To solve this problem it is necessary to apply the concepts related to hydrostatic pressure or pressure due to a fluid.
Mathematically this pressure is given under the formula
[tex]P_h = \rho g h[/tex]
Where,
[tex]\rho[/tex] = Density
h = Height
g = Gravitational acceleration
Rearranging in terms of g
[tex]g = \frac{P_h}{\rho h}[/tex]
our values are given as
[tex]P_h = 1.1 atm (\frac{101325Pa}{1atm}) = 111457.5Pa[/tex]
[tex]\rho = 1000kg/m^3[/tex]
[tex]h = 12.3m[/tex]
Replacing we have
[tex]g = \frac{111457.5}{(1000)(12.3)}[/tex]
[tex]g = 9.061m/s^2[/tex]
Therefore the gravitational acceleration on the planet's surface is [tex]9.061m/s^2[/tex] (Almost the gravity of the Earth)