Use the Hertzsprung-Russell diagram and temperature and luminosity data to identify each star.

fgravity=10x10=100n case 1

fgravity=30x20=600n case 2

6 times more

force is mass*acceleration.

we have a very small mass: 11.4*0.001 kg

if we want 0.035n of force, we need an acceleration:

0.035 = 11.4*0.001*a

a = 0.035/(11.4*0.001) m/s^2