  This paper presents an investigation on the four open clusters Czernik 14,
Haffner 14, Haffner 17 and King 10 located near the Perseus arm of Milky Way
Galaxy using Gaia DR2, 2MASS, WISE, APASS and Pan-STARRS1 data sets. We find
normal interstellar extinction in twelve photometric bands for these clusters.
Likely cluster members are identified as 225, 353, 350 and 395 for Czernik 14,
Haffner 14, Haffner 17 and King 10, respectively by using Gaia DR2 proper
motion data. Radii are determined as 3.5, 3.7, 6.2 and 5.7 arcmin for Czernik
14, Haffner 14, Haffner 17 and King 10 respectively. Mean proper motions in RA
and DEC are estimated as (-0.42 \pm 0.02, -0.38 \pm 0.01), (-1.82 \pm 0.009,
1.73 \pm 0.008), (-1.17 \pm 0.007, 1.88 \pm 0.006) and (-2.75 \pm 0.008, -2.04
\pm 0.006) mas/yr for Czernik 14, Haffner 14, Haffner 17 and King 10,
respectively. The comparison of observed CMDs with solar metallicity isochrones
leads to an age of 570 \pm 60, 320 \pm 35, 90 \pm 10 and 45 \pm 5 Myr for these
clusters. The distances 2.9 \pm 0.1, 4.8 \pm 0.4, 3.6 \pm 0.1 and 3.8 \pm 0.1
kpc determined using parallax are comparable with the values derived by the
isochrone fitting method. Mass function slopes are found to be in good
agreement with the Salpeter value. The total masses are derived as 348, 595,
763 and 1088 solar mass for the clusters Czernik 14, Haffner 14, Haffner 17 and
King 10, respectively. Evidence for the existence of mass-segregation effect is
observed in each cluster. Using the Galactic potential model, Galactic orbits
are derived for the clusters. The present study indicates that all clusters
under study fallow a circular path around the Galactic center.
