Astrophysics (Index)About

isotope

(subclass of an element with a specific number of nucleons)

An isotope is a subclass of an element with a specific number of nucleons (protons and neutrons), i.e., a specific nuclide. The number of protons (atomic number) determines the element, and given that, the number of neutrons, or equivalently the total of protons and neutrons (mass number) determines the isotope of that element. Some isotopes (unstable isotopes or radioactive isotopes) do not last long, e.g., undergo beta decay frequently enough that their half life is short. Stable isotopes are those that last a long time, and are ultimately more common after the unstable ones disappear. The ratio of the amount of an unstable isotope with its stable result can be used to determine ages of material, i.e., how long since some particular ratio was established.

A typical notation uses the element's symbol with a "left-side superscript" (i.e., superscript preceding the symbol) to indicate the mass number and (optionally, for clarity) a "left-side subscript" to indicate the atomic number. This notation is used, for example, in descriptions of nuclear reactions (e.g., nucleosynthesis). For example (the notation of the common stable isotope of helium, with two protons and two neutrons):

4
 He
2

(physics)
Further reading:
https://en.wikipedia.org/wiki/Isotope

Referenced by pages:
abundances
Advanced Composition Explorer (ACE)
alpha capture
Avogadro's number (NA)
Big Bang nucleosynthesis (BBN)
beta decay
Bose-Einstein statistics
calcium (Ca)
carbon (C)
methane (CH4)
carbon monoxide (CO)
dalton (Da)
deuterium (D)
element
fractionation
fractionation factor
hydrogen cyanide (HCN)
helium (He)
International Cometary Explorer (ICE)
iron (Fe)
potassium/thorium ratio (K/Th ratio)
lithium (Li)
lithium burning
lanthanide (Ln)
magnesium (Mg)
mass number
mole (mol)
Moon formation
neon (Ne)
neutronization
nickel (Ni)
nitrogen (N)
nuclide
oxygen (O)
proton-proton chain
presolar grain
radioactive dating
radioactive decay
radioactive heating
Rosetta
r-process
silicon (Si)
superluminous supernova (SLSN)
supernova light curve (SN light curve)
solar neutrino unit (SNU)
sodium (Na)
Solar and Heliospheric Observatory (SOHO)
spectral line designation
sulfur (S)
technetium star
valley of beta stability

Index