HR1835 is a main-sequence star in the constellation of Columba.
HR1835 visual magnitude is 5.57. Because of its reltive faintness, HR1835 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 HR1835:
Celestial coordinates and finder chart of HR1835
HR1835 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1835 are provided in the following table:
The simplified sky map below shows the position of HR1835 in the sky:
Visibility of HR1835 from your location
Digitized Sky Survey image of HR1835
The image below is a photograph of HR1835 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 HR1835 is 0.009 arcsec per year in Right Ascension and 0.074 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1835 from the Sun and relative movement
HR1835 is distant 293.69 light years from the Sun and it is moving far from the Sun at the speed of 50 kilometers per second.
Spectral properties of HR1835
HR1835 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1835 is situated in the Hertzsprung–Russell diagram.