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@chocolatte15.bsky.social

31 πŸ‡²πŸ‡½πŸ€πŸˆβš½οΈ Bay Area Sports lover | For the Emperor | OW, EFT, & CS

8 Followers  |  7 Following  |  3 Posts  |  Joined: 04.12.2024  |  1.7803

Latest posts by chocolatte15.bsky.social on Bluesky

Various types of mecha

Various types of mecha

04.05.2025 04:15 β€” πŸ‘ 2887    πŸ” 701    πŸ’¬ 60    πŸ“Œ 35
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β€œPlayoff physicality has gone too far”

03.05.2025 03:30 β€” πŸ‘ 197    πŸ” 21    πŸ’¬ 6    πŸ“Œ 2
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Those eyes! This little tuxedo kitty is the definition of adorable. πŸ₯°πŸ˜»πŸ–€πŸ€

Credit: kohaze102
#cat #catlover #cute #pets

03.01.2025 20:28 β€” πŸ‘ 15971    πŸ” 833    πŸ’¬ 274    πŸ“Œ 35
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Delving in Carlsbad Caverns, New Mexico πŸŒŒπŸ¦‡

#carlsbadcaverns #exploringnewmexico #nationalparks

13.12.2024 01:03 β€” πŸ‘ 17    πŸ” 3    πŸ’¬ 1    πŸ“Œ 0
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Cathedral Caverns was such a beautiful cave! Definitely worth the trip!

12.12.2024 16:52 β€” πŸ‘ 0    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
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I can’t begin to tell you how this one feels more accurate than that AI Piece of garbage wrapped.

07.12.2024 06:08 β€” πŸ‘ 0    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0
Hubble was recently retrained on NGC 6302, known as the "Butterfly Nebula," to observe it across a more complete spectrum of light, from near-ultraviolet to near-infrared, helping researchers better understand the mechanics at work in its technicolor "wings" of gas. The observations highlight a new pattern of near-infrared emission from singly ionized iron, which traces an S shape from lower left to upper right. This iron emission likely traces the central star system’s most recent ejections of gas, which are moving at much faster speeds than the previously expelled mass.

The star or stars at its center are responsible for the nebula's appearance. In their death throes, they have cast off layers of gas periodically over the past couple thousand years. The "wings" of NGC 6302 are regions of gas heated to more than 36,000 degrees Fahrenheit that are tearing across space at more than 600,000 miles an hour.

NGC 6302 lies between 2,500 and 3,800 light-years away in the constellation Scorpius.

Hubble was recently retrained on NGC 6302, known as the "Butterfly Nebula," to observe it across a more complete spectrum of light, from near-ultraviolet to near-infrared, helping researchers better understand the mechanics at work in its technicolor "wings" of gas. The observations highlight a new pattern of near-infrared emission from singly ionized iron, which traces an S shape from lower left to upper right. This iron emission likely traces the central star system’s most recent ejections of gas, which are moving at much faster speeds than the previously expelled mass. The star or stars at its center are responsible for the nebula's appearance. In their death throes, they have cast off layers of gas periodically over the past couple thousand years. The "wings" of NGC 6302 are regions of gas heated to more than 36,000 degrees Fahrenheit that are tearing across space at more than 600,000 miles an hour. NGC 6302 lies between 2,500 and 3,800 light-years away in the constellation Scorpius.

NGC 6302: The "Butterfly Nebula"
Credit:NASA

03.12.2024 21:15 β€” πŸ‘ 5828    πŸ” 474    πŸ’¬ 53    πŸ“Œ 28
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when the sky comes alive ✨

03.12.2024 20:55 β€” πŸ‘ 18501    πŸ” 1147    πŸ’¬ 132    πŸ“Œ 44
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Colorado is just so dang beautiful

04.12.2024 08:00 β€” πŸ‘ 3    πŸ” 0    πŸ’¬ 0    πŸ“Œ 0

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