Helium ( ) is the chemical element with atomic number 2, and is represented by the symbol He. 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.
Welcome to CWAnswers
CWAnswers is your guide to the sprawling world wide web. The directory aims to provide a useful guide made by users. You can share your knowledge as well - simply sign up and edit your first entry. For questions just contact the team at support - at - cwanswers.com.
Weblinks for Helium
Top 10 for Helium
Things about Helium you find nowhere else.
Select content modules
The official blog of Helium.com
So I've joined Helium! ... now what? The official blog of Helium.com ... future features guest blog helium.com Helium Marketplace hyperlocal instruction ...heliumblog.wordpress.com/Blogs & Online Writing Jobs - Helium
A directory of real world knowledge. ... What is Helium. Show All Channels. Jobs & Careers. Online Jobs. Blogs & Online Writing Jobs ...www.helium.com/channels/392-Blogs-Online-Writing-JobsIs Helium a blog? - Who & What is Helium - Helium
15 articles on Is Helium a blog? ... Helium on the face of it has much in common with a blog. ... Yes and no. Like a blog, Helium.com is a way to share ...www.helium.com/knowledge/8351-is-helium-a-blogHelium — Blogs, Pictures, and more on WordPress
... on helium. antihelium wrote 18 hours ago: Boy, the guys at Helium must be ... antihelium wrote 1 day ago: Jim Logan is the latest Helium lackey to email me. ...en.wordpress.com/tag/helium/Helium | QUEST Community Science Blog - KQED
... Field", aircraft, Airship, baseball, Blimp, Hangar, Helium, nasa, Zeppelin. About this Blog ... QUEST Community Science Blog explores local science, nature, ...www.kqed.org/quest/blog/tag/helium/Helium ( ) is the chemical element with atomic number 2, and is represented by the symbol He. 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.
An unknown yellow spectral line signature in light was first observed from a solar eclipse in 1868 by French astronomer Pierre Janssen who is jointly credited with the discovery of the element with Norman Lockyer who observed the same eclipse and was the first to propose this was a new element which he named helium. In 1903, large reserves of helium were found in the natural gas fields of the United States, which is by far the largest supplier of the gas. The substance is used in cryogenics, in deep-sea breathing systems, to cool superconducting magnets, in helium dating, for inflating balloons, for providing lift in airships and as a protective gas for many industrial uses (such as arc welding and growing silicon wafers). Inhaling a small volume of the gas temporarily changes the timbre and quality of the human voice. The behavior of liquid helium-4's two fluid phases, helium I and helium II, is important to researchers studying quantum mechanics (in particular the phenomenon of superfluidity) and to those looking at the effects that temperatures near absolute zero have on matter (such as superconductivity).
Helium is the second lightest element and is the second most abundant in the observable Universe. Most helium was formed during the Big Bang, but new helium is being created as a result of the nuclear fusion of hydrogen in stars. On Earth, helium is relatively rare and is created by the natural radioactive decay of some elements, as alpha particles that are emitted consist of helium nuclei. This radiogenic helium is trapped with natural gas in concentrations up to seven percent by volume, from which it is extracted commercially by a low-temperature separation process called fractional distillation.
Scientific discoveries
The first evidence of helium was observed on August 18, 1868 as a bright yellow line with a wavelength of 587.49 nanometers in the spectrum of the chromosphere of the Sun. The line was detected by French astronomer Pierre Janssen during a total solar eclipse in Guntur, India. This line was initially assumed to be sodium. On October 20 of the same year, English astronomer Norman Lockyer observed a yellow line in the solar spectrum, which he named the D3 Fraunhofer line because it was near the known D1 and D2 lines of sodium. He concluded that it was caused by an element in the Sun unknown on Earth. Lockyer and English chemist Edward Frankland named the element with the Greek word for the Sun, ἥλιος (helios).
























