HR3571
HR3571 is a double bright giant star in the constellation of Carina.
HR3571 visual magnitude is 3.84. Because of its moderate brightness, HR3571 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR3571:
HR3571 is below the horizon from Greenwich, United Kingdom .
Altitude: -37.3°
Azimuth: 216.6°
Direction: South-West
Celestial coordinates and finder chart of HR3571
HR3571 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 HR3571 are provided in the following table:
The simplified sky map below shows the position of HR3571 in the sky:

Visibility of HR3571 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
HR3571 is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of HR3571
The image below is a photograph of HR3571 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 HR3571 is -0.021 arcsec per year in Right Ascension and 0.038 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR3571 from the Sun and relative movement
HR3571 is distant 311.96 light years from the Sun and it is moving far from the Sun at the speed of 25 kilometers per second.
Spectral properties of HR3571
HR3571 belongs to spectral class B8 and has a luminosity class of II corresponding to a bright giant star.
The red dot in the diagram below shows where HR3571 is situated in the Hertzsprung–Russell diagram.

HR3571 star system properties
HR3571 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 HR3571 double sysyem: