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@mcbishop.bsky.social

39 Followers  |  41 Following  |  2 Posts  |  Joined: 16.11.2024
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Post image 17.01.2025 05:22 โ€” ๐Ÿ‘ 45    ๐Ÿ” 8    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0

Who else is really looking forward to not watching the Inauguration?

๐Ÿ‘€ ๐Ÿ‘Ž

12.01.2025 21:40 โ€” ๐Ÿ‘ 86068    ๐Ÿ” 12163    ๐Ÿ’ฌ 6754    ๐Ÿ“Œ 1025

The enemy of my enemy is still my enemy

12.01.2025 03:25 โ€” ๐Ÿ‘ 3    ๐Ÿ” 0    ๐Ÿ’ฌ 1    ๐Ÿ“Œ 0

I have whiskey and weed with arms reach.

12.01.2025 01:07 โ€” ๐Ÿ‘ 2    ๐Ÿ” 0    ๐Ÿ’ฌ 2    ๐Ÿ“Œ 0
Post image

So did I, Tris. I am beyond disappointed. So much So that I find myself questioning the rule of law in this country. Is there a rule of law still, TBH IDK. Based on what they have gotten away with I have my doubts.

Just one example of many I could use...

11.01.2025 23:28 โ€” ๐Ÿ‘ 309    ๐Ÿ” 71    ๐Ÿ’ฌ 13    ๐Ÿ“Œ 2
The luminous, hot star Wolf-Rayet 124 (WR 124) is prominent at the centre of the James Webb Space Telescopeโ€™s composite image combining near-infrared and mid-infrared wavelengths of light. The star displays the characteristic diffraction spikes of Webbโ€™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 Webbโ€™s Mid-Infrared Instrument (MIRI) reveals the nebulaโ€™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 starโ€™s past episodes of mass loss can be read in the nebulaโ€™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 Telescopeโ€™s composite image combining near-infrared and mid-infrared wavelengths of light. The star displays the characteristic diffraction spikes of Webbโ€™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 Webbโ€™s Mid-Infrared Instrument (MIRI) reveals the nebulaโ€™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 starโ€™s past episodes of mass loss can be read in the nebulaโ€™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.
๐Ÿ”ญ ๐Ÿงช

10.01.2025 17:37 โ€” ๐Ÿ‘ 5801    ๐Ÿ” 498    ๐Ÿ’ฌ 62    ๐Ÿ“Œ 21
Post image 20.11.2024 13:46 โ€” ๐Ÿ‘ 157    ๐Ÿ” 23    ๐Ÿ’ฌ 5    ๐Ÿ“Œ 1