HR 6875

HR 6875, previously known as Sigma Telescopii, is a single star in the constellation Corona Australis. It has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.24. This object is located at a distance of approximately 590 light years from the Sun based on parallax. It is listed as a member of the Sco OB2 association.
This is a hot B-type main-sequence star with a stellar classification of B3 V. It is around 103 million years old and is spinning rapidly with a projected rotational velocity of 248 km/s or perhaps higher. The star has 4.5 times the mass of the Sun and about four times the Sun's radius. It is radiating nearly 400 the luminosity of the Sun from its photosphere at an effective temperature of
A magnitude 10.13 visual companion is located at an angular separation of along a position angle of 162°.