HR5457
HR5457 is a main-sequence star in the constellation of Lupus.
HR5457 visual magnitude is 6.07. Because of its reltive faintness, HR5457 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 HR5457 is -0.182 arcsec per year in Right Ascension and -0.211 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Key facts about HR5457
HR5457 is below the horizon from Greenwich, United Kingdom.
Altitude: -21.7°
Azimuth: 139.1°
Direction: South-East
Celestial coordinates and finder chart of HR5457
HR5457 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5457 are provided in the following table:
The simplified sky map below shows the position of HR5457 in the sky:
Visibility of HR5457 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
HR5457 is currently not visible from Greenwich, United Kingdom
Distance of HR5457 from the Sun and relative movement
HR5457 is distant 117.44 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR5457
HR5457 belongs to spectral class F7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5457 is situated in the Hertzsprung–Russell diagram.
