An astrophysicist compiles a dataset of main-sequence stars in a nearby stellar cluster to study stellar evolution.
| Mass of star (relative to the Sun) | Main-sequence lifetime (years) |
|---|---|
| 60.060.060.0 | 3.0×1063.0 \times 10^63.0×106 |
| 10.010.010.0 | 3.0×1073.0 \times 10^73.0×107 |
| 2.02.02.0 | 1.2×1091.2 \times 10^91.2×109 |
| 1.01.01.0 (the Sun) | 1.0×10101.0 \times 10^{10}1.0×1010 |
| 0.70.70.7 | 2.0×10102.0 \times 10^{10}2.0×1010 |
| 0.20.20.2 | 1.0×10121.0 \times 10^{12}1.0×1012 |
State how the main-sequence lifetime of a star changes as the mass of the star increases.