HR1753 is a double main-sequence star in the constellation of Lepus.
HR1753 visual magnitude is 6.36. Because of its reltive faintness, HR1753 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 HR1753:
Celestial coordinates and finder chart of HR1753
HR1753 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 HR1753 are provided in the following table:
The simplified sky map below shows the position of HR1753 in the sky:
Visibility of HR1753 from your location
Digitized Sky Survey image of HR1753
The image below is a photograph of HR1753 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 HR1753 is 0.012 arcsec per year in Right Ascension and 0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1753 from the Sun and relative movement
HR1753 is distant 791.26 light years from the Sun and it is moving far from the Sun at the speed of 10 kilometers per second.
Spectral properties of HR1753
HR1753 belongs to spectral class B3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1753 is situated in the Hertzsprung–Russell diagram.
HR1753 star system properties
HR1753 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR1753 double sysyem: