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A couple of dozen bright stars in the foreground, mostly blue-white but some red-orange. Red-orange gas and dust in the background along the bottom half of the image and in the top-right corner. Thousands more stars in the background, scattered throughout.

Cloud-Filled, Starry Open Cluster BSDL 2757

Bright, blue-white stars of the open cluster BSDL 2757 pierce through the rusty-red tones of gas and dust clouds in this Hubble Space Telescope image. Hubble captured the scene as part of a study looking at how dust in the Large Magellanic Cloud obscures ultraviolet light in four different star-forming regions of this nearby, irregular galaxy. The researchers studied growing, early-stage stars that are still accumulating mass from the clouds that envelop them. As gas and dust spirals toward a budding, young star, it releases ultraviolet light. By analyzing how this light interacts with dust, astronomers can better understand the dust’s properties in different environments. The colors blue, green, and orange in this image represent their respective colors in the visible light spectrum. The color red represents light in the near-infrared part of the spectrum.

Image Credit: NASA, ESA, and L. Bianchi (Johns Hopkins University); Processing: G. Kober (NASA/Catholic University of America)
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