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Chamaeleon Dark Nebulas

November 19, 2025

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Selected image source ↗ APOD published November 19, 2025. Credit: Xinran Li & Houbo Zhao. A publication-date match, not a photo taken on your date. Independent of NASA.

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Chamaeleon Dark Nebulas

Original APOD · November 19, 2025 ↗

Read the original APOD for the astronomer’s explanation and full image credits. Its text is preserved in the archive as published.

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Sometimes the dark dust of interstellar space has an angular elegance. Such is the case toward the far-south constellation of Chamaeleon. Normally too faint to see, dark dust is best known for blocking visible light from stars and galaxies behind it. In this 11.4-hour exposure, however, the dust is seen mostly in light of its own, with its strong red and near-infrared colors creating a brown hue. Contrastingly blue, a bright star Beta Chamaeleontis is visible on the upper right of the V, with the dust that surrounds it preferentially reflecting blue light from its primarily blue-white color. All of the pictured stars and dust occur in our own Milky Way Galaxy with one notable exception: a white spot just below Beta Chamaeleontis is the galaxy IC 3104, which lies far in the distance. Interstellar dust is mostly created in the cool atmospheres of giant stars and dispersed into space by stellar light, stellar winds, and stellar explosions such as supernovas.

Image credit: Xinran Li & Houbo Zhao

Explore November 19 in other years · 31 APOD entries, 1995–2025

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