Logo
Unionpedia
Communication
Get it on Google Play
New! Download Unionpedia on your Android™ device!
Download
Faster access than browser!
 

Presolar grains and S-process

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Presolar grains and S-process

Presolar grains vs. S-process

Presolar grains are interstellar solid matter in the form of tiny solid grains that originated at a time before the Sun was formed (presolar: before the Sun). The slow neutron-capture process or s-process is a series of reactions in nuclear astrophysics that occur in stars, particularly AGB stars.

Similarities between Presolar grains and S-process

Presolar grains and S-process have 11 things in common (in Unionpedia): Asymptotic giant branch, Cosmic dust, Donald D. Clayton, Isotope, Noble gas, Nucleosynthesis, R-process, Red giant, Silicon carbide, Stable nuclide, Xenon.

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 Presolar grains · Asymptotic giant branch and S-process · See more »

Cosmic dust

Cosmic dust, also called extraterrestrial dust or space dust, is dust which exists in outer space, as well as all over planet Earth.

Cosmic dust and Presolar grains · Cosmic dust and S-process · See more »

Donald D. Clayton

Donald Delbert Clayton (born March 18, 1935) is an American astrophysicist whose most visible achievement was the prediction from nucleosynthesis theory that supernovae are intensely radioactive.

Donald D. Clayton and Presolar grains · Donald D. Clayton and S-process · See more »

Isotope

Isotopes are variants of a particular chemical element which differ in neutron number.

Isotope and Presolar grains · Isotope and S-process · See more »

Noble gas

The noble gases (historically also the inert gases) make up a group of chemical elements with similar properties; under standard conditions, they are all odorless, colorless, monatomic gases with very low chemical reactivity.

Noble gas and Presolar grains · Noble gas and S-process · See more »

Nucleosynthesis

Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons, primarily protons and neutrons.

Nucleosynthesis and Presolar grains · Nucleosynthesis and S-process · See more »

R-process

The rapid neutron-capture process, or so-called r-process, is a set of nuclear reactions that in nuclear astrophysics is responsible for the creation (nucleosynthesis) of approximately half the abundances of the atomic nuclei heavier than iron, usually synthesizing the entire abundance of the two most neutron-rich stable isotopes of each heavy element.

Presolar grains and R-process · R-process and S-process · See more »

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.

Presolar grains and Red giant · Red giant and S-process · See more »

Silicon carbide

Silicon carbide (SiC), also known as carborundum, is a semiconductor containing silicon and carbon.

Presolar grains and Silicon carbide · S-process and Silicon carbide · See more »

Stable nuclide

Stable nuclides are nuclides that are not radioactive and so (unlike radionuclides) do not spontaneously undergo radioactive decay.

Presolar grains and Stable nuclide · S-process and Stable nuclide · See more »

Xenon

Xenon is a chemical element with symbol Xe and atomic number 54.

Presolar grains and Xenon · S-process and Xenon · See more »

The list above answers the following questions

Presolar grains and S-process Comparison

Presolar grains has 61 relations, while S-process has 64. As they have in common 11, the Jaccard index is 8.80% = 11 / (61 + 64).

References

This article shows the relationship between Presolar grains and S-process. To access each article from which the information was extracted, please visit:

Hey! We are on Facebook now! »