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 ^ { -1 } 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 ~ { } M _ { \odot } 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 .