HR5445
HR5445 is a double main-sequence star in the constellation of Boötes.
HR5445 visual magnitude is 6.33. Because of its reltive faintness, HR5445 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.
The proper motion of HR5445 is 0.108 arcsec per year in Right Ascension and 0.007 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Key facts about HR5445
HR5445 is above the horizon from Greenwich, United Kingdom .
Altitude: 24.1°
Azimuth: 67.4°
Direction: East-North-East
Celestial coordinates and finder chart of HR5445
HR5445 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 HR5445 are provided in the following table:
The simplified sky map below shows the position of HR5445 in the sky:
Visibility of HR5445 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR5445 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Distance of HR5445 from the Sun and relative movement
HR5445 is distant 137.44 light years from the Sun and it is moving towards the Sun at the speed of 8 kilometers per second.
Spectral properties of HR5445
HR5445 belongs to spectral class F5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5445 is situated in the Hertzsprung–Russell diagram.
HR5445 star system properties
HR5445 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 HR5445 double sysyem: