The following table is adapted from the one given by Eddington for the relation between distance,
, from the center, density
, and temperature
, for a typical giant star of Class
, effective temperature 6500°. The distance from the center is expressed in terms of the solar radius, the density in grams per cubic centimeter, and the temperature in absolute units. The last entry in the first column represents the total radius of the star.
| 0 | 0.1085 | 6,590,000° | 4 | 0.0010 | 1,380,000° |
| 1 | 0.0678 | 5,640,000 | 5 | 0.00015 | 730,000 |
| 2 | 0.0215 | 3,840,000 | 6 | 0.0000093 | 290,000 |
| 3 | 0.0050 | 2,370,000 | 6.9 | 0.000000 | ...... |