HR53
HR53 is a double main-sequence star in the constellation of Andromeda.
HR53 visual magnitude is 6.35. Because of its reltive faintness, HR53 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 HR53:
HR53 is below the horizon from Greenwich, United Kingdom .
Altitude: -10.2°
Azimuth: 346.8°
Direction: North-North-West
Celestial coordinates and finder chart of HR53
HR53 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 HR53 are provided in the following table:
The simplified sky map below shows the position of HR53 in the sky:

Visibility of HR53 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR53 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 HR53
The image below is a photograph of HR53 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 HR53 is 0.021 arcsec per year in Right Ascension and -0.031 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR53 from the Sun and relative movement
HR53 is distant 411.62 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Spectral properties of HR53
HR53 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR53 is situated in the Hertzsprung–Russell diagram.

HR53 star system properties
HR53 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR53 double sysyem: