HR3445
HR3445 is a variable and double supergiant star in the constellation of Vela.
HR3445 visual magnitude is 3.84. Because of its moderate brightness, HR3445 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 HR3445 is 0 arcsec per year in Right Ascension and 0.003 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Key facts about HR3445
HR3445 is below the horizon from Greenwich, United Kingdom.
Altitude: -44.5°
Azimuth: 113.7°
Direction: East-South-East
Celestial coordinates and finder chart of HR3445
HR3445 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 HR3445 are provided in the following table:
The simplified sky map below shows the position of HR3445 in the sky:
Visibility of HR3445 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
HR3445 is currently not visible from Greenwich, United Kingdom
Distance of HR3445 from the Sun and relative movement
HR3445 is distant 3,104.76 light years from the Sun and it is moving far from the Sun at the speed of 25 kilometers per second.
Spectral properties of HR3445
HR3445 belongs to spectral class F3 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR3445 is situated in the HertzsprungāRussell diagram.
HR3445 star system properties
HR3445 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 HR3445 double sysyem: