Reionization marks the point at which the hydrogen in the Universe became ionized.
Ionization is the process by which an atom or a molecule acquires a negative or positive charge by gaining or losing electrons to form ions, often in conjunction with other chemical changes.
It is just an Artist rendition of what our galaxy would look like from another galaxy.
The photo above is not to make you feel insignificant, it is only for reference and scale. Depending on your field of view, you would have to be around 100,000 light years away to see this Galaxy using the naked human eye.
ISO/IEC 17005-accredited Beta Analytic is one of the sponsors of the British Sedimentological Research Group (BSRG) 2011 Annual General Meeting to be held in the Royal School of Mines at Imperial College, London, from December 18 to December 21.
This year’s event is the 50th annual general meeting of the BSRG.
Ion is an Atom or a molecule in which the total number of electrons is not equal to the total number of protons, giving the atom or molecule a net positive or negative electrical charge.
Ions can be created, by either chemical or physical means, via ionization. Oxygen is what makes the sky blue, molecules in the air scatter blue light from the sun more than they scatter red light.
The laboratory uses Accelerator Mass Spectrometry (AMS) technology for all analyses, giving the most advanced precision and accuracy.
In the early 2000s, BETA was selected to be senior advisor during the standardization of ASTM D6866, a method that employs radiocarbon dating technology to determine the biobased or fossil origin of carbon in solid, liquid and gaseous samples.
Since 2008, BETA has been annually awarded the ISO/IEC 17005 accreditation by Perry Johnson Laboratory Accreditation, a guarantee that the lab has the technical competency and management systems required to deliver technically valid results consistently.