a) Calculate the luminosity of a star at a distance of 10 light-years (ly) with brightness 2500 W/m? b) How does this compare to the luminosity of the Sun? c) What would the brightness of this star be at a distance of 100 ly?

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Problem 3. Brightness and Luminosity
31
The brightness or flux intensity of a star at an observer's location may be
determined by measuring the rate at which its light enters the aperture of an
observing instrument (this is referred to as photometry). We will call this "" (with
units [Energy/time/Area] or [Watts/Area]). Imagine a sphere of radius, d (labeled
"p" in the figure below), equal to the star's distance from the observer's location,
at which the star is at the center (see the figure below). ALL of the star's light
passes through the surface area of this sphere but only a small fraction passes
through the instrument aperture. The fraction of the star's rate of light energy
emission measured by the instrument is proportional to the ratio of the instrument
aperture area (A) to the area of the sphere (A§). If L is the rate at which light
energy is emitted from the star in all directions (the Luminosity) then
ALL
As
b =
A1
L.
As
4nd
>
CVX.csv
Show all
11:49 PM
e Type here to search
3/4/2021
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心)
||
II
Transcribed Image Text:E A X M Inbo b Last Class N Netf + Prob Logir | X Math M Inbo Good #3 Mail y! CVX ET Wha 4 Grou EHL 4 fre G neve docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit M AST1002001FALL2017PS7 ☆ A Request edit access Share File Edit View Tools Help Problem 3. Brightness and Luminosity 31 The brightness or flux intensity of a star at an observer's location may be determined by measuring the rate at which its light enters the aperture of an observing instrument (this is referred to as photometry). We will call this "" (with units [Energy/time/Area] or [Watts/Area]). Imagine a sphere of radius, d (labeled "p" in the figure below), equal to the star's distance from the observer's location, at which the star is at the center (see the figure below). ALL of the star's light passes through the surface area of this sphere but only a small fraction passes through the instrument aperture. The fraction of the star's rate of light energy emission measured by the instrument is proportional to the ratio of the instrument aperture area (A) to the area of the sphere (A§). If L is the rate at which light energy is emitted from the star in all directions (the Luminosity) then ALL As b = A1 L. As 4nd > CVX.csv Show all 11:49 PM e Type here to search 3/4/2021 + 心) || II
E A X
X Math
M Inbo
b Last
Class
N Netf
+
Prob
Logir
M Inbo
4
Good
#3
Grou
Mail
y! CVX
EHL 4 fre
ET Wha
G neve
docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit
M
AST1002001FALL2017PS7 ☆ A
Request edit access
Share
File Edit View Tools Help
31
Area of sphere = 4rr?
Area of instrument
aperture
aperture = A,
Star
a) Calculate the luminosity of a star at a distance of 10 light-years (ly) with
brightness 2500 W/m²
b) How does this compare to the luminosity of the Sun?
c) What would the brightness of this star be at a distance of 100 ly?
11:49 PM
e Type here to search
3/4/2021
+
(8)
Transcribed Image Text:E A X X Math M Inbo b Last Class N Netf + Prob Logir M Inbo 4 Good #3 Grou Mail y! CVX EHL 4 fre ET Wha G neve docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit M AST1002001FALL2017PS7 ☆ A Request edit access Share File Edit View Tools Help 31 Area of sphere = 4rr? Area of instrument aperture aperture = A, Star a) Calculate the luminosity of a star at a distance of 10 light-years (ly) with brightness 2500 W/m² b) How does this compare to the luminosity of the Sun? c) What would the brightness of this star be at a distance of 100 ly? 11:49 PM e Type here to search 3/4/2021 + (8)
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