Faster access than browser!Similarities between Nucleosynthesis and Stellar evolution
Nucleosynthesis and Stellar evolution have 31 things in common (in Unionpedia): Alpha process, Astrophysics, Asymptotic giant branch, Black hole, Carbon, Carbon-burning process, CNO cycle, Deuterium, Electron capture, Helium, Hydrogen, Iron, Isotope, Magnesium, Metallicity, Neon-burning process, Neutron, Nuclear fusion, Nuclear reaction, Nucleon, Oxygen-burning process, Photodisintegration, Planetary nebula, Proton–proton chain reaction, Red giant, Star, Stellar nucleosynthesis, Supernova, Triple-alpha process, Type II supernova, ..., White dwarf. Expand index (1 more) »
Alpha process
The alpha process, also known as the alpha ladder, is one of two classes of nuclear fusion reactions by which stars convert helium into heavier elements, the other being the triple-alpha process.
Alpha process and Nucleosynthesis · Alpha process and Stellar evolution ·
Astrophysics
Astrophysics is the branch of astronomy that employs the principles of physics and chemistry "to ascertain the nature of the astronomical objects, rather than their positions or motions in space".
Astrophysics and Nucleosynthesis · Astrophysics and Stellar evolution ·
Asymptotic giant branch
The asymptotic giant branch (AGB) is a region of the Hertzsprung–Russell diagram populated by evolved cool luminous stars.
Asymptotic giant branch and Nucleosynthesis · Asymptotic giant branch and Stellar evolution ·
Black hole
A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it.
Black hole and Nucleosynthesis · Black hole and Stellar evolution ·
Carbon
Carbon (from carbo "coal") is a chemical element with symbol C and atomic number 6.
Carbon and Nucleosynthesis · Carbon and Stellar evolution ·
Carbon-burning process
The carbon-burning process or carbon fusion is a set of nuclear fusion reactions that take place in the cores of massive stars (at least 8 \beginsmallmatrixM_\odot\endsmallmatrix at birth) that combines carbon into other elements.
Carbon-burning process and Nucleosynthesis · Carbon-burning process and Stellar evolution ·
CNO cycle
The CNO cycle (for carbon–nitrogen–oxygen) is one of the two known sets of fusion reactions by which stars convert hydrogen to helium, the other being the proton–proton chain reaction.
CNO cycle and Nucleosynthesis · CNO cycle and Stellar evolution ·
Deuterium
Deuterium (or hydrogen-2, symbol or, also known as heavy hydrogen) is one of two stable isotopes of hydrogen (the other being protium, or hydrogen-1).
Deuterium and Nucleosynthesis · Deuterium and Stellar evolution ·
Electron capture
Electron capture (K-electron capture, also K-capture, or L-electron capture, L-capture) is a process in which the proton-rich nucleus of an electrically neutral atom absorbs an inner atomic electron, usually from the K or L electron shell.
Electron capture and Nucleosynthesis · Electron capture and Stellar evolution ·
Helium
Helium (from lit) is a chemical element with symbol He and atomic number 2.
Helium and Nucleosynthesis · Helium and Stellar evolution ·
Hydrogen
Hydrogen is a chemical element with symbol H and atomic number 1.
Hydrogen and Nucleosynthesis · Hydrogen and Stellar evolution ·
Iron
Iron is a chemical element with symbol Fe (from ferrum) and atomic number 26.
Iron and Nucleosynthesis · Iron and Stellar evolution ·
Isotope
Isotopes are variants of a particular chemical element which differ in neutron number.
Isotope and Nucleosynthesis · Isotope and Stellar evolution ·
Magnesium
Magnesium is a chemical element with symbol Mg and atomic number 12.
Magnesium and Nucleosynthesis · Magnesium and Stellar evolution ·
Metallicity
In astronomy, metallicity is used to describe the abundance of elements present in an object that are heavier than hydrogen or helium.
Metallicity and Nucleosynthesis · Metallicity and Stellar evolution ·
Neon-burning process
The neon-burning process (nuclear decay) is a set of nuclear fusion reactions that take place in massive stars (at least 8 Solar masses).
Neon-burning process and Nucleosynthesis · Neon-burning process and Stellar evolution ·
Neutron
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Neutron and Nucleosynthesis · Neutron and Stellar evolution ·
Nuclear fusion
In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons).
Nuclear fusion and Nucleosynthesis · Nuclear fusion and Stellar evolution ·
Nuclear reaction
In nuclear physics and nuclear chemistry, a nuclear reaction is semantically considered to be the process in which two nuclei, or else a nucleus of an atom and a subatomic particle (such as a proton, neutron, or high energy electron) from outside the atom, collide to produce one or more nuclides that are different from the nuclide(s) that began the process.
Nuclear reaction and Nucleosynthesis · Nuclear reaction and Stellar evolution ·
Nucleon
In chemistry and physics, a nucleon is either a proton or a neutron, considered in its role as a component of an atomic nucleus.
Nucleon and Nucleosynthesis · Nucleon and Stellar evolution ·
Oxygen-burning process
The oxygen-burning process is a set of nuclear fusion reactions that take place in massive stars that have used up the lighter elements in their cores.
Nucleosynthesis and Oxygen-burning process · Oxygen-burning process and Stellar evolution ·
Photodisintegration
Photodisintegration (also called phototransmutation) is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, enters an excited state, and immediately decays by emitting a subatomic particle.
Nucleosynthesis and Photodisintegration · Photodisintegration and Stellar evolution ·
Planetary nebula
A planetary nebula, abbreviated as PN or plural PNe, is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.
Nucleosynthesis and Planetary nebula · Planetary nebula and Stellar evolution ·
Proton–proton chain reaction
The proton–proton chain reaction is one of the two (known) sets of fusion reactions by which stars convert hydrogen to helium.
Nucleosynthesis and Proton–proton chain reaction · Proton–proton chain reaction and Stellar evolution ·
Red giant
A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses) in a late phase of stellar evolution.
Nucleosynthesis and Red giant · Red giant and Stellar evolution ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
Nucleosynthesis and Star · Star and Stellar evolution ·
Stellar nucleosynthesis
Stellar nucleosynthesis is the theory explaining the creation (nucleosynthesis) of chemical elements by nuclear fusion reactions between atoms within the stars.
Nucleosynthesis and Stellar nucleosynthesis · Stellar evolution and Stellar nucleosynthesis ·
Supernova
A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.
Nucleosynthesis and Supernova · Stellar evolution and Supernova ·
Triple-alpha process
The triple-alpha process is a set of nuclear fusion reactions by which three helium-4 nuclei (alpha particles) are transformed into carbon.
Nucleosynthesis and Triple-alpha process · Stellar evolution and Triple-alpha process ·
Type II supernova
A Type II supernova (plural: supernovae or supernovas) results from the rapid collapse and violent explosion of a massive star.
Nucleosynthesis and Type II supernova · Stellar evolution and Type II supernova ·
White dwarf
A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.
Nucleosynthesis and White dwarf · Stellar evolution and White dwarf ·
The list above answers the following questions
- What Nucleosynthesis and Stellar evolution have in common
- What are the similarities between Nucleosynthesis and Stellar evolution
Nucleosynthesis and Stellar evolution Comparison
Nucleosynthesis has 119 relations, while Stellar evolution has 138. As they have in common 31, the Jaccard index is 12.06% = 31 / (119 + 138).
References
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