Stars Besides
Spica, other bright stars in Virgo include
β Virginis (Zavijava),
γ Virginis (Porrima),
δ Virginis (Auva) and
ε Virginis (Vindemiatrix). Other fainter stars that were also given names are
ζ Virginis (Heze),
η Virginis (Zaniah),
ι Virginis (Syrma),
κ Virginis (Kang),
λ Virginis (Khambalia) and
φ Virginis (Elgafar). Image:Virgo (Annotated) (virgo-ann).tiff|thumb|left|The constellation Virgo showing the IAU boundaries, the constellation stick figure, and labels for its brightest stars. Astrophotograph by Eckhard Slawik, from NOIRLab's 88 Constellations project. The 7 main stars of Virgo form 2 distinct star patterns: Beta, Gamma, Delta, Epsilon and Eta Virginis; form an asterism known as "
The Bowl of Virgo". Together with Spica and
Theta Virginis, they form a Y shape. The star
70 Virginis has one of the first known
extrasolar planetary systems with one confirmed planet 7.5 times the mass of
Jupiter. The star
Chi Virginis has one of the most massive planets ever detected, with a mass of 11.1 times that of Jupiter. The sun-like star
61 Virginis has three known planets: one is a
super-Earth and two are
Neptune-mass planets.
SS Virginis is a variable star with a noticeable red color. It varies in magnitude from a minimum of 9.6 to a maximum of 6.0 over approximately one year.
Exoplanets There are 35 verified exoplanets orbiting 29 stars in Virgo, including
PSR B1257+12 (three planets),
70 Virginis (one planet),
Chi Virginis (one planet),
61 Virginis (three planets),
NY Virginis (two planets), and
59 Virginis (one planet).
Deep-sky objects Sombrero Galaxy in Virgo, obtained by the
Event Horizon Telescope collaboration. This is the first direct image of a black hole. Because of the presence of a
galaxy cluster (consequently called the
Virgo Cluster) within its borders 5° to 12° west of ε Vir (Vindemiatrix), this constellation is especially rich in
galaxies. Some examples are
Messier 49 (
elliptical),
Messier 58 (
spiral),
Messier 59 (elliptical),
Messier 60 (elliptical),
Messier 61 (spiral),
Messier 84 (
lenticular),
Messier 86 (lenticular),
Messier 87 (elliptical and a famous
radio source),
Messier 89 (elliptical) and
Messier 90 (spiral). A noted galaxy that is not part of the cluster is the
Sombrero Galaxy (M104), an unusual spiral galaxy. It is located about 10° due west of Spica.
NGC 4639 is a face-on
barred spiral galaxy located from Earth (redshift 0.0034). Its outer arms have a high number of
Cepheid variables, which are used as
standard candles to determine astronomical distances. Because of this, astronomers used several Cepheid variables in NGC 4639 to calibrate
type Ia supernovae as standard candles for more distant galaxies.
M87 is the largest galaxy in the Virgo cluster, and is at a distance of from Earth (redshift 0.0035). It is a major radio source, partially due to its jet of electrons being flung out of the galaxy by its central
supermassive black hole. Because this jet is visible in several different wavelengths, it is of interest to astronomers who wish to observe black holes in a unique galaxy. With a mass of at least 7.2 billion times that of the Sun, it is the most massive black hole within the immediate vicinity of the Milky Way.
M84 is another elliptical
radio galaxy in the constellation of Virgo; it is at a distance of (redshift 0.0035) as well. Astronomers have surmised that the speed of the gas clouds orbiting the core (approximately ) indicates the presence of an object with a mass 300 million times that of the sun, which is most likely a
black hole. The
Sombrero Galaxy, M104, is an edge-on spiral galaxy located 28 million light-years from Earth (redshift 0.0034). It has a
bulge at its center made up of older stars that are larger than normal. It is surrounded by large, bright
globular clusters and has a very prominent
dust lane made up of
polycyclic aromatic hydrocarbons.
NGC 4438 is a
peculiar galaxy with an
active galactic nucleus, at a distance of from Earth (redshift 0.0035). Its supermassive black hole is ejecting
jets of matter, creating bubbles with a diameter of up to .
NGC 4261 also has a black hole from its center with a mass of 1.2 billion solar masses. It is located at a distance of from Earth (redshift 0.0075), and has an unusually dusty disk with a diameter of . Along with M84 and M87, NGC 4261 has strong emissions in the
radio spectrum. Virgo is also home to the
quasar 3C 273 which was the first quasar ever to be identified. With a magnitude of ~12.9, it is also the optically brightest quasar in the sky. == Mythology ==