S62 on a 9.9 yr Orbit around SgrA*

Understand

We observe the S-cluster star S62 on its Keplerian orbit around the supermassive black hole in the center of our galaxy, SgrA*.

• The orbital time period of S62 around SgrA* is 9.9 years.
• We derive its mass to be around 2 M_solar which is consistent with other members of the S-cluster.
• From the Lucy-Richardson deconvolved images, we determine a K-band magnitude of 16.1 mag.