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This study reports the first comprehensive astrometric, photometric andkinematical analysis of four newly discovered open clusters; namely QC1, QC2,QC3, and QC4, using astrometric and photometric data from the most recent GaiaEDR3 for G<17 mag. Utilizing the ASteCA code, we identified the most probable(P>=50%) star candidates and found the numbers of star members (N) to be 118(QC1), 142(QC2), 210 (QC3), and 110 (QC4). By fitting King's density profile tothe cluster's RDPs, we found the internal structural parameters of each clustersuch as the cluster radii that are in the range 7.00 to 11.00arcmin. For eachcluster we constructed the CMD and by fitting them with suitable isochrones wefound that the metallicity range is (0.0152-0.0199) which is in line with theSolar value, the logarithmic age (in yrs) range between 6.987 and 8.858. Thedistances derived from CMD are 1674+/-41, 1927+/-44, 1889+/-43,and 1611+/-40(pc) for QC1, QC2, QC3, and QC4, respectively, and they are in good agreementup to 85% with the values obtained from the astrometric data. In addition, fromthe MLR of the clusters, we obtained a total mass, M_C in Solar units, of 158,177, 232, and 182 and an absolute magnitude MG(mag)of 4.33, 3.80, 4.25, and4.10 for QC1, QC2, QC3, and QC4, respectively. The dynamical analysis andevolution parameters of the cluster members indicated that all the fourclusters are dynamically relaxed;except QC1 which has an evolution parametertau=0.82 that indicates a dynamical activity within the cluster. From thekinematical analysis of the cluster data, we computed the space velocity, thecoordinates of the apex point (A,D) using the AD-diagram method, as well as theSolar elements (S_sun, l_A, b_A,alpha_A,delta_A)

A comprehensive photometric and kinematical characteristic of the newly discovered QCs clusters with Gaia EDR3