ਰਸਾਇਣਕ ਤੱਤ: ਰੀਵਿਜ਼ਨਾਂ ਵਿਚ ਫ਼ਰਕ

ਸਮੱਗਰੀ ਮਿਟਾਈ ਸਮੱਗਰੀ ਜੋੜੀ
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ਲਾਈਨ 7:
ਇਹ ਕਿਰਿਆਵਾਂ ਇਸ ਪ੍ਰਕਾਰ ਹਨ:
* [[ਕਾਸਮਿਕ ਤਰੰਗ ਬਿਖੇੜਾ]] (important for [[lithium]], [[beryllium]] and [[boron]], though some of these may have formed in the Big Bang), and
* [[stellarਤਾਰਾ nucleosynthesisਨਾਭਿਕ ਸੰਸਲੇਸ਼ਣ]] which produces all elements heavier than boron (with carbon being the first of this series). The very heaviest elements (those beyond element 94, [[plutonium]]) decay with [[Half-life|half lives]] too short to allow them to be observed naturally on Earth.
 
In total, 118 elements have been characterized as of March 2010, and new elements of higher atomic number are "discovered" from time to time, as new synthetic products of artificial [[nuclear reaction]]s. Of the known elements, the first 94 occur naturally on Earth. Of these, oxygen is the most abundant element in the [[Earth's crust]]. Exactly 80 elements have stable [[isotopes]]: namely all elements with atomic numbers 1 to 82, except elements 43 and 61 ([[technetium]] and [[promethium]]).