HR9070 is a variable main-sequence star in the constellation of Andromeda.
HR9070 visual magnitude is 6.54. Because of its reltive faintness, HR9070 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 HR9070:
Celestial coordinates and finder chart of HR9070
HR9070 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 HR9070 are provided in the following table:
The simplified sky map below shows the position of HR9070 in the sky:
Visibility of HR9070 from your location
HR9070 is circumpolar and transits at 19:01 UTC (altitude: 84.9°)
Digitized Sky Survey image of HR9070
The image below is a photograph of HR9070 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 HR9070 is 0.022 arcsec per year in Right Ascension and -0.005 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR9070 from the Sun and relative movement
HR9070 is distant 1,358.33 light years from the Sun and it is moving towards the Sun at the speed of 1 kilometers per second.
Spectral properties of HR9070
HR9070 belongs to spectral class B4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR9070 is situated in the Hertzsprung–Russell diagram.