Astrophysics (Index)About

proton

(type of baryon that is stable and has an electric charge of +1)

A proton is a type of baryon that has an electric charge of +1 and is stable. (A baryon is a hadron, i.e., a composite particle, that is made up of three quarks.) Protons are subject to the strong force, the force which draws together protons and neutrons to form an atomic nucleus as well as holds the three quarks of a neutron or proton together. The nucleus of all elements include protons, but the simplest/most-common hydrogen nucleus consists of just a proton, and ionized hydrogen is just free protons. At room-temperature velocities, protons are merely hydrogen and not dangerous, but higher-velocity protons found in the solar wind and cosmic rays are a danger to humans and to equipment in outer space. Neutrons and protons have roughly the same mass (around 940 MeV), which is about 1800 times that of an electron (around 0.5 MeV).

Protons were created very soon after the Big Bang when the temperature dropped sufficiently that quarks combined into protons and neutrons. Radioactive decay sometimes converts a proton within a nucleus to a neutron or vice versa.


(physics,particle)
Further reading:
https://en.wikipedia.org/wiki/Proton
https://www.britannica.com/science/proton-subatomic-particle
http://hyperphysics.phy-astr.gsu.edu/hbase/Particles/proton.html
https://scienceworld.wolfram.com/physics/Proton.html

Referenced by pages:
1H
acidity (pH)
Advanced Composition Explorer (ACE)
alpha particle
anomalous cosmic rays (ACR)
atomic dark matter (aDM)
atomic number (Z)
aurora
Avogadro's number (NA)
baryon
baryon acoustic oscillations (BAO)
baryonic matter
beta decay
binding energy
Bose-Einstein statistics
Cooper pair
cosmic microwave background (CMB)
cosmic neutrino background (CNB)
cosmic rays (CR)
dalton (Da)
Deep Underground Neutrino Experiment (DUNE)
deuterium (D)
early universe
electron (e-)
electron capture
element
epoch of reionization (EOR)
Fermi-Dirac statistics
fermion
fusion
Genesis
gravitational potential well
gravitational wave strain (h)
ground state
GZK limit
hadron
helium (He)
IMB
International Cometary Explorer (ICE)
inverse square law
ion
isotope
Kamioka Observatory
LIGO
lithium burning
Mars Pathfinder (MPF)
mass
mass number (A)
mole (mol)
neutron
neutron degenerate matter
neutron rich
neutronization
nuclear spectral line
nucleon
nuclide
p-process
pair production
Parker Solar Probe (PSP)
particle
pion (π)
proton-proton chain
quantum number
quark
quark matter (QM)
r-process
radioactivity
recombination
relic
rp-process
SAMPEX
solar energetic particle (SEP)
solar neutrino unit (SNU)
solar particle
solar particle event (SPE)
solar storm
solar wind
standard model
state of ionization
strong force
Sun surface features
superionic ice
synchrotron radiation
valley of beta stability

Index