55 Virginis
55 Virginis is a main-sequence star in the constellation of Virgo.
55 Virginis visual magnitude is 5.33. Because of its reltive faintness, 55 Virginis should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about 55 Virginis:
55 Virginis is below the horizon from Greenwich, United Kingdom .
Altitude: -58.3°
Azimuth: 353.0°
Direction: North
Celestial coordinates and finder chart of 55 Virginis
55 Virginis is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 55 Virginis are provided in the following table:
The simplified sky map below shows the position of 55 Virginis in the sky:

Visibility of 55 Virginis from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's 55 Virginis rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of 55 Virginis
The image below is a photograph of 55 Virginis from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of 55 Virginis is -0.122 arcsec per year in Right Ascension and 0.167 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Distance of 55 Virginis from the Sun and relative movement
55 Virginis is distant 125.92 light years from the Sun and it is moving towards the Sun at the speed of 45 kilometers per second.
Spectral properties of 55 Virginis
55 Virginis belongs to spectral class G6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 55 Virginis is situated in the Hertzsprung–Russell diagram.
