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The\u00a0spiral galaxy\u00a0NGC 3596 is on display in this NASA\/ESA Hubble Space Telescope\u00a0Picture of the Week, which incorporates six different\u00a0wavelengths\u00a0of light. NGC 3596 is situated 90 million light-years from Earth in the constellation\u00a0Leo. The galaxy was discovered in 1784 by astronomer William Herschel, the namesake of ESA\u2019s\u00a0Herschel Space Observatory.\u00a0<\/p>\n
NGC 3596 appears almost perfectly face-on when viewed from Earth, showcasing the galaxy\u2019s neatly wound spiral arms. The bright arms mark where the galaxy\u2019s\u00a0stars, gas and dust are concentrated. Star formation is also most active in a galaxy\u2019s spiral arms, as shown by the brilliant pink star-forming regions and young blue stars tracing NGC 3596\u2019s arms in this image.<\/p>\n
What causes these spiral arms to form? It\u2019s a surprisingly difficult question to answer, partly because of the remarkable diversity of spiral galaxies. Some have\u00a0clear spiral arms, while others have\u00a0patchy, feathery arms. Some have\u00a0prominent bars across their centres, while others have\u00a0compact, circular nuclei. Some have\u00a0close neighbours, while others are\u00a0isolated.<\/p>\n
Early ideas of how spiral arms formed were stumped by what\u2019s called the \u2018winding problem\u2019. If a galaxy\u2019s spiral arms are coherent structures, the arms would be wound tighter and tighter as the galaxy spins, until the arms are no longer visible. Now, researchers believe that spiral arms represent a pattern of high-density and low-density areas rather than a physical structure. As stars, gas and dust orbit within a galaxy\u2019s disc, they pass in and out of the spiral arms. Much like cars moving through a traffic jam, these materials slow down and bunch up as they enter a spiral arm, before emerging and continuing their journey through the galaxy.<\/p>\n
[Image Description:<\/i>\u00a0A spiral galaxy viewed face-on, with a slightly oval-shaped disc. The centre is a bright white spot surrounded by a golden glow. Two spiral arms extend out from the centre, wrapping around the galaxy and broadening out to form the thick outer edge of the disc. Thin reddish strands of dust and bright pink spots follow the arms through the disc. Faint strands of stars extend from the arms\u2019 tips, out beyond the disc.]<\/p>\n<\/p><\/div>\n<\/p><\/div>\n