In: Advanced Math
the table below lists information for seven Cepheid variables where ‘Period’ is the pulsation period of the star, and ?/?⊙ is the luminosity in solar units.
| 
 Period (days)  | 
 L/L⨀  | 
| 
 4.5  | 
 835  | 
| 
 7.2  | 
 1418  | 
| 
 15.0  | 
 3761  | 
| 
 29.3  | 
 8176  | 
| 
 51.6  | 
 16623  | 
| 
 82.8  | 
 28220  | 
| 
 172.5  | 
 75140  | 
a) Plot the PL relation for these stars using the logarithms of the values in the table (that is, ???(?) vs ???(?/?⊙)) and extract the slope and y-intercept of the relation the data define
Let's write the given data in logarithmic values,where
'
represents luminosity in solar units| log(P) | log(L/L ) | 
|---|---|
| 0.6532 | 2.9217 | 
| 0.8573 | 3.1517 | 
| 1.1761 | 3.5753 | 
| 1.4668 | 3.9125 | 
| 1.7126 | 4.2207 | 
| 1.9180 | 4.4506 | 
| 2.2368 | 4.8759 | 
slope of the equation (m) = (4.8759-2.9217)/(2.2368-0.6532) = 1.234
So, the equation be of the form y=mx+c,c:y-intercept
Then the equation is : log(L/L
)
= mlog(P) + C
log(L/L
)
= 1.234*log(P) + C;
Substitute any data from above table to get y-intercept;
3.9125
= 1.234*1.4668+C;
C
= 2.1025
Therefore, the y-intercept is the luminosity of the star
at start(i.e., log(P)=0 
P=1).So, on the first day of period the luminosity =
[(10)2.1025] = 126.62 solar units.And the luminosity is
increased by [(10)1.234 = 17.14 solar units] for a
period of one day(this relation is from the slope).