Simulations uncover why some supernova explosions produce so much manganese and nickel Post a Comment Researchers have found white dwarf stars with masses close to the maximum stable mass are likely to produce large amounts of manganese, iron, and nickel after it orbits another star and explodes. Baca JugaAdvanced atomic clock makes a better dark matter detectorPrototype fuel gauge for orbitStellar flares can lead to diminishment of a planet's habitability Read More Share : You may like these posts :Torus nuclear fusion project gets Brexit funding pledge'Very strong' climate change signal in record June heatLarge-scale study 'shows neonic pesticides harm bees'Designers reinvent the tree to beat air pollution Post a Comment for "Simulations uncover why some supernova explosions produce so much manganese and nickel"
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