MCG+07-07-072, a barred spiral galaxy in the Perseus Cluster, is highlighted for its ring-like spiral arms in this Hubble Space Telescope image. Credit: ESA/Hubble & NASA, I. Chilingarian In the Perseus Cluster lies the galaxy MCG+07-07-072, a barred spiral with an unusual near-circular structure.
Its classification as an SBc(r) galaxy reveals the complexity of galactic forms. The subject of this mesmerizing circular Hubble Space Telescope image is situated in the Perseus Cluster, also known as Abell 426, 320 million light-years from Earth. It’s a barred spiral galaxy known as MCG+07-07-072, seen here among a number of photobombing stars that are much closer to Earth than it is.
Unique Structures in Spiral Galaxies MCG+07-07-072 has quite an unusual shape, for a spiral galaxy, with thin arms emerging from the ends of its barred core to draw a near-circle around its disc. It is classified, using a common extension of the basic Hubble scheme, as an SBc(r) galaxy: the c denotes that its two spiral arms are loosely wound, each only performing a half-turn around the galaxy, and the (r) is for the ring-like structure they create. Rings in galaxies come in quite a few forms, from merely uncommon, to rare and astrophysically important! Diverse Galactic Forms: Lenticular and Ring Galaxies Lenticular galaxies are a type that sit between elliptical and spiral galaxies.
They feature a large disc, unlike an elliptical galaxy, but lack any spiral arms. Lenticular means lens-shaped, and t.