HR4167
HR4167 is a double sub-giant star in the constellation of Vela.
HR4167 visual magnitude is 3.84. Because of its moderate brightness, HR4167 should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.
The proper motion of HR4167 is -0.155 arcsec per year in Right Ascension and -0.017 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Key facts about HR4167
HR4167 is below the horizon from Greenwich, United Kingdom.
Altitude: -74.4°
Azimuth: 87.3°
Direction: East
Celestial coordinates and finder chart of HR4167
HR4167 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 HR4167 are provided in the following table:
The simplified sky map below shows the position of HR4167 in the sky:
Visibility of HR4167 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
HR4167 is currently not visible from Greenwich, United Kingdom
Distance of HR4167 from the Sun and relative movement
HR4167 is distant 86.45 light years from the Sun and it is moving far from the Sun at the speed of 19 kilometers per second.
Spectral properties of HR4167
HR4167 belongs to spectral class F4 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR4167 is situated in the HertzsprungāRussell diagram.
HR4167 star system properties
HR4167 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 HR4167 double sysyem: