Initially, it seems that the face-value interpretation of the question can have no answer. The history tag, though, poses a definite problem, which enables us to think about the problem slightly more in depth. My first thought was as follows:
Historically, the metre was defined as one ten-millionth of a quarter of the circumference of the earth, although our calculations were slightly off. Similarly, the second was historically defined as one $86,400$th of a solar day which is slightly longer than the sidereal day (the period of the rotation of the earth - different by one day every year because after the earth has completed a revolution it is back in the same position but having completed an 'extra' rotation).
Thus if (which is a big if, given the barriers in language and culture), fblthp's countrypeople have arrived at their definitions of length and time units in similar ways to us, it implies that their length and time units are in the same relation to the circumference and period of rotation of their planet as our own. This does not however, narrow down the possibilities very much as the length of the day of a planet is highly variable. Specifically, if this were the case, it would mean that if we let $G$ be the gravitational constant, $M$ the mass of the planet, $r_p$ its radius, $g$ the gravity at its surface, $C$ the circumference of the earth, $C_p$ the circumference of their planet, $D$ the length of our day, $D_p$ the length of their day, $m_p$ their unit of length, and $s_p$ their unit of time, we have:
$$g=\frac{GM}{r_p^2}=\frac{10m_p}{s_p^2}=\frac{10\left(\frac{C_p}{C}\right)}{\left(\frac{D_p}{D}\right)^2}\frac{m}{s^2}$$
$$\therefore D_p=D\sqrt{\frac{20\pi r_p^3}{GMC}}$$
Which is an expression for the length of their day in terms of the radius of their planet and its mass. Unfortunately, there's very little physical connection (as far as I'm aware) between the period of rotation of a planet and its radius and mass, which enables us to deduce very little.
However, an even bleaker prospect opens up for fblthp if we step back even further historically:
The original historical connection between the definition of metre and second was that the metre was defined as roughly the length of a pendulum that swings from one side to the other in one second. This doesn't add any new information though, as it's due to the fact that $g\approx\pi^2$, since the period of a pendulum of length $L$ is roughly:
$$T\approx2\pi\sqrt{\frac{L}{g}}$$
Put another way, no matter what planet you are on, and no matter how you have defined your time unit, if you define your length unit (like we roughly did) as the length of a pendulum with a period of $2$ time units, then $g$ the surface gravity on that planet will be just under $10$ (i.e. $\approx\pi^2$ length units per time units squared). Because of this, if fblthp's society has arrived at their length and time units similarly to how we did, then knowing the surface gravity of the planet in their units conveys precisely zero information about the planet itself.
The only problem with this reasoning of course, is that there is no a priori reason that fblthp's society should define their units the same way as us. However, the OP has indicated that this is the intended solution to the puzzle.
As a more general reflection on this type of problem:
Thinking about how different societies could communicate about physical constants is interesting. Of course, the only such constants whose numerical values could be communicated straightforwardly are the dimensionless constants, such as the fine-structure constant. All dimensional quantities have to be described in proportion to some other agreed quantity (e.g. here, also see here), which of course becomes a problem of chicken-and-egg. Without doing something like telling us how many Planck lengths are in the radius of their earth, we cannot learn anything specific about their units.
This would make the situation no longer a puzzle though. For what it's worth, the trick of recognizing the historical connection between metre and second was a good one, and therefore gripes aside I say 'good puzzle!'.