HR419 is a double main-sequence star in the constellation of Pisces.
HR419 visual magnitude is 6.58. Because of its reltive faintness, HR419 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 HR419:
Celestial coordinates and finder chart of HR419
HR419 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 HR419 are provided in the following table:
The simplified sky map below shows the position of HR419 in the sky:
Visibility of HR419 from your location
Digitized Sky Survey image of HR419
The image below is a photograph of HR419 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 HR419 is 0.004 arcsec per year in Right Ascension and -0.035 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR419 from the Sun and relative movement
HR419 is distant 521.60 light years from the Sun and it is moving far from the Sun at the speed of 15 kilometers per second.
Spectral properties of HR419
HR419 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR419 is situated in the Hertzsprung–Russell diagram.
HR419 star system properties
HR419 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 HR419 double sysyem: