HR1330 is a main-sequence star in the constellation of Perseus.
HR1330 visual magnitude is 5.45. Because of its reltive faintness, HR1330 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 HR1330:
Celestial coordinates and finder chart of HR1330
HR1330 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 HR1330 are provided in the following table:
The simplified sky map below shows the position of HR1330 in the sky:
Visibility of HR1330 from your location
HR1330 is circumpolar and transits at 23:40 UTC (altitude: 88.6°)
Digitized Sky Survey image of HR1330
The image below is a photograph of HR1330 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 HR1330 is 0.061 arcsec per year in Right Ascension and -0.052 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1330 from the Sun and relative movement
HR1330 is distant 258.94 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.
Spectral properties of HR1330
HR1330 belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1330 is situated in the Hertzsprung–Russell diagram.