HR1019 is a multiple hypergiant star in the constellation of Perseus.
HR1019 visual magnitude is 5.61. Because of its reltive faintness, HR1019 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 HR1019:
Celestial coordinates and finder chart of HR1019
HR1019 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1019 are provided in the following table:
The simplified sky map below shows the position of HR1019 in the sky:
Visibility of HR1019 from your location
Today's HR1019 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR1019
The image below is a photograph of HR1019 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 HR1019 is 0.038 arcsec per year in Right Ascension and -0.028 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1019 from the Sun and relative movement
HR1019 is distant 526.66 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR1019
HR1019 belongs to spectral class A0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where HR1019 is situated in the Hertzsprung–Russell diagram.
HR1019 star system properties
HR1019 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 HR1019 double sysyem: