New Type Balloon Helium

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$8.00 - $190.00 / Units | 1 Unit/Units (Min. Order)
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Quick Details
helium balloon gas
helium balloon gas
Place of Origin:
Shanghai, China
Brand Name:
SEFIC helium balloon gas
Model Number:
SEFIC-50 helium balloon gas
Helium Gas:
99.999% helium balloon gas
275-187-7 helium balloon gas
Molecular Weight:
4.003 helium balloon gas
Gas Density:
0.1786g/L helium balloon gas
Liquid Density:
125.2g/L helium balloon gas
Specific Gravity:
0.14 helium balloon gas
Boiling Point:
4.3k helium balloon gas
Melting Point:
1.0k helium balloon gas
Critical Temperature:
-268.95 helium balloon gas
Critical Pressure:
0.228MPA helium balloon gas
Supply Ability
Supply Ability:
50000 Unit/Units per Month helium balloon gas
Packaging & Delivery
Packaging Details
SHANGHAI helium balloon gas

Bottle Helium Gas




Product Description



Bottle Helium Gas
(1) Gas: Helium
(2) 10M3/50L Bottle
(3) 200BAR
(4) CE/TPED / GB / DOT  


Helium Introduction:



Helium is a chemical element with symbol He and atomic number 2. It is a colorless, odorless, tasteless, non-toxic, inert, monatomic gas that heads the noble gas group in the periodic table. Its boiling and melting points are the lowest among the elements and it exists only as a gas except in extreme conditions.

Helium is the second lightest element and is the second most abundant element in the observable universe, being present at about 24% of the total elemental mass, which is more than 12 times the mass of all the heavier elements combined. Its abundance is similar to this figure in the Sun and in Jupiter. This is due to the very high nuclear binding energy (per nucleon) of helium-4 with respect to the next three elements after helium. This helium-4 binding energy also accounts for why it is a product of both nuclear fusion and radioactive decay. Most helium in the universe is helium-4, and is believed to have been formed during the Big Bang. Large amounts of new helium are being created by nuclear fusion of hydrogen in stars.

Helium is named for the Greek God of the Sun, Helios. It was first detected as an unknown yellow spectral line signature in sunlight during a solar eclipse in 1868 by French astronomer Jules Janssen. Janssen is jointly credited with detecting the element along with Norman Lockyer. Jannsen observed during the solar eclipse of 1868 while Lockyer observed from Britain. Lockyer was the first to propose that the line was due to a new element, which he named. The formal discovery of the element was made in 1895 by two Swedish chemists, Per Teodor Cleve and Nils Abraham Langlet, who found helium emanating from the uranium ore cleveite. In 1903, large reserves of helium were found in natural gas fields in parts of the United States, which is by far the largest supplier of the gas today.

Helium is used in cryogenics (its largest single use, absorbing about a quarter of production), particularly in the cooling of superconducting magnets, with the main commercial application being in MRI scanners. Helium's other industrial uses—as a pressurizing and purge gas, as a protective atmosphere for arc welding and in processes such as growing crystals to make silicon wafers—account for half of the gas produced. A well-known but minor use is as a lifting gas in balloons and airships.[2] As with any gas with differing density from air, inhaling a small volume of helium temporarily changes the timbre and quality of the human voice. In scientific research, the behavior of the two fluid phases of helium-4 (helium I and helium II), is important to researchers studying quantum mechanics (in particular the property of superfluidity) and to those looking at the phenomena, such as superconductivity, that temperatures near absolute zero produce in matter.

On Earth it is relatively rare—0.00052% by volume in the atmosphere. Most terrestrial helium present today is created by the natural radioactive decay of heavy radioactive elements (thorium and uranium, although there are other examples), as the alpha particles emitted by such decays consist of helium-4 nuclei. This radiogenic helium is trapped with natural gas in concentrations up to 7% by volume, from which it is extracted commercially by a low-temperature separation process called fractional distillation.












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