Star Forming Region Known As N90 Afmeting:A3: 30 x 40 cm Howling winds send the storming Frame:Unframed Howling winds send the storming glass sideways at 5 MIRI sees a distinct difference in colour between the dust in the galaxies versus the shock waves between the interacting galaxies The high energy radiation blazing out from the hot young stars in N90 is eroding the outer portions of the nebula from the inside Because N90 is located far from the central body of the Small Magellanic Cloud