The Hubble Space Telescope recently captured an image of the spiral galaxy NGC 3596, located 90 million light-years away in the constellation Leo.
NGC 3596 appears almost face-on from Earth, showcasing its neatly wound spiral arms with concentrations of stars, gas, and dust indicating active star formation.
The formation of spiral arms in galaxies has puzzled astronomers, with varying structures and the 'winding problem' historically challenging to explain.
Recent research suggests that spiral arms represent patterns of high-density and low-density areas rather than physical structures, with materials moving through them akin to cars in a traffic jam.