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K !

@tatertoot.bsky.social

24 • she/they • shitty artist • twitch streamer • cosmetologist

15 Followers  |  15 Following  |  1 Posts  |  Joined: 16.11.2024  |  2.1628

Latest posts by tatertoot.bsky.social on Bluesky

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My painting NORTHERN ENGLAND

30.04.2025 13:15 — 👍 15668    🔁 1022    💬 315    📌 32

Goal of the protagonist in:
French novel: "to fall in love"
British novel: "to get married"
Russian novel: "to become a great man"
American novel: "to kill that fuckin' whale, man. I want that GOD DAMN whale to die. FUCK, I hate whales so much!!"

03.12.2024 18:49 — 👍 4808    🔁 560    💬 119    📌 45
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 — 👍 5825    🔁 474    💬 53    📌 28

If you’re afraid that books might change someone’s thinking, you’re not afraid of books, you’re afraid of thinking.

03.12.2024 21:02 — 👍 65899    🔁 11614    💬 881    📌 400

Normalize posting the messy sketches!
Normalize sharing your least favorite pieces!
Normalize creating art for vengeance by drawing your enemies in compromising positions with various farm equipment!
Normalize group critiques!

18.11.2024 04:52 — 👍 23326    🔁 2189    💬 314    📌 91

My turn!!! Let’s be friends!!!

💙Nana
🦋The band ghost
🌀Scott pilgrim
💙Studio ghibli
🦋Final fantasy X
🌀Alt/emo/midwest Emo/metal music
💙Animal crossing
🦋Zelda
🌀Fallout
💙Cats
🦋Horror
🌀Junji ito
💙Dexter
🦋Minecraft
🌀Streamer
💙Video games
🦋and lots more!!!

#promosky

18.11.2024 18:36 — 👍 8    🔁 0    💬 1    📌 0

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