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  2. Stellar chemistry - Wikipedia

    en.wikipedia.org/wiki/Stellar_chemistry

    The significance of stellar chemical composition is an open ended question at this point. Some research asserts that a greater abundance of certain elements (such as carbon, sodium, silicon, and magnesium) in the stellar mass are necessary for a star's inner solar system to be habitable over long periods of time.

  3. Structural analog - Wikipedia

    en.wikipedia.org/wiki/Structural_analog

    A structural analog, also known as a chemical analog or simply an analog, is a compound having a structure similar to that of another compound, but differing from it in respect to a certain component. [1] [2] [3] It can differ in one or more atoms, functional groups, or substructures, which are replaced with other atoms, groups, or ...

  4. Spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Spectroscopy

    The measured spectra are used to determine the chemical composition and physical properties of astronomical objects (such as their temperature, density of elements in a star, velocity, black holes and more). [12] An important use for spectroscopy is in biochemistry. Molecular samples may be analyzed for species identification and energy content ...

  5. Astrochemistry - Wikipedia

    en.wikipedia.org/wiki/Astrochemistry

    Astrochemistry is the study of the abundance and reactions of molecules in the universe, and their interaction with radiation. [1] The discipline is an overlap of astronomy and chemistry . The word "astrochemistry" may be applied to both the Solar System and the interstellar medium .

  6. Astronomy - Wikipedia

    en.wikipedia.org/wiki/Astronomy

    The study of chemicals found in space, including their formation, interaction and destruction, is called astrochemistry. These substances are usually found in molecular clouds , although they may also appear in low-temperature stars, brown dwarfs and planets.

  7. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    Typical boundary conditions set the values of the observable parameters appropriately at the surface (=) and center (=) of the star: () =, meaning the pressure at the surface of the star is zero; () =, there is no mass inside the center of the star, as required if the mass density remains finite; () =, the total mass of the star is the star's ...

  8. Star - Wikipedia

    en.wikipedia.org/wiki/Star

    A star is a luminous spheroid of plasma held together by self-gravity. [1] The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night; their immense distances from Earth make them appear as fixed points of light.

  9. B2FH paper - Wikipedia

    en.wikipedia.org/wiki/B2FH_paper

    The B 2 FH paper [1] was a landmark scientific paper on the origin of the chemical elements. The paper's title is Synthesis of the Elements in Stars, but it became known as B 2 FH from the initials of its authors: Margaret Burbidge, Geoffrey Burbidge, William A. Fowler, and Fred Hoyle.