Birth Of Solar System #cosmology #space #cosmolog #solarsystem

Birth Of Solar System #cosmology #space #cosmolog #solarsystem

Beyond the Observable Universe

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@shielamarieomang4092
@shielamarieomang4092 - 23.06.2025 16:02

😢

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@shielamarieomang4092
@shielamarieomang4092 - 23.06.2025 16:02

sun is the king

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@清朝皇帝陛下威猛
@清朝皇帝陛下威猛 - 23.06.2025 16:14

Correction🤓:Jupiter came first than Saturn and the rest of the outer planets than was the Inner Planets,oh and Earth started as molten lava (even the surface),by the way only now have I noticed that the rotation of Saturn’s rings doesn’t aline itself with the face,and Uranus’s rings are sideways(so don’t change them it would be more accurate,but uglier)(Jupiter was originally going to be a inner planet,but the creation of Saturn made it become a outer planet,in the process it also made the original inner planets shatter into pieces)

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@RÍTÚ_RÃJ_SÂH
@RÍTÚ_RÃJ_SÂH - 23.06.2025 16:51

Our solar system formed from a vast, swirling cloud of gas and dust called the solar nebula, approximately 4.6 billion years ago. This nebula collapsed, likely triggered by a shockwave from a supernova. The collapsing nebula formed a spinning disk, with most of the material drawn to the center to create the Sun. The remaining material in the disk then clumped together, eventually forming planets, dwarf planets, moons, asteroids, and comets.
Here's a more detailed breakdown:
1. The Solar Nebula:
The process began with a giant, rotating cloud of gas and dust, rich in elements forged in previous stars.
2. Collapse and Flattening:
The nebula collapsed under its own gravity, possibly due to an external trigger like a supernova. As it collapsed, it began to spin faster and flatten into a disk, with most of the material concentrated in the center.
3. Star Formation:
The immense pressure and temperature in the center of the disk led to nuclear fusion, igniting the Sun.
4. Planet Formation:
Within the swirling disk, dust grains collided and stuck together, gradually growing into larger objects called planetesimals. These planetesimals then accreted more material, forming protoplanets and eventually planets.
5. Diverse Planetary System:
The inner solar system, closer to the Sun, became a region of higher temperature, favoring the formation of rocky planets like Mercury, Venus, Earth, and Mars. Further out, where it was cooler, gas and ice giants like Jupiter and Saturn formed, along with Uranus and Neptune.
6. Leftovers:
Asteroids, comets, and other smaller bodies represent the leftover material from the early solar system that didn't coalesce into planets.



Can I get a like please 🥺, it took me half an hour to write

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@annamariearimado7556
@annamariearimado7556 - 23.06.2025 17:18

Where pluto

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@GörkemBayrak-j7r
@GörkemBayrak-j7r - 23.06.2025 17:19

Bu müzik uymuşmu a..

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@carlosdominguez1106
@carlosdominguez1106 - 23.06.2025 17:46

I love the solar system! Who here loves the solar system ⬇.

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@Rewêndcreator
@Rewêndcreator - 23.06.2025 18:05

I love you

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@Birds2456
@Birds2456 - 23.06.2025 21:22

❤❤❤❤

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@AbdulrahmanAlaagouda
@AbdulrahmanAlaagouda - 23.06.2025 22:29

The solar system formed approximately 4.6 billion years ago from a collapsing cloud of gas and dust called the solar nebula. This cloud, likely triggered by a supernova shockwave, began to spin faster and flatten into a disk. The center of the disk became increasingly dense and hot, eventually igniting nuclear fusion and forming the Sun. Around the young Sun, dust and gas in the disk coalesced through accretion, forming planets, dwarf planets, moons, asteroids, and comets.
Here's a more detailed breakdown:

1. The Solar Nebula:
The solar system originated from a vast, rotating cloud of gas and dust, primarily hydrogen and helium, with traces of heavier elements.

2. Gravitational Collapse:
The nebula began to collapse under its own gravity, possibly triggered by a nearby supernova explosion.
3. Formation of the Protoplanetary Disk:
As the nebula collapsed, it started spinning faster and flattened into a disk shape, called a protoplanetary disk, with the majority of the mass concentrated at the center.
4. Birth of the Sun:
The central concentration of mass became extremely hot and dense, eventually initiating nuclear fusion, marking the birth of the Sun.
5. Planetary Accretion:
Within the protoplanetary disk, dust and gas particles began to collide and clump together due to gravity and other forces, growing into larger and larger objects.
6. Planet Formation:
Through continued accretion, these clumps formed protoplanets, which eventually evolved into the planets, dwarf planets, and moons we see today.
7. Clearing the Disk:
The remaining gas and dust in the disk were eventually blown away by the solar wind and radiation from the newly formed Sun.

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@HyamHYam-s4e
@HyamHYam-s4e - 23.06.2025 23:47

Fifkei 10=2025 🤲🏿🤲🏿🤲🏿🥺🥺🌍☀️

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@HyamHYam-s4e
@HyamHYam-s4e - 23.06.2025 23:52

11=264=1200=1927=1998=2018=2025 ❤️😭☀️🌍

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@rosieliz7125
@rosieliz7125 - 24.06.2025 03:50

The sun is lucky to have us and we’re also lucky to have him, warm family ❤

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