  This study focuses on determining the characteristics of the young open
cluster NGC 6383. To achieve this, the HDBSCAN clustering algorithm is utilized
to identify potential cluster members based on proper motions and parallaxes
from Gaia Data Release 3. Various parameters of NGC 6383, such as tidal radius,
core radius, distance through parallax and isochrone-fitting, proper motion,
age, metallicity, and relevant others, are assessed. To perform this analysis,
we utilize an extension of Hamiltonian Monte Carlo, the No-U-Turn Sampler. The
results of this analysis point out that NGC 6383 is a very young open cluster
$(\sim 1 - 4~\mathrm{Myr})$, with a distance of $\sim 1.1~\mathrm{kpc}$.
