@yuay908: 席替え好きな人とちょっと近かった!!嬉しい😍てか今日買い物行ったら先輩に会えた꒰^ ̳> ·̫ < ̳^꒱@Closer Food #おすすめにのりたい #口元ASMR #運営さん大好き #粘土加工

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Monday 01 September 2025 06:34:06 GMT
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sondes.24
𝒮ℴ𝓃𝒹ℯ𝓈 :
2025-09-03 13:51:33
308
yoonmi_best
yoonmi_best :
TELL ME HOW IS HER TEETH STILL WHITE😭
2025-09-03 00:20:02
105
rodrig3289
𝓡𝓸𝓭𝓻𝓲𝓰𝓾𝓮𝔃 ⋆ :
Soy la única q abla español???
2025-09-02 21:00:00
32
iyynuueelll_
ciyynull_ :
gua plg suka di situ madu tau😭
2025-09-04 16:46:21
245
admin_eisya
Eisya🏊 :
Me pls 🍓🍩🍭🍭🍭🍰🍉🌭🥦
2025-09-23 11:22:20
2
enardbo67
EnardBaba :
wow
2025-09-25 10:53:55
2
wannafahmook
ฟ้าใสไข่มุก แฟมิลี่ :
What time I need my car hi🥓🥓🥓🍬🍭🍡🍧🍰🍫🧋🧋🧋🧋🍫🍫🍫🍫🍫🍫🍫
2025-09-22 11:41:55
2
sallypriv5
Sallyprivv :
Is that mango thing actually a mango or is it candy?
2025-09-04 01:15:22
8
stecuuuuu448
√ :
apa cmn aku yang indo
2025-09-01 08:03:40
80
md.junaed270
💕আসমানি 💕 :
🧀🥨🍧🍫🍰🧊 প্লিজ প্লিজ
2025-09-18 09:23:00
2
abrahaham_100
𝓓𝓐𝓡𝓘𝓞 :
pplliiss
2025-09-20 22:40:43
2
yashainun
୨୧ :
paling suka bagian mangga 😭
2025-09-24 16:11:18
27
ru17191
? :
待って一緒!笑今日席替えしてないけど、好きな人と席近い!笑
2025-10-03 11:45:34
2
rin._.mimi._.love
みみ🐈ྀི🪽🎀 :
口元界隈ってなんでそんなに恋愛上手く言ってるんだ💖
2025-09-20 03:15:18
2
sdi52170
SDI.えむ𝓜❀𓈒𓏸︎︎︎︎ :
いいなー!うち逆に嫌いな人となった(笑)
2025-09-02 13:30:18
9
lookman186
Sleepylook_man :
Mulai bermunculan asmr guyss
2025-09-21 11:11:11
3
misa._2029
ℳ. :
女子の先輩だったらめっちゃ嬉しいけど男子の先輩とかだとめっちゃ気まずい笑
2025-09-01 07:40:59
6
mai06735
mai🫧🌻 :
うち好きな人と隣になったんですけど私の前の女子と好きぴが、授業中ずっと喋ってて気まずすぎてもういやです🥺🥺
2025-09-06 10:01:51
2
user43059421666088
07彼氏依存性 :
僕も、彼女と席隣に、なりました!
2025-09-09 11:41:20
2
user8184181757565
り :
かわいい❤️😍
2025-09-05 13:50:53
2
chen_ruyi1
陈如意 :
cara buat yg air itu gimana sih gw nyoba engga pecah² 😭😭
2025-09-21 14:41:33
3
lexiepot334
🩷|l•Lian•l|🩷 :
🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🧊🍭🍭🍭🍭🍭🍭🍭🍭🍭🍭🍭🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🥛🧀🧀🧀🧀🧀🧀🧀🧀🧀🧀🧀can you do this pls🥰
2025-09-23 08:14:04
2
misa._2029
ℳ. :
今日も動画最高すぎる
2025-09-01 07:40:24
2
misa._2029
ℳ. :
好きな人の近くとかめっちゃいいじゃん💖
2025-09-01 07:40:09
2
.ceya_1098
nazipa😺 :
こんにちは、皆さんお元気ですか?いつも健康でいらっしゃることを願っております。🤭👋🤗
2025-09-04 08:53:39
3
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Some of the earliest cosmological models of the universe were geocentric, placing Earth at the center. During the Scientific Revolution, astronomical observations led to a heliocentric model. Further observational improvements led to the realization that the Sun is one of a few hundred billion stars in the Milky Way, which is one of a few hundred billion galaxies in the observable universe. At the largest scale, galaxies are distributed uniformly and the same in all directions. At smaller scales, galaxies are distributed in clusters and superclusters, which form immense filaments and voids in space, creating a vast foam-like structure.[11] Discoveries in the early 20th century, including general relativity, led to the modern view of an expanding, isotropic, homogeneous universe. Evidence accumulated supporting the Big Bang theory: an initial hot fireball cooled and becoming less dense as the universe expanded, allowing the first subatomic particles and simple atoms to form. Giant clouds of hydrogen and helium were gradually drawn to the places where matter was most dense, forming the first galaxies, stars, and eventually, everything else. From studying the effects of gravity on both matter and light, it has been discovered that the universe contains much more matter than is accounted for by visible objects; stars, galaxies, nebulae and interstellar gas. This unseen matter is known as dark matter.[12] In the widely accepted ΛCDM cosmological model, dark matter accounts for about 25.8%±1.1% of the mass and energy in the universe while about 69.2%±1.2% is dark energy, a mysterious form of energy responsible for the acceleration of the expansion of the universe.[13] Ordinary ('baryonic') matter therefore composes only 4.84%±0.1% of the universe.[13] Stars, planets, and visible gas clouds only form about 6% of this ordinary matter.[14] There are many competing hypotheses about the ultimate fate of the universe and about what, if anything, preceded the Big Bang.#fyp #explore
Some of the earliest cosmological models of the universe were geocentric, placing Earth at the center. During the Scientific Revolution, astronomical observations led to a heliocentric model. Further observational improvements led to the realization that the Sun is one of a few hundred billion stars in the Milky Way, which is one of a few hundred billion galaxies in the observable universe. At the largest scale, galaxies are distributed uniformly and the same in all directions. At smaller scales, galaxies are distributed in clusters and superclusters, which form immense filaments and voids in space, creating a vast foam-like structure.[11] Discoveries in the early 20th century, including general relativity, led to the modern view of an expanding, isotropic, homogeneous universe. Evidence accumulated supporting the Big Bang theory: an initial hot fireball cooled and becoming less dense as the universe expanded, allowing the first subatomic particles and simple atoms to form. Giant clouds of hydrogen and helium were gradually drawn to the places where matter was most dense, forming the first galaxies, stars, and eventually, everything else. From studying the effects of gravity on both matter and light, it has been discovered that the universe contains much more matter than is accounted for by visible objects; stars, galaxies, nebulae and interstellar gas. This unseen matter is known as dark matter.[12] In the widely accepted ΛCDM cosmological model, dark matter accounts for about 25.8%±1.1% of the mass and energy in the universe while about 69.2%±1.2% is dark energy, a mysterious form of energy responsible for the acceleration of the expansion of the universe.[13] Ordinary ('baryonic') matter therefore composes only 4.84%±0.1% of the universe.[13] Stars, planets, and visible gas clouds only form about 6% of this ordinary matter.[14] There are many competing hypotheses about the ultimate fate of the universe and about what, if anything, preceded the Big Bang.#fyp #explore

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