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| has gloss | eng: Supernova nucleosynthesis is the production of new chemical elements inside supernovae. It occurs primarily due to explosive nucleosynthesis during explosive oxygen burning and silicon burning. Those fusion reactions create the elements silicon, sulfur, chlorine, argon, sodium, potassium, calcium, scandium, titanium and iron peak elements: vanadium, chromium, manganese, iron, cobalt, nickel. As a result of their ejection from individual supernovae, their abundances grow increasingly larger within the interstellar medium. Heavy elements (heavier than nickel) are created primarily by a neutron capture process known as the r process. However, there are other processes thought to be responsible for some of the element nucleosynthesis, notably a proton capture process known as the rp process and a photodisintegration process known as the gamma (or p) process. The latter synthesizes the lightest, most neutron-poor, isotopes of the heavy elements. |
| lexicalization | eng: Supernova nucleosynthesis |
| instance of | (noun) a star that explodes and becomes extremely luminous in the process supernova |
| Meaning | |
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| Bulgarian | |
| lexicalization | bul: Нуклеосинтез |
| French | |
| lexicalization | fra: Nucléosynthèse dans les supernovae |
| Korean | |
| has gloss | kor: 초신성 핵합성이란 초신성 내부에서 일어나는 핵융합 혹은 핵분열을 가리킨다. 초신성 초신성은 항성의 대규모 폭발로, 두 가지 발생 원인이 있다. 하나는 백색왜성이 인접 항성으로부터 물질을 흡수하다가 마침내 찬드라세카 한계에 도달하여 폭발을 일으키는 것이다. 다른 한 가지는 보다 일반적인 경우로, 적색거성과 같은 거대한 별이 핵융합 연료를 모두 소진하고 마침내 붕괴하면서 에너지를 방출하는 경우이다. |
| lexicalization | kor: 초신성 핵합성 |
| Castilian | |
| has gloss | spa: La Nucleosíntesis de supernovas se refiere a la producción de nuevos elementos químicos dentro de las supernovas. Ocurre principalmente debido a la nucleosíntesis explosiva durante la combustión de oxígeno explosivo y la combustión del silicio. Estas reacciones de fusión crean los elementos silicio, azufre, cloro, argón, potasio, calcio, escandio, titanio, vanadio, cromo, manganeso, hierro, cobalto y niquel. Como resultado de su expulsión desde supernovas individuales, sus abundancias crecen incrementalmente en el medio interestelar. Los elementos pesados (más pesados que el níquel) son creados principalmente por un proceso de captura de neutrones conocido como Proceso-R. Sin embargo, hay otros procesos que se piensa que son responsables de algunas nucleosíntesis de elementos, principalmente un proceso de captura de protones conocido como el Proceso rp y un proceso de fotodisgregación conocido como el Proceso p. Al final se sintetizan los isótopos más ligeros (pobres en neutrones) de los elementos pesados. |
| lexicalization | spa: Nucleosintesis de supernovas |
| lexicalization | spa: Nucleosíntesis de supernovas |
| Chinese | |
| has gloss | zho: 超新星核合成是闡明新的化學元素如何在超新星內產生，主要發生在易於爆炸的氧燃燒和矽燃燒的爆炸過程產生的核合成。 這些融合反應創造的元素有矽、硫、氯、氬、鉀、鈣、鈧、鈦和鐵峰頂元素：釩、鉻、錳、鐵、鈷、鎳。由於這些元素在每次的超新星爆炸中被拋出來，因此在星際介質中的豐度越來越大。重元素（比鎳重的）主要是由所謂的r-過程捕獲中子創造出來的。然而，還有其他的過程對某些元素的核合成有所貢獻，像是著名的捕獲質子的Rp-過程和導致光致蛻變過程的γ過程或p-過程。重元素中最輕的，中子最少的同位素，都是由後者的程序產生的。 |
| lexicalization | zho: 超新星核合成 |
| Media | |
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| media:img | Keplers supernova.jpg |
| media:img | Nucleosintesis de las Supernovas.jpg |
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