Harman Patil (Editor)

Rho Tucanae

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Magnitude
  
5.38

Constellation
  
Tucana

People also search for
  
Gamma Tucanae, Eta Tucanae

Rho Tucanae (ρ Tuc, ρ Tucanae) is a binary star in the constellation Tucana.

Rho Tucanae is a spectroscopic binary composed of two yellow-white F-type main sequence dwarfs with a combined apparent magnitude of +5.38. The binary star has a rotation period of 4.82 days. It is approximately 133 light years from Earth.

The projected rotational velocity is 7004235000000000000♠23.5±1.2 km/s.

References

Rho Tucanae Wikipedia