I imagine your lecturer was referring to the
Planck length, though it's closer to 10^-35 meters. The Planck length is thought to be about the length scale at which the current best theory of gravity,
general relativity, would probably become totally inaccurate and we would need a more accurate theory of
quantum gravity to replace it (see my recent post
here discussing how the Big Bang can be derived from using general relativity to project the observed expansion of the universe backwards). However, I don't think it's accurate to say that quantum gravity becomes important when the universe is the size of a Planck length--probably it would be more like when the
density of the universe was high enough to reach the "Planck density", or
Planck mass per Planck volume (Planck length cubed), which would mean the observable universe as a whole could have been significantly larger in size than one Planck length. That's just a rough guess though, quantum gravity effects might start to become important a little before it reached that density, for example I found
this page from physicist [URL='https://www.physicsforums.com/insights/author/john-baez/']John Baez[/url] which says:
Anyway, what are the results? What does the currently popular theory of loop quantum cosmology imply?
In a nutshell: if you follow the history of the Universe back in time, it looks almost exactly like what ordinary cosmology predicts until the density reaches about 1/100 of the Planck density.
Loop quantum gravity is one attempt to develop a theory of quantum gravity, the other major one being string theory.
Let's do a back-of-the-envelope style rough calculation. According to
this, the current density of all forms of mass and energy (and energy can be treated as a form of mass by E=mc^2) is about 0.85 * 10^-26 kg/m^3. The Planck density is around 5*10^96 kg/m^3. So to squeeze the observable universe to the Planck density, you'd have to divide its volume by about 6*10^122. Since the volume of a spherical region is the cube of its radius, we have to take the cube root of this to find how much to divide the radius, or 8*10^40. The radius of the observable universe is thought to be about 47 billion light years which works out to about 4*10^25 meters, so dividing this by 8*10^40 implies the radius of the observable universe would be about 5*10^-16 meters if it was squeezed to the Planck density. That's fairly close to the size of a proton, about 9*10^-16 meters. So the observable universe would have been small, but still many orders of magnitude larger than the Planck length.