#(g_e)/(g_m)=6.05#
The data given in the question is way out. The mass of the moon is 1/81.3 of the earth so I'll work through with that.
I'll also use the radius of the moon to be 0.273 x the radius of the earth.
We'll compare an object of mass #m# on the surface of the earth with an object of mass #m# on the surface of the moon.
Newton says that the force of attraction between 2 objects #M# and #m# is:
#F=(GmM)/(R^(2)#
For this problem:
#F_e# = force of attraction on the earth
#F_m# = force of attraction on the moon
#R_e# = radius earth
#R_m# = radius moon
#m# = mass object
So:
#F_e=(GmM_e)/(R_e^(2)# Eqn #color(red)((1))#
#F_m=(GmM_m)/(R_m^(2))# Eqn#color(red)((2))#
We know that:
#R_m=0.273R_e#
and:
#M_m=M_e/81.3#
So we can substitute these values into #color(red)((2))# #rArr#
#F_m=(Gm[(M_e)/(81.3)])/((0.273R_e)^(2))#
#F_m=(Gm[(M_e)/(81.3)])/(0.0745R_e^(2))# Eqn #color(red)((3))#
Now divide #color(red)((1))# by #color(red)((3))# #rArr#
#(F_e)/(F_m)=(GmM_e)/(R_e^(2))xx(0.0745R_e^(2))/(Gm[[M_e)/(81.3)]#
This cancels down to:
#(F_e)/(F_m)=(0.0745)/((1)/(81.3))=6.05#
Since #F=ma#:
#(mg_e)/(mg_m)=6.05#
So:
#(g_e)/(g_m)=6.05#
This agrees with the generally accepted value of the acceleration due to gravity of the moon being about 1/6 of that of the earth.
You can substitute the values given in the question if you want to but I would check their source.