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Surya Ka Janam: Bhayanak Grahon Ke Beech Ka Maha Manthan Surya ek tarah ka garam gas hai jo hydrogen aur helium se bana hua hai aur khud mein jal raha hai. Is process ko nuclear fusion kehte hain. Surya ka janm lagbhag 4.6 billion saal pehle hua tha. Iska janm ek molekuler cloud (gaseous anday) ke collapse hone se hua tha. Jab yeh gaseous cloud apne aas-pass ke bhag ka sannata samet leta hai, toh usmein gravitational forces (gurutvakarshan kriyayein) aur pressure increase hota hai. Is process ke result mein, cloud ka center extremely high temperature aur pressure par aa jata hai. Jab temperature aur pressure itne high hote hain ki hydrogen atoms ki nuclear fusion shuru ho jati hai, tab surya ka janm hota hai. Is process mein hydrogen atoms ke nuclei (protons) ek-doosre se mil kar helium nuclei banate hain, sath hi energy release hoti hai. Is energy ke karan surya roshni aur garmi emit karta hai. Is tarah, surya ka janm ek complex process hai jo gravitational forces, pressure, temperature, aur nuclear fusion ke interaction se sambhav hua hai. Is process ke baad se surya lagatar nuclear fusion ke dwara apni energy produce karta hai aur humare solar system mein light aur heat pradan karta hai.