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The Samnites (Oscan: Safineis) were an ancient Italic people who lived in Samnium, which is located in modern inland Abruzzo, Molise and Campania in south-central Italy. An Oscan-speaking people who may have originated as an offshoot of the Sabines, they formed a confederation consisting of four tribes: the Hirpini, Caudini, Caraceni, and Pentri. Although they allied with Rome against the Gauls in 354 BC, they later became enemies of the Romans and fought them in a series of three wars; despite an overwhelming victory at the Battle of the Caudine Forks (321 BC), the Samnites were subjugated in 290 BCE. Although severely weakened, the Samnites would still side against the Romans, first in the Pyrrhic War and then with Hannibal in the Second Punic War. They also fought in the Social War and later in Sulla's civil war as allies of the Roman consuls Papirius Carbo and Gaius Marius against Sulla, who defeated them and their leader Pontius Telesinus at the Battle of the Colline Gate (82 BC). Afterwards, they were assimilated by the Romans and ceased to exist as a distinct people.
The Samnites had an economy focused upon livestock and agriculture. Samnite agriculture was highly advanced for its time, and they practiced transhumance. Aside from relying on agriculture the Samnites exported goods such as ceramics, bronze, iron, olives, wool, pottery, and terracottas.
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The Sun is the star at the center of the Solar System. It is a nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy mainly as light and infrared radiation. It is by far the most important source of energy for life on Earth. Its diameter is about 1.39 million kilometres (864,000 miles), or 109 times that of Earth, and its mass is about 330,000 times that of Earth. It accounts for about 99.86% of the total mass of the Solar System.
Roughly three quarters of the Sun's mass consists of hydrogen (~73%); the rest is mostly helium (~25%), with much smaller quantities of heavier elements, including oxygen, carbon, neon, and iron.The Sun is a G-type main-sequence star (G2V) based on its spectral class. As such, it is informally and not completely accurately referred to as a yellow dwarf (its light is closer to white than yellow). It formed approximately 4.6 billion years ago from the gravitational collapse of matter within a region of a large molecular cloud. Most of this matter gathered in the center, whereas the rest flattened into an orbiting disk that became the Solar System. The central mass became so hot and dense that it eventually initiated nuclear fusion in its core. It is thought that almost all stars form by this process.
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