This paper presents an analysis of the first 2MASS (The Two Micron All Sky
Survey) sampler data as observed at lower Galactic latitude in our Galaxy.
These new near-infrared data provide insight into the structure of the thin
disk of our Galaxy. The interpretation of star counts and color distributi
ons of stars in the near-infrared with the synthetic stellar population mod
el, gives strong evidence that the Galactic thin disk density scale length,
h(R), is rather short (2.7 +/- 0.1 kpc).