HR3537 is a double sub-giant star in the constellation of Volans.
HR3537 visual magnitude is 5.35. Because of its reltive faintness, HR3537 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 HR3537:
Celestial coordinates and finder chart of HR3537
HR3537 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 HR3537 are provided in the following table:
The simplified sky map below shows the position of HR3537 in the sky:
Visibility of HR3537 from your location
HR3537 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR3537
The image below is a photograph of HR3537 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 HR3537 is 0.089 arcsec per year in Right Ascension and 0.097 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR3537 from the Sun and relative movement
HR3537 is distant 171.22 light years from the Sun and it is moving far from the Sun at the speed of 42 kilometers per second.
Spectral properties of HR3537
HR3537 belongs to spectral class F5 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR3537 is situated in the Hertzsprung–Russell diagram.
HR3537 star system properties
HR3537 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR3537 double sysyem: