Examples of using Heavier elements in English and their translations into Chinese
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Where did heavier elements than iron come from?
It then began fusing helium into heavier elements.
Heavier elements need a slight excess of neutrons.
We thought we had a chance of seeing heavier elements escaping.
For heavier elements, this effect is negligible.
Most are hydrogen nuclei, some are helium nuclei,and the rest heavier elements.
To build those heavier elements, nuclei of lighter atoms had to fuse together.
Once its hydrogen supply is depleted,the sun will start consuming its heavier elements.
They thus fuse heavier elements, spinning rapidly and tossing material into space.
If it had been 0.008 or higher,the hydrogen would have fused to make heavier elements.
Stars that contain a lot of heavier elements shed a lot of that mass over their lives.
If it were too large, say 0.008,all the hydrogen would have fused to make heavier elements.
Bigger stars can generate heavier elements like mercury, which has 80 protons in its nucleus.
Most cosmic rays are atomic nuclei: most are hydrogen nuclei, some are helium nuclei,and the rest heavier elements.
If this force were slightly stronger, only heavier elements, but no hydrogen, could be found.
Soon after, even heavier elements also begin to fuse, and the sun on the whole will look a bit worse for the wear.
Inside the ultra-hot environment of the stars,simple hydrogen and helium atoms fused together to create heavier elements.
Bigger stars can generate heavier elements like mercury, which has 80 protons in its nucleus.
These regions are called molecular clouds and consist mostly of hydrogen, with about 23-28% helium and a few percent heavier elements.
Over time, these heavier elements condensed down under gravity to form small clouds and rocks.
Carbon, oxygen, iron, and the like had to wait for stars- especially the massive ones-to form and create heavier elements via nuclear fusion.
One hypothesis is that the heavier elements came from comets that crashed into Jupiter and it absorbed them.
It turns out that, at least according to their calculations, these white dwarfs could reignite in a supernova-like explosion,generating heavier elements.
Since stardust atoms are the heavier elements, the percentage of star mass in our body is much more impressive.
Heavier elements needed to make rocky planets, like silicon and iron, had to be created in the first generations of stars.
Given how fragile elements in the 110s already are, heavier elements might struggle to hold on even that long.
In massive stars, heavier elements can also be burned in a contracting core through the Neon burning process and Oxygen burning process.
But Since star dust atoms are heavier elements, the percentage of star mass in our body is much more impressive.
Heavier elements joined the mix millions of years later, after early stars forged those elements and then dispersed them when they died.