TZ Mensae

TZ Mensae is a binary star in the southern circumpolar constellation Mensa. The system has a combined maximum apparent magnitude of 6.19, placing it near the limit for naked eye visibility. Parallax measurements place the system at a distance of 403 light years. The radial velocity is small.

The components of TZ Mensae have stellar classifications of A0 V and A8 V, both indicating that they are ordinary A-type main-sequence stars. They have masses of $$, and radii of $8.569 days$, respectively. The primary has an effective temperature of $0.13 AU$ and a luminosity 40 times that of the Sun. As for the companion, it has a temperature of 7,178 K. and a luminosity less than The rotation of both stars is apparently synchronous with the orbital period, with projected rotational velocities of $$ respectively. The system is estimated to be 141 million years old.

The two components take about 8 days to revolve around each other in a relatively circular orbit. Since the inclination is close to $$ (actually $$), the two stars periodically pass in front of one another and it has been classified as a eclipsing binary, specifically the Algol type. If the brighter component is eclipsing the dimmer one, the brightness drops to 6.36. If vice versa, it drops to 6.87, which is below the limit for naked eye visibility.