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A nova (plural novae or novas) or classical nova (CN or plural CNe) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star, that slowly fades over several weeks or many months. Novae involve an interaction between two stars that cause the flareup that is perceived as a new entity that is much brighter than the stars involved.
Causes of the dramatic appearance of a nova vary, depending on the circumstances of the two progenitor stars. All novae involve closely located binary stars (the progenitors), either a pair of red dwarfs in the process of merging, or a white dwarf and another star.
The main sub-classes of novae are classical novae, recurrent novae (RNe), and dwarf novae. They are all considered to be cataclysmic variable stars. Luminous red novae share the name and are also cataclysmic variables, but are a different type of event caused by a stellar merger. Also with similar names are the much more energetic supernovae (SNe) and kilonovae.
Classical nova eruptions are the most common type of nova. They are likely created in a close binary star system consisting of a white dwarf and either a main sequence, sub-giant, or red giant star. When the orbital period falls in the range of several days to one day, the white dwarf is close enough to its companion star to start drawing accreted matter onto the surface of the white dwarf, which creates a dense, but thin, atmosphere. This atmosphere is mostly hydrogen and is thermally heated by the hot white dwarf, which eventually reaches a critical temperature causing rapid runaway ignition by fusion.
From the dramatic and sudden energies created, the now hydrogen-burnt atmosphere is then dramatically expelled into interstellar space, and its brightened envelope is seen as the visible light created from the nova event, and previously was mistaken as a "new" star. A few novae produce short-lived nova remnants, lasting for perhaps several centuries. Recurrent nova processes are the same as the classical nova, except that the fusion ignition may be repetitive because the companion star can again feed the dense atmosphere of the white dwarf.
Novae most often occur in the sky along the path of the Milky Way, especially near the observed galactic centre in Sagittarius; however, they can appear anywhere in the sky. They occur far more frequently than galactic supernovae, averaging about ten per year. Most are found telescopically, perhaps only one every year to eighteen months reaching naked-eye visibility. Novae reaching first or second magnitude occur only several times per century. The last bright nova was V1369 Centauri reaching 3.3 magnitude on 14 December 2013.

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  1. P

    WTB WA  Benelli Nova 12ga 28 or 26 inch barrel

    title says it all!
  2. cHaOsReX

    Benelli Nova Tactical with ghost ring sights

    Benelli Nova Tactical with ghost ring sights Sling and butt stock shell holder included There is some slight cosmetic damage to the left side of the gun around the trigger can be seen in pics round count = less than 50 $300 Trades: S&W 586 4" no lock, Ruger PC Carbine 9mm, Colt Snake Gun, BCM...
  3. wired

    WTS WA  Benelli Super Nova Tactical

    18 1/2" Barrel Modified choke ghost ring sights Benelli Super Nova Tactical with Nordic 2 round extension and side rail adapter. Includes original Benelli tube cap and spring, follower. $450. Great 12 gauge 3 1/2" chamber (!) pump gun with unloading feature.
  4. bpotter01

    WTT OR  Beneli nova or win. sxp

    Have a beneli nova and a Winchester sxp. Both are 12g 3.5" both camo beneli is well used sxp is new looking for trade offers not set on anything just don't need two guns that are the same. In the picture the benelli is far left win is on right thanks