We report a trigonometric parallax measurement with the Very Long Baseline Array for the water maser in the distant high-mass star-forming region G75.30+1.32 .
This source has a heliocentric distance of 9.25 ^ { +0.45 } _ { -0.40 } kpc , which places it in the Outer arm in the first Galactic quadrant .
It lies 200 pc above the Galactic plane and is associated with a substantial H i enhancement at the border of a large molecular cloud .
At a Galactocentric radius of 10.7 kpc , G75.30+1.32 is in a region of the Galaxy where the disk is significantly warped toward the North Galactic Pole .
While the star-forming region has an instantaneous Galactic orbit that is nearly circular , it displays a significant motion of 18 km s ^ { -1 } toward the Galactic plane .
The present results , when combined with two previous maser studies in the Outer arm , yield a pitch angle of about 12 \arcdeg for a large section of the arm extending from the first quadrant to the third .