τ Piscis Austrini (tau Piscis Austrini)
τ Piscis Austrini is a main-sequence star in the constellation of Piscis Austrinus.
τ Piscis Austrini visual magnitude is 4.92. Because of its moderate brightness, τ Piscis Austrini 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 τ Piscis Austrini:
τ Piscis Austrini (tau Piscis Austrini) is above the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of τ Piscis Austrini
τ Piscis Austrini 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 τ Piscis Austrini are provided in the following table:
The simplified sky map below shows the position of τ Piscis Austrini in the sky:
Visibility of τ Piscis Austrini from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's τ Piscis Austrini (tau Piscis Austrini) rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of τ Piscis Austrini
The image below is a photograph of τ Piscis Austrini 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 τ Piscis Austrini is 0.434 arcsec per year in Right Ascension and 0.013 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of τ Piscis Austrini from the Sun and relative movement
τ Piscis Austrini is distant 61.09 light years from the Sun and it is moving towards the Sun at the speed of 15 kilometers per second.
Spectral properties of τ Piscis Austrini
τ Piscis Austrini belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where τ Piscis Austrini is situated in the Hertzsprung–Russell diagram.