HR3495 is a main-sequence star in the constellation of Volans.
HR3495 visual magnitude is 6.05. Because of its reltive faintness, HR3495 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 HR3495:
Celestial coordinates and finder chart of HR3495
HR3495 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 HR3495 are provided in the following table:
The simplified sky map below shows the position of HR3495 in the sky:
Visibility of HR3495 from your location
HR3495 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR3495
The image below is a photograph of HR3495 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 HR3495 is -0.062 arcsec per year in Right Ascension and 0.101 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR3495 from the Sun and relative movement
HR3495 is distant 197.70 light years from the Sun and it is moving far from the Sun at the speed of 9 kilometers per second.
Spectral properties of HR3495
HR3495 belongs to spectral class A4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR3495 is situated in the Hertzsprung–Russell diagram.