MoonyMood
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moonymood.bsky.social
MoonyMood
@moonymood.bsky.social
22 followers 25 following 2 posts
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chimeracoder.bsky.social
RT if you also wish ill upon JK Rowling.
August 21, 2025 at 1:43 PM
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enrich12.bsky.social
As American as apple pie. 😳
July 14, 2025 at 11:17 AM
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upandoutcomic.bsky.social
gottem
January 16, 2025 at 5:27 PM
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moon1over.bsky.social
📷 Nikola Petanjko
January 23, 2025 at 1:12 PM
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moon1over.bsky.social
January 15, 2025 at 4:12 AM
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stuntmaenbob.bsky.social
✨ #pixelart
Pixel art landscape (+ outer space) - front: trees and rocks. Middle: lake, trees and some mountains. Background: planets and stars in front of a dark sky. Purple and pink tones.
January 13, 2025 at 6:36 AM
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cathelizabeth.bsky.social
Our beautiful Moon
Waxing Gibbous 98% illuminated
Sunday 12th January 2025
SeeStar S50
January 12, 2025 at 8:28 PM
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bruib.bsky.social
Guider.
#art
A kitty made of stars sits on a wire in front of a purple background
December 25, 2024 at 12:45 AM
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quantumkat.bsky.social
Flaming Star Nebula (IC 405)
A runaway star, ejected from its original system, traveling alone through space and illuminating a gas cloud spanning 5 light-years across.

📸 Capture Details:
Telescope: Newton 130/900
Camera: Sony A7S
@kat-astro-bot.bsky.social pleasing perform astrometry.
Astrophotography image of the Flaming Star Nebula (IC 405), a combination of emission and reflection nebula located in the constellation Auriga.
January 10, 2025 at 12:50 PM
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moon1over.bsky.social
January 10, 2025 at 12:42 AM
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jwstfeed.bsky.social
High resolution image of a heavy star.
🔭 🧪
The luminous, hot star Wolf-Rayet 124 (WR 124) is prominent at the centre of the James Webb Space Telescope’s composite image combining near-infrared and mid-infrared wavelengths of light. The star displays the characteristic diffraction spikes of Webb’s Near-infrared Camera (NIRCam), caused by the physical structure of the telescope itself. NIRCam effectively balances the brightness of the star with the fainter gas and dust surrounding it, while Webb’s Mid-Infrared Instrument (MIRI) reveals the nebula’s structure. Background stars and galaxies populate the field of view and peek through the nebula of gas and dust that has been ejected from the ageing massive star. A history of the star’s past episodes of mass loss can be read in the nebula’s structure. Rather than smooth shells, the nebula is formed from random, asymmetric ejections. Bright clumps of gas and dust appear like tadpoles swimming toward the star, their tails streaming out behind them, blown back by the stellar wind.
January 10, 2025 at 5:37 PM
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markhamillofficial.bsky.social
#EmbarrassmentInChief 🤮
January 10, 2025 at 10:37 PM