
V745 SCO
by Smithsonian Astrophysical Observatory
V745 Sco is a binary star system that consists of a red giant star and a white dwarf locked together by gravity. These two stellar objects orbit so closely around one another that the outer layers of
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v745-sco.glb: b0d902d8632ac88f0c9fe99d50cfa2f2918b130f7eb649f408c95b4c6be17396
Made by Smithsonian Astrophysical Observatory
V745 Sco is a binary star system that consists of a red giant star and a white dwarf locked together by gravity. These two stellar objects orbit so closely around one another that the outer layers of the red giant are pulled away by the intense gravitational force of the white dwarf. This material gradually falls onto the surface of the white dwarf. Over time, enough material may accumulate on the white dwarf to trigger a colossal thermonuclear explosion, causing a dramatic brightening of the binary called a nova.
Description Credit: INAF-Osservatorio Astronomico di Palermo/ S.Orlando & NASA/CXC/SAO/A.Jubett et al.
From Smithsonian Astrophysical Observatory, released by the Smithsonian under CC0 through its Open Access programme. The Smithsonian does not endorse ModelsXi. Its own page has the object record and other copies, including full-resolution and print-ready files where they exist.
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