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Showing posts from September, 2018

Stellar Nucleosynthesis

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Element Origins After the Big Bang, the ordinary matter in the Universe was composed primarily of just two elements: hydrogen and helium. Currently, there are a wide range of elements, from argon to zirconium. These more complex elements were nearly all produced via stellar evolution processes. The formation of new elements is called nucleosynthesis . Below,  I have describe the basics of the chemistry of the Universe and how it has changed over time. Big Bang Nucleosynthesis  The star-forming region 30 Doradus. The blue stars are massive, hot, young stars. They have formed in a cluster out of gas and dust. (Credit: NASA, ESA, HST WFC3) When the Big Bang occurred approximately 14 billion years ago, the Universe was very hot and dense. Over time, the Universe expanded and cooled down. Approximately 0.001 seconds after the Big Bang, particles (e.g., protons and neutrons) began to fuse together to form atomic nuclei, dubbed nuclear fusion . Nuclear fusion process

Astronomy club Demonstration On ATL Inaugration

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On the occasion of the inaugural ceremony of ATL, Astronomy club got a chance to showcase our skills and knowledge about space and space related sciences where we presented hydro rockets, live meteoroid composition , exoplanet weight composition and we gave other others a chance to use see through our MISO(our beloved telescope) which was modified with an inbuilt screen with various star gaze indicators.