Asteroid belt
The asteroid balt or main balt is a ring of small and large rocks and dust between the orbits of Mars and Jupiter. The biggest object in the asteroid balt is Ceres, a dwarf planet. The Kirkwood gaps separate the asteroid balt into several groups.
Most asteroids orbit at 2 to 3 times the distance between Earth and the Sun. Planets that are "inside" - or before - the asterold balt (which means they are closer to the sun) are called inner planets. Planets that are "outside" - that is, after - the asterold balt are called outer planets: so Mercury, Venus, Earth, and Mars are inner planets, while Jupiter, Saturn, Uranus and Neptune are the outer planets.and...Omae wa mou shinderu!!!We must spit on them my brothas. IM A BIG KID NOW
https://www.youtube.com/channel/UCCEnqT2gxaG89PHzfXy7wQg
so im cool but the moon is fake so the asteroid belt is also fake-Umer M 2019
Orgins,lungs,and the Heart
In 1802, shortly after discovering 2 Pallas, Heinrich Olbers suggested to William Herschel that Ceres and Pallas were fragments of a much larger planet that once occupied the Mars–Jupiter region, this planet having suffered an internal explosion or a cometary impact many million years before.[1] This hypothesis has fallen from favor. The large amount of energy needed to destroy a planet, and with the belt's low combined mass (only about 4% of the mass of the Moon) do not support the hypothesis. Also, the significant chemical differences between the asteroids are difficult to explain if they come from the same planet.[2] Today, most scientists accept that the asteroids never formed a planet at all.
In general, the formation and evolution of the Solar System happened when a cloud of interstellar dust and gas collapsed under the influence of gravity to form the Sun and planetesimals, and eventually the planets.[3] This gravitational accretion led to the formation of the rocky planets and the gas giants.
Planetesimals in the region which would become the asteroid belt were too strongly disturbed by Jupiter's gravity to form a planet. Instead they continued to orbit the Sun as before, while occasionally colliding.[4] In regions where the velocity of the collisions was too high, the shattering of planetesimals was more common than accretion,[5] preventing the formation of planet-sized bodies.
References
- ↑ "A brief history of asteroid spotting". Open2.net. Retrieved 2007-05-15.
- ↑ Masetti, M.; and Mukai, K. (2005). "Origin of the Asteroid Belt". NASA Goddard Spaceflight Center. Retrieved 2007-04-25.
{{cite web}}: CS1 maint: multiple names: authors list (link) - ↑ Watanabe, Susan (2001). "Mysteries of the Solar Nebula". NASA. Retrieved 2007-04-02.
- ↑ Petit, J.-M.; Morbidelli, A.; and Chambers, J. (2001). "The primordial excitation and clearing of the Asteroid Belt" (PDF). Icarus. 153 (2): 338–347. Bibcode:2001Icar..153..338P. doi:10.1006/icar.2001.6702. Archived from the original (PDF) on 21 February 2007. Retrieved 2007-03-22.
{{cite journal}}: Unknown parameter|deadurl=ignored (|url-status=suggested) (help)CS1 maint: multiple names: authors list (link) - ↑ Edgar, R.; and Artymowicz, P. (2004). "Pumping of a planetesimal disc by a rapidly migrating planet" (PDF). Monthly Notices of the Royal Astronomical Society. 354: 769–772. arXiv:astro-ph/0409017. Bibcode:2004MNRAS.354..769E. doi:10.1111/j.1365-2966.2004.08238.x. Retrieved 2007-04-16.
{{cite journal}}: CS1 maint: multiple names: authors list (link) CS1 maint: unflagged free DOI (link)
