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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sagittarius |
Right ascension | 17h 45m 40.036s[1] |
Declination | −29° 00′ 28.17″[1] |
Orbit[2] | |
Primary | Sgr A* |
Companion | S62 |
Period (P) | 9.9 yr |
Semi-major axis (a) | 740.1 au |
Eccentricity (e) | 0.976 |
Inclination (i) | 72.76° |
Longitude of the node (Ω) | 122.61° |
Periastron epoch (T) | 2003.33 |
Argument of periastron (ω) (secondary) | 42.62° |
Details | |
Mass | 6.1[2] M☉ |
Database references | |
SIMBAD | data |
S62 is a star in the cluster surrounding Sagittarius A* (Sgr A*), the supermassive black hole in the center of the Milky Way. S62 orbits Sgr A* in 9.9 years, one of the shortest orbital period of any star around Sgr A*. The current record holder, S4716 has a 4.0-year period.[3]
In addition, S62 has a highly eccentric orbit which makes it pass very close to Sgr A*, only 16 astronomical units (2.4×109 km), less than the distance between Uranus and the Sun. The star therefore passes only about 215 times the Schwarzschild radius of Sgr A* (the Schwarzschild radius of Sgr A* is approximately 0.082 AU, or 12 million km).[3]
S62 passes so close to Sgr A* that its orbit has a very large precession: its orbit shifts by about 10° with each revolution. At closest approach, its velocity is about 0.10c (10% of the speed of light) relative to Sgr A*. S62's most recent approach to Sgr A* was towards the end of 2022.[3]
The discovery of S62 improved the bounds on the mass distribution in the center of the Galactic Center, showing that (4.15±0.6)×106 M☉ are concentrated within 16 AU of the center, fully consistent with Sgr A* being a supermassive black hole.[3]