Hydrogen atoms are the smallest units of hydrogen, which is a gas found in nature. They consist of a nucleus, which is a tiny particle, and an electron that orbits around it.
Hydrogen atoms are the building blocks of hydrogen gas and are involved in chemical reactions to form compounds.
Full definition
All fatty acids consist for the most part of a chain of carbon atoms with varying numbers
of hydrogen atoms attached to them.
The abundance of active
hydrogen atoms on the large particles promotes the formation of methane.
Both materials were then sprayed with hydrogen gas in which the bonds were broken to form
single hydrogen atoms.
As hydrogen atoms move about in space, they can absorb small amounts of energy, sending the atom's single electron to a higher energy state.
The result is that it has two
fewer hydrogen atoms than a saturated fat and a bend at the double bond.
It is the abundance of
active hydrogen atoms on the large particles that promotes the formation of methane from carbon dioxide and hydrogen.
In 100 characters or less: Larger particles offer
more hydrogen atoms, which determine the fate of carbon dioxide's conversion.
The extremely high temperatures — hundreds of millions of degrees Celsius — cause fusion to occur
between hydrogen atoms in the plasma, releasing tons of energy.
However, when water molecules are broken by the stellar radiation into hydrogen and oxygen, the relatively
light hydrogen atoms can escape the planet.
For example, when vegetable oil is heated in the presence of a heavy - metal catalyst and hydrogen,
hydrogen atoms combine with the carbon chain to turn the oil solid.
The fatty acid is bombarded with
hydrogen atoms until those double bonds are broken up and the resulting free electron is shared with a hydrogen.
Within these clouds, on the surfaces of tiny dust grains,
hydrogen atoms link with oxygen to form water.
What makes one fat different from another is the length and shape of the carbon chain and the number of
hydrogen atoms connected to the carbon atoms.
In the universe that consisted of
hydrogen atoms alone, the sum total of occasions of experience must have been minimal in cosmic history.
They are also all saturated fats, chains of single - bonded carbon atoms with
hydrogen atoms neatly lined up on either side of each carbon.
The traditional technique for weighing them takes advantage of the fact that
glowing hydrogen atoms in the disk emit visible light at a particular wavelength.
There, water molecules will be exposed to ultraviolet rays, which will break them into hydrogen and oxygen — and then many of those
lightweight hydrogen atoms will fly off into space.
What they couldn't figure out — what nobody has yet figured out — is where those
original hydrogen atoms came from.
Their composition is largely dependent on
hydrogen atoms in the molecules, and the ability of these to create hydrogen bonds with other elements.
Whenever a pair
of hydrogen atoms is missing the adjacent carbon atoms must form a double bond which produces a weak link in the carbon chain.
In the intense heat at the core of these stars the
lighter hydrogen atoms that had evolved much earlier were transformed into the heavier elements such as carbon, nitrogen and oxygen.
Unlike the sun, which generates energy by fusing
hydrogen atoms into helium, RR Lyrae stars have already used up all the hydrogen in their core and are fusing helium into carbon instead.
Based on previous research and work in the field of plasma physics, the two former Creo laser printing employees believe they can build a reactor to
fuse hydrogen atoms together by pneumatically - driven pistons and produce enormous increases in energy.
Stars below about 1.5 times the mass of the Sun (or 1.5 solar masses) fuse
hydrogen atoms together in a series of stages to form helium, a sequence called the proton - proton chain.
In the case of looking
for hydrogen atoms in water under pressure, the «light» consists of a stream of neutrons.
Instead of searching for the light from individual galaxies with an optical telescope, the team stalked a different quarry, red - shifted radio waves emitted
by hydrogen atoms floating in huge clouds within the galaxies.
Electrical engineers Joseph Lyding and Mark Hersam of the University of Illinois developed a technique for plucking single
hydrogen atoms from a silicon sheet, which may lead to a millionfold increase in the number of transistors that can be packed onto a chip.
Building on a 1981 proposal by three Russian theorists and more recent work that brought that proposal into the realm of possibility, the team first fired two lasers at
hydrogen atoms inside a chamber, kicking off electrons at speeds and directions that depended on their underlying wave functions.
Cosmic and biological evolution involve change in structures — as, for example, when electrons and protons
form hydrogen atoms.
An easy - to - measure current density of one microampere per square centimeter corresponds a stream of about six trillion (6 × 10 ^ 12) single
hydrogen atoms per second per square centimeter.
As the first stars flickered on, their ultraviolet light excited neutral
hydrogen atoms around them, causing the gas to emit a faint radio signal at 1,420 megahertz.
The second involves colliding a positively charged muon and a muonic
hydrogen atom made up of a proton and a negative muon.
He and his colleagues slammed a beam of
heavy hydrogen atoms into a cloud composed of more heavy hydrogen.
When the two catalysts are added to a batch of short alkanes, the first catalyst
strips hydrogen atoms off adjacent carbon atoms in single alkane molecules.
The technique involves
replacing hydrogen atoms on fatty acids with their isotope, deuterium, without changing their physicochemical properties and behavior like traditional strategies do.
As our solar system slowly orbits around the galactic center, the sun's ultraviolet radiation carves out an egg - shaped region of
ionized hydrogen atoms surrounded by neutral hydrogen gas.
The sun was born in a moment some 4.6 billion years ago,
when hydrogen atoms began fusing into helium.
Phrases with «hydrogen atoms»