars
• Definition of apparent
magnitude
– The magnitude of Vega is 0.
– For every factor of 10 fainter,
the magnitude is 2.5 greater.
– More generally
• m=-2.5 log (flux/fluxVega)
• Absolute magnitude is
apparent magnitude if the
distance of the star is 10 pc.
http://obswww.unige.ch/~cramer/images.jpg/sirius-l.jpg
Sirius A and Sirius B
Summarizing question
Walter Adams 1876-1956
• Apparent mag of Sirius A
is -1.5
• Apparent mag of Sirius B
is 8.7
• Sirius A & B orbit each
other.
• In 1914, Walter Adams
measured the colors of A
and B to be about the
same. What did he
discover?
• How can a star at the same temperature and
the same distance as the sun be much
brighter?
http://chandra.harvard.edu/photo/2000/0065/0065_optical.jpg
2