氦元素 | XPS元素周期表 | 赛默飞 | Thermo Fisher Scientific

Helium • Noble Gases

Primary XPS region: N/A
Overlapping regions: N/A
Binding energies of common chemical states: N/A

Experimental information

Helium has a very low photoelectron cross-section and is unlikely to be detected in XPS spectra.

Interpretation of XPS spectra

N/A

General comments

He could possibly be implanted by ion bombardment.
- The small size of a He atom means it is also likely that any implanted He will escape through damage in the crystal structure.

About this element

Symbol: He
Date of discovery: 1895
Name origin: Greek helios
Appearance: colorless
Discoverer: Sir William Ramsay
Obtained from: natural gas deposit air

Melting point: 1.15 K
Boiling point: 4.55 K
Density[kg/m³]: 0.1785
Molar volume: 21.0 × 10^-6 m³/mol
Protons/Electrons: 2
Neutrons: 2
Shell structure: 2
Electron configuration: 1s2
Oxidation state: 0
Crystal structure: hexagonal

While helium was first detected in 1868 as a bright yellow line in the solar spectrum, it took until 1895 for W. Ramsay to isolate it from cleveite. In 1905, H. Cady and D. McFarland isolated helium from natural gas, the current source for most helium today. Helium is a colorless, odorless gas under standard conditions. However, it does exhibit an unusual liquid state near absolute zero known as superfluidity. Many are aware of helium’s lifting power for airships and balloons. Helium is also used as a coolant in MRI systems, superconducting magnets and cryogenics because of its low melting and boiling points. Helium’s inert properties also allow it to be used as a coolant for nuclear reactors.