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
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).