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@efootballwithsani: Zico Blitz Curl ⚡#efootball #efootballmobile #zicoblitzcurler #efootballlover #viral #foreyoupage #efootballwithsani
Efootball With Sani
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Region: BD
Sunday 14 December 2025 09:15:57 GMT
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no name :
need training
2025-12-16 09:42:44
1
COVID 23s :
vai training Ta den plz
2026-07-26 08:20:39
0
kemo :
التطويره ياخويا
2026-02-02 17:07:38
0
rafi :
😬😬😬
2025-12-15 14:58:06
1
Abdullah Alfaz :
🤡
2025-12-16 03:44:10
0
🎀TAMIM🧸 :
bai or t.n. ar pic diban pls
2026-03-06 15:19:31
0
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An ocean planet (or water world) is a hypothetical class of exoplanets where water is not just a surface feature, but a dominant building block, making up 10% to 50% of the planet's total mass. For comparison, while Earth's surface is 71% water, the actual mass of our oceans accounts for a mere 0,02% of Earth's total weight. These aquatic worlds represent a distinct intermediate category between rocky Super-Earths and icy giants like Uranus and Neptune. On these planets, land is completely non-existent, and a global ocean covers 100% of the surface. While Earth’s oceans average about 3.7 kilometers in depth, the global oceans on water worlds plunge down for hundreds or even thousands of kilometers. This immense volume of water generates crushing pressures at the bottom. Under these extreme conditions, water molecules are forced into a solid crystalline structure known as exotic "hot ice" (such as Ice VII or Ice X). This ice remains solid even at temperatures of several hundred degrees Celsius, forming a thick mantle that completely isolates the liquid ocean from the planet's rocky core. This lack of contact between water and minerals is a major focus for scientists, as it could severely hinder the chemical reactions needed to spark life. Ocean planets owe their existence to a process called planetary migration. They initially form in the freezing outer reaches of their solar systems, far beyond the "frost line," where they accumulate from a mix of rock, metal, and vast amounts of water ice. Over time, gravitational interactions with the surrounding protoplanetary disk cause the planet to spiral inward toward its host star. As it heats up, the surface ice melts into a boundless ocean, and the atmosphere fills with water vapor, triggering a powerful greenhouse effect. Today, astronomers have identified several strong candidates based on their mass-to-radius ratios, including the exoplanets GJ 1214 b, TOI-1452 b, and the worlds within the Kepler-138 system. If you would like to explore this topic further, I can explain how scientists calculate a planet's water content from trillions of miles away, or we can look at what the weather and wave cycles would look like on a world with no continents. Which direction would you prefer to go? #ocean #water #Science #fact
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