  Accurate modeling of astrophysical jets is critical for understanding
accretion systems and their impact on the interstellar medium. While
astronomical observations can validate models, they have limitations.
Controlled laboratory experiments offer a complementary approach for
qualitative and quantitative demonstration. Laser experiments offer a
complementary approach. This article introduces a new platform on the OMEGA
laser facility for high-velocity (1500 km/s), high-aspect-ratio ($\sim$36) jet
creation with strong cylindrical symmetry. This platform s capabilities bridge
observational gaps, enabling controlled initial conditions and direct
measurements
