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  2. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    The Solar System, and the other stars/dwarfs listed here, are currently moving within (or near) the Local Interstellar Cloud, roughly 30 light-years (9.2 pc) across. The Local Interstellar Cloud is, in turn, contained inside the Local Bubble, a cavity in the interstellar medium about 300 light-years (92.0 pc) across.

  3. List of nearest stars by spectral type - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars_by...

    Below there are lists the nearest stars separated by spectral type. The scope of the list is still restricted to the main sequence spectral types: M , K , F , G , A , B and O . It may be later expanded to other types, such as S , D or C .

  4. List of nearby stellar associations and moving groups

    en.wikipedia.org/wiki/List_of_nearby_stellar...

    The regions with higher density of stars are shown; these correspond with known star clusters (Hyades and Coma Berenices) and moving groups. This is a list of nearby stellar associations and moving groups. A stellar association is a very loose star cluster, looser than an open cluster. A moving group is the remnant of such a stellar association ...

  5. Diffuse interstellar bands - Wikipedia

    en.wikipedia.org/wiki/Diffuse_interstellar_bands

    Polycyclic aromatic hydrocarbons, long carbon-chain molecules such as polyynes, and fullerenes are all potentially important. [6] [13] These types of molecule experience rapid and efficient deactivation when excited by a photon, which both broadens the spectral lines and makes them stable enough to exist in the interstellar medium. [14] [15]

  6. Fullerene - Wikipedia

    en.wikipedia.org/wiki/Fullerene

    The older, "bottom-up" theory proposes that they are built atom-by-atom. The alternative "top-down" approach claims that fullerenes form when much larger structures break into constituent parts. [74] In 2013 researchers discovered that asymmetrical fullerenes formed from larger structures settle into stable fullerenes.

  7. Endohedral fullerene - Wikipedia

    en.wikipedia.org/wiki/Endohedral_fullerene

    Only very stable fullerenes such as [Sc 3 N] +6 @[C 80] −6 pass through the column unreacted. In Ce 2 @C 80 the two metal atoms exhibit a non-bonded interaction. [4] Since all the six-membered rings in C 80-I h are equal [4] the two encapsulated Ce atoms exhibit a three-dimensional random motion. [5]

  8. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets. The 1,033 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d).

  9. List of star systems within 30–35 light-years - Wikipedia

    en.wikipedia.org/wiki/List_of_star_systems_within...

    System ← → ← → Star or (sub-) brown dwarf Distance ()Constellation Coordinates: RA, Dec (Ep J2000, Eq J2000)Stellar class Apparent magnitude (V) Parallax (Notes and additional references