  K3-35 is an extremely young bipolar planetary nebula that contains a
precessing bipolar jet and a small (radius 80 AU) water maser equatorial ring.
We have obtained VISIR- VLT images of K 3-35 in the PAH1 ({\lambda}=8.6
{\mu}m), [S iv] ({\lambda}=10.6 {\mu}m), and SiC ({\lambda}=11.85 {\mu}m)
filters to analize the mid-IR morphology and the temperature structure of its
dust emission. The images show the innermost nebular regions undetected at
optical wavelegths and the precessing bipolar jets. The temperature map shows
variations in the temperature in the equatorial zone and in regions associated
to its jets.
