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Brandy Irie

@brandyirie.bsky.social

28 Followers  |  22 Following  |  6 Posts  |  Joined: 13.11.2024  |  1.4077

Latest posts by brandyirie.bsky.social on Bluesky

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Trump’s neofascism is here now. Here are 10 things you can do to resist | Robert Reich America has deep problems, which is why we can’t give up. Protect the vulnerable, organize boycotts and keep fighting

www.theguardian.com/commentisfre...

28.01.2025 21:43 — 👍 0    🔁 0    💬 0    📌 0
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Dr. Poo!

11.01.2025 08:24 — 👍 0    🔁 0    💬 0    📌 0
Post image 11.01.2025 08:24 — 👍 1    🔁 1    💬 0    📌 0

Thorian? That you?

11.01.2025 07:42 — 👍 0    🔁 0    💬 0    📌 0
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Hundreds of Mexican firefighters have arrived in Southern California to help combat the wildfires.

Thank you, Mexico🇺🇸🇲🇽

11.01.2025 02:24 — 👍 68851    🔁 11816    💬 1787    📌 934
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.

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.

High resolution image of a heavy star.
🔭 🧪

10.01.2025 17:37 — 👍 5826    🔁 500    💬 62    📌 21

Skyrim, Morrowind, Resident Evil, City of Heros, Super Mario Bros, Pitfall... I think about them all of the time.

11.01.2025 07:39 — 👍 0    🔁 0    💬 0    📌 0

World of Warcraft. I still have life long friends from that game.

11.01.2025 07:37 — 👍 7    🔁 0    💬 1    📌 0

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