THE Sun generates huge amounts of energy by combining
hydrogen nuclei into helium.
The most obvious example is a fusion reactor that has been running smoothly for more than 4 billion years: the sun, which fuses hundreds of millions of tons of
hydrogen nuclei into helium every second.
Not exact matches
This theory assumes that the heavier elements have properties which can only actually result from a very rare process in the universe which makes several
hydrogen nuclei fuse
into heavier ones.
Pagels (1984) points out that if the relative masses of protons and neutrons were different by a small fraction of 1 per cent, making the proton heavier than the neutron,
hydrogen atoms would be unstable since the protons that constitute their
nuclei would spontaneously decay
into neutrons.
With no nuclear fusion to sustain them, they collapse
into Earth - size balls of tightly bound carbon and oxygen
nuclei with an outer layer of
hydrogen plasma (disrupted atoms).
Immense heat, pressure and magnetic fields ionise and contain the gas, turning it
into a plasma in which
hydrogen nuclei fuse to form helium
nuclei, releasing energy.
Magnetized Linear inertial Fusion (MagLIF) combines powerful laser light with strong magnetic fields to fuse
hydrogen atoms
into helium
nuclei.
Specifically, they measured
hydrogen and its isotope, deuterium (
hydrogen with an extra neutron in its
nucleus) with ion microprobes, which use a focused beam of ions to sputter ions from a small rock sample
into a mass spectrometer.
Comets are surrounded by a huge cloud of atomic
hydrogen because water (H2O) vaporizes from the icy
nucleus, and solar ultraviolet light breaks it apart
into hydrogen and oxygen.
Their hope was that the neutrons shooting
into the acetone would collide with the carbon and
hydrogen nuclei, and this would create disturbances that would «seed» the bubbles produced by the sound waves.
When an antineutrino hits a proton — a
hydrogen nucleus in a water molecule in the giant tank — it transforms that proton
into a neutron and a positron.
The team used a novel technique that involves replacing the electrons in
hydrogen atoms with negatively charged particles called muons, and then measuring subtle shifts in the energy that is required to bump a muon
into a higher - energy orbit around the single - proton
nucleus.
... the Sun and most other stars is the fusion of the lightest element,
hydrogen, its
nucleus having a single proton,
into helium, the second lightest and second most abundant, with a
nucleus consisting of two protons and two neutrons.
When a very massive star begins to run out of
hydrogen and other nuclear fuels, it can collapse so suddenly that almost all its electrons are driven
into nuclei.
Within the Sun's core, nuclear fusion reactions take place, with
hydrogen nuclei being fused
into helium
nuclei.
«It takes tremendous amounts of energy for protons (
hydrogen nuclei) to combine and change
into neutrons.