@cbali07:

🦁ALI5 🦁
🦁ALI5 🦁
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Sunday 19 July 2026 11:33:16 GMT
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user4324600501268
هرون عبدالشافي عبدالله :
2026-07-27 13:53:07
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user8152807339961
user8152807339961 :
2026-07-27 13:40:05
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user8779061600727
ابراهيم زكريا :
@مومة
2026-07-27 10:01:49
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abdraman.ibrahim412
Abdraman Ibrahim :
😳😳
2026-07-27 09:39:39
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cbali33
✌️ALi 5✌️ :
Dujfbflcogjebdbcjkcbdbcifkebvdkcicjdhsvxbcjkvirjfjkcjvjxjskakqjdjcjckckjfjsjjdjcjcjcjcxbxbckckckcjgnjdifigkcncbbfbfkfkfkfkgkfikekfjgkgkfkjfjebfififjjrjrjfjgkgkekfjjfkgigkgkgkfkgjjgkfkrkfkigifkekfkgkgkkgkgkgktktizokrkgoh’fkd’f’fkfkgkglofjcnwoskejrbfjickgkgkfkfkrkrjjejekrkgkfkkfkfkrkgkiejdhfjjfjgjrjfjjfjfjsjejkekg’g’kgkfkgj’fkdkgbfbdjhfjrbfjf
2026-07-26 16:39:28
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user8076542279615
سيف الدين هارون :
😇😇😇😇
2026-07-27 15:43:29
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haruonmhd
هارون محمد :
2026-07-27 09:42:18
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mht.abakar16
hassan abakar kaywa :
2026-07-27 08:05:14
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dartama01
Dar tama :
2026-07-26 23:59:33
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user8457306115585
إبراهيم :
2026-07-27 17:37:05
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dartama01
Dar tama :
2026-07-27 00:00:16
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com.riski75
🦁ALI5🦁 :
Rndnflzkeo je suis morte mort 💀 il m’a dit ça en mode il a dit il va pas faire ça à son la rjxjeioo o opecjn. Xldlcnnenwb3&8283849392974747193957920284820483918;€,!!:!:&,&,!;!!;!,!;!!;!;€:€!;&;€€;!;!!;!:!2):));€&,€,):)3)€3€3€3€3€4€4€&4€4€(&;&;€;€&:€:€;€€3€3€37.)2717738485949392992949494948484737392947239487574838388474749939391910203030494
2026-07-26 16:46:32
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kosseymi03
PHONE SÛR 235 PRO :
2026-07-27 09:46:11
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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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