From the HR diagram above, we could determine that the star Barnard's Star has a temperature 3.03E+3 K and a luminosity of 4.79E-3 Lsun. What then is its radius measured in meters? m (It may help you to know that 11 in 38 x 1026 Watte Leo 3 1415 for Pi
From the HR diagram above, we could determine that the star Barnard's Star has a temperature 3.03E+3 K and a luminosity of 4.79E-3 Lsun. What then is its radius measured in meters? m (It may help you to know that 11 in 38 x 1026 Watte Leo 3 1415 for Pi
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
Transcribed Image Text:luminosity (solar units)
106
105
104
103
102
13
10
0.1
10-2
10-3
10-4
10-5
60 Msun
30 Msun
10 Solar Radli
Lifetime
10 yrs
1 Solar Radius
0.1 Solar Radius
10-2 Solar Radius
10-3 Solar Radius
30,000
increasing
temperature
10²
Solar Radi
B Centauri
Spica
10 M Sun
MAIN
Sirius B
Bellatrix
Lifetime
10 yrs
B
m
Rigel
Deneb
6 Msun
Achernar
SEQUENCE
M Sun
Vega
Lifetime
10⁹ yrs
WHITE
SUPERGIANTS
103 Solar Radi
Sirius
DWARFS
Procyon B
Lifetime
1010 yrs
Altair
A
Canopus
Sun
Polaris
Arcturus
Procyon
$1.5 Mean
Lifetime
1011 yrs
T Ceti
GIANTS
x Centauri A
Mexin
Pollux
Centauri B
Eridani
F G K
10,000
6,000
surface temperature (Kelvin)
Aldebaran
Barnard's Star
61 Cygni A
61 Cygni B
Lacaille 9352
0.3 Msun
Betelgeuse
Antares
Wolf 359
Proxima Centauri
DX Cancri
M
(It may help you to know that 1 Lsun is 3.8 x 1026 Watts. Use 3.1415 for Pi.)
Gliese 725 A
Gliese 725 B
0.1 Msun
Ross 128
The physics of thermally radiating gases relates the luminosity (L), temperature (T) and radius (r) of a star.
You have identified the relevant equation in the previous questions. Note "sigma" is the Stefan-Boltzman constant, 5.67 x 10-8 Watts/m²K4.
3,000
decreasing
temperature
From the HR diagram above, we could determine that the star Barnard's Star has a temperature 3.03E+3 K and a luminosity of 4.79E-3 Lsun. What then is its radius measured in meters?
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