Examples of using Heavier elements in English and their translations into German
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Max voltage 50 kV, ideal for heavier elements FingerPrinting module.
Heavier elements than iron and nickel require a supernova for their formation.
Larger stars fused, first, carbon and oxygen and, then, heavier elements.
Heavier elements therefore were only available when the stars of later generations formed.
These so-called waiting point nucleiact like stop signals on the way to even heavier elements.
All heavier elements originate from nucleosynthesis in stars and gigantic stellar explosions.
Observations like this showed that the host galaxy contains surprising amounts of heavier elements and dust.
But no heavier elements, like carbon or oxygen, would have been formed in the early universe.
Within that mixture of material particles andradiation well could appear fusion to even heavier elements.
These heavier elements get blasted into space when massive dying stars explode as supernovae.
The temperature is so great in their interior that they produce heavier elements such as carbon, nitrogen, and oxygen.
All heavier elements like carbon, nitrogen, and oxygen were created much later in the hot nuclear furnaces of stars.
The first stars formed in the universe were comprised of hydrogen andhelium since there was no way to produce heavier elements.
The other 0.1% is made up of heavier elements, mainly carbon, nitrogen, oxygen, neon, magnesium, silicon and iron.
The nuclear fusion reactions that take place when a star hasstopped fusing hydrogen to helium generate heavier elements.
All heavier elements such as iron were produced via nuclear fusion in the interior of these stars and released during supernova explosions.
After about 400 million years, the first stars formed, and that hydrogen, that helium,then began to cook into the heavier elements.
At the end of its life, the Sun will start to fuse helium atoms into heavier elements and swell up, ultimately growing so large it will swallow the Earth.
The interstellar medium of dust and gas from which stars form is primarilycomposed of hydrogen and helium with trace amounts of heavier elements.
The process of building up heavier elements from lighter ones by nuclear reactions, and adjusting the internal structure to balance gravity and pressure, is called stellar evolution.
Unfortunately, with the exception of helium, they found that it was impossible to form heavier elements in any appreciable quantity.
Almost all heavier elements were formed a great deal later, either through fusion processes in the interior of stars or in the course of supernova explosions at the end of a star's life.
They would have been hotter than the Sun,and would have burnt the original hydrogen and helium, into heavier elements, such as carbon, oxygen, and iron.
All heavier elements materialised later in the interior of stars or during star explosions, with each generation of stars contributing a little to enriching the universe with chemical elements. .
Or"Stars shine because their cores are dense and hot enoughthat hydrogen atoms fuse, turning into helium and heavier elements and releasing energy.
And the star stays alive by burning thermonuclear fuel, and as it does so,you get heavier elements like the sponge and all that energy released, like the energy released in a bomb.
Stars of great mass, whose mass is at least eight times the mass of our sun,continue the combustion processes in the core to produce even heavier elements;
When its interior temperature reaches 100 million degrees Kelvin or more and the density of the core is at least ten kilograms per cubic centimeter,the star begins to produce heavier elements.
This creates a situation in which stellar nucleosynthesis produces large amounts of carbon and oxygen butonly a small fraction of these elements is converted into neon and heavier elements.
For example he reads that stars are sustained by fuel:“Stars shine by burning their nuclear fuel, which is initially mainly hydrogen; they fuse it into helium and,later, heavier elements.