HR5233 is a multiple main-sequence star in the constellation of Virgo.
HR5233 visual magnitude is 6.19. Because of its reltive faintness, HR5233 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 HR5233:
Celestial coordinates and finder chart of HR5233
HR5233 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 HR5233 are provided in the following table:
The simplified sky map below shows the position of HR5233 in the sky:
Visibility of HR5233 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's HR5233 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 HR5233
The image below is a photograph of HR5233 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 HR5233 is -0.172 arcsec per year in Right Ascension and -0.03 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR5233 from the Sun and relative movement
HR5233 is distant 110.25 light years from the Sun and it is moving towards the Sun at the speed of 19 kilometers per second.
Spectral properties of HR5233
HR5233 belongs to spectral class F8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5233 is situated in the Hertzsprung–Russell diagram.
HR5233 star system properties
HR5233 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR5233 double sysyem: