Near-infrared and optical imaging of HD32297 indicate that it has an edge-on debris disk , similar to \beta Pic .
I present high resolution optical spectra of the Na i doublet toward HD32297 and stars in close angular proximity .
A circumstellar absorption component is clearly observed toward HD32297 at the stellar radial velocity , which is not observed toward any of its neighbors , including the nearest only 0 \farcm 9 away .
An interstellar component is detected in all stars > 90 pc , including HD32297 , likely due to the interstellar material at the boundary of the Local Bubble .
Radial velocity measurements of the nearest neighbors , BD+07 777s and BD+07 778 , indicate that they are unlikely to be physically associated with HD32297 .
The measured circumstellar column density around HD32997 , \log N _ { NaI } \sim 11.4 , is the strongest Na i absorption measured toward any nearby main sequence debris disk , even the prototypical edge-on debris disk , \beta Pic .
Assuming that the morphology and abundances of the gas component around HD32297 are similar to \beta Pic , I estimate an upper limit to the gas mass in the circumstellar disk surrounding HD32297 of \sim 0.3 M _ { \oplus } .