Oct 20, 2025
Small Magellanic Cloud
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Small Magellanic Cloud
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Located in the Small Magellanic Cloud, NGC 346 is a region of star formation seen here in Hubble Space Telescope visible light data (red, green, and blue) and Chandra observatory X-rays (pinkish purple).
The large, neon-pink X-ray cloud hangs in the upper right, representing the high-energy environment of stars roughly 1 to 3 million years old. The dark blue background is scattered with orange and white stellar specks and hazy streaks of gas and dust.
NGC 346 is home to more than 2,500 newborn stars. The cluster’s most massive stars, which are many times more massive than our Sun, blaze with an intense blue light in this image.
Credit: X-ray: NASA/CXC/SAO; Optical: ESA/Hubble and NASA, A. Nota, P. Massey, E. Sabbi, C. Murray, M. Zamani (ESA/Hubble); Image Processing: NASA/CXC/SAO/L. Frattare.
A Dwarf Galaxy, the Small Magellanic Cloud ©
A "necklace" of nebulae in the SMC // Kartik Atre
Milky Way at York, Western Australia
Nikon d810a - 50mm - ISO 6400 - f/2.5 - Foreground: 7 x 30 seconds - Sky: 35 x 30 seconds - iOptron SkyTracker - Hoya Red Intensifier filter
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N81: Starbirth in the SMC - July 27th, 1998.
"A very young star cluster had been discovered in a neighboring galaxy. The stars found in this cluster, dubbed N81, are so young and massive that they furiously eject matter and light up the surrounding nebula. The ejected stellar winds combine and interact to sculpt beautiful and complex structures. Visible near the center of the above representative-colour picture are two of N81's brightest stars. Just above them lies a dark knot of dust and gas where these massive stars likely originated. The home galaxy of this stellar nursery is the Small Magellanic Cloud (SMC) located about 200,000 light-years away."
Small Magellanic Cloud
Trans flag colorpicked from the Small Magellanic Cloud
