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ᯓ★ 𝗦𝐔𝐏𝐄𝐑𝐍𝒪𝐕𝐀 .ᐟ
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ᯓ★ 𝗦𝐔𝐏𝐄𝐑𝐍𝒪𝐕𝐀 .ᐟ
@VELOCIDARES
「 #𝐒𝐭𝐚𝐫𝐫𝐲𝐂𝐨𝐟𝐟𝐞𝐞𝐂𝐮𝐩 」 Mun is 21. Slow and sporadic activity. Written by Coffee (she/her) #⃝𝙈̲𝙐̲𝙇̲𝙏̲𝙄̲𝘾̲𝙊̲𝙉̲𝙎̲
Tham gia Şubat 2024
696 Đang theo dõi657 Người theo dõi
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The beauty of the universe is truly unmatched ✨
I never get tired of it
Jasmine 🌌🔭@astro_jaz
how can you not be romantic about space
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“It’s not a loss at all.
Onions are nasty🤢”
#⃝𝙈̲𝙐̲𝙇̲𝙏̲𝙄̲𝘾̲𝙊̲𝙉̲𝙎̲
Asuka Langley Soryu@PilotSoryu
Your loss #⃝𝙈̲𝙐̲𝙇̲𝙏̲𝙄̲𝘾̲𝙊̲𝙉̲𝙎̲
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@TheScientistMon @PEACHYKUNOCHI @SukaiNoMiko *Meanwhile, Melevedy could be seen building sound up in his body for his attack, saying the first word of his attack*
Melevedy: ❝𝐑𝐄𝐂𝐎𝐑𝐃❞
#⃝𝙈̲𝙐̲𝙇̲𝙏̲𝙄̲𝘾̲𝙊̲𝙉̲𝙎̲
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@DE1TY_0F_WAR “ I guess it doesn’t matter much now does it, endeavor or Escanor.
The ball is in your court now. So stop making a pretty lady wait for so long. ”
#⃝𝙈̲𝙐̲𝙇̲𝙏̲𝙄̲𝘾̲𝙊̲𝙉̲𝙎̲

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Planetary Nebula Kronberger 61 – The Soccer Ball NebulaFloating in the constellation Cygnus, about 13,000 light-years from Earth, lies one of the most strikingly spherical planetary nebulae ever discovered: Kronberger 61, affectionately nicknamed the Soccer Ball Nebula.Its brilliant blue glow comes mainly from doubly ionized oxygen atoms (OIII), which emit light at a distinctive wavelength when energized by intense ultraviolet radiation. At the heart of this glowing shell sits a scorching-hot white dwarf — the exposed core of a once Sun-like star. This ultra-hot stellar remnant bathes the surrounding gas in fierce radiation, stripping electrons from atoms and making the entire nebula shine like a cosmic lantern.The nebula’s remarkably round shape and intricate filamentary patterns give it the appearance of a perfectly stitched soccer ball suspended in space. It was discovered in January 2011 by Austrian amateur astronomer Matthias Kronberger while examining archival data, highlighting how even today, dedicated amateurs continue to uncover remarkable objects in our galaxy.Like all planetary nebulae, Kronberger 61 represents the final evolutionary stage of a medium-mass star. After exhausting the hydrogen and helium in its core, the star gently ejected its outer layers into space, creating this beautiful, expanding shell of ionized gas that will slowly fade over the next several thousand years.

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