TYC 9486-927-1

TYC 9486-927-1 1

Observation data
Epoch       Equinox
Constellation Octans
Right ascension 21h 25m 27.489s[1]
Declination –81° 38 27.68[1]
Characteristics
Spectral type M1 V[1][2]
Astrometry
Radial velocity (Rv)8.7 (±4.6) km/s
Parallax (π)MAS mas
Distance80.7 ly
(24.75 pc)
Details
Mass0.4 M
Temperature3,490 K
RotationVariable Rotation
Rotational velocity (v sin i)43.5 (±1.2)[3] km/s
Age10-45 Myr
Other designations
2MASS J21252752-8138278

TYC 9486-927-1 (also known as 2MASS J21252752-8138278) is a star located at a distance of 24.75 (± 4.25) parsecs from Earth in the southern direction in the constellation of Octans. It is a dwarf (luminosity class V) red (spectral class M1) variable by rotation.

The star is the primary object of a planetary system having the secondary object 2MASS J21265040-8140293. This substellar object, being an exoplanet, is the most extensive planetary systems known to date.

TYC 9486-927-1 has rapid rotation and coronal and chromospheric activity suggestive of a young age. Observations and multi-epoch radial velocity data suggest that TYC 9486-927-1 is a single, rapidly rotating star rather than a spectroscopic or tight, visual binary. However, it is still possible that TYC 9486-927-1 is an equal mass binary with a face-on orbit and close separation.[3]

2MASS J21265040-8140293

Main article: 2MASS J2126-8140

2MASS J21265040-8140293 orbits TYC 9486-927-1 and remains a little-known subject. With a weight from 11.6 to 15 Jupiter masses, it was considered to be either a star, a brown dwarf, or a giant planet.[4][5] It has since be confirmed that it is actually an exoplanet.

References

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