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Face-on spiral galaxy. Bright-white core surrounded by spiral arms. Areas of reddish-pink star formation regions dot the spiral arms which appear like a light-bluish haze. Dark rusty-brown dust lanes follow the curves of the spiral arms.

Face-On Spiral Galaxy NGC 3982

Though the universe is chock full of spiral-shaped galaxies, no two look exactly the same. This face-on spiral galaxy, called NGC 3982, is striking for its rich tapestry of star birth, along with its winding arms. The arms are lined with pink star-forming regions of glowing hydrogen, newborn blue star clusters, and obscuring dust lanes that provide the raw material for future generations of stars. The bright nucleus is home to an older population of stars, which grow ever more densely packed toward the center. NGC 3982 is located about 68 million light-years away in the constellation Ursa Major. The galaxy spans about 30,000 light-years, one-third of the size of our Milky Way galaxy. The rich color range comes from the fact that the galaxy was photographed invisible and near-infrared light.

Image Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: A. Riess (STScI)
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