HR1359 is a double main-sequence star in the constellation of Eridanus.
HR1359 visual magnitude is 6.37. Because of its reltive faintness, HR1359 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 HR1359:
Celestial coordinates and finder chart of HR1359
HR1359 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 HR1359 are provided in the following table:
The simplified sky map below shows the position of HR1359 in the sky:
Visibility of HR1359 from your location
Digitized Sky Survey image of HR1359
The image below is a photograph of HR1359 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 HR1359 is 0.017 arcsec per year in Right Ascension and -0.006 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1359 from the Sun and relative movement
HR1359 is distant 378.63 light years from the Sun and it is moving far from the Sun at the speed of 16 kilometers per second.
Spectral properties of HR1359
HR1359 belongs to spectral class A3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1359 is situated in the Hertzsprung–Russell diagram.
HR1359 star system properties
HR1359 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 HR1359 double sysyem: