WISE J080822.18-644357.3

J080822.18-644357.3

Artist's depiction of J080822.18-644357.3
Credit: NASA/Jonathan Holden
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 08h 08m 22.18s
Declination −64° 43 57.3
Characteristics
Evolutionary stage red dwarf
Spectral type M5.5V
Astrometry
Radial velocity (Rv)22.7 ± 0.5 km/s
Proper motion (μ) RA: −11.54±0.12 mas/yr
Dec.: 25.61±0.10 mas/yr
Parallax (π)9.8599±0.0551 mas
Distance331 ly
(101.4 ± 0.6 pc)
Details
Mass0.16+0.03
−0.04
 M
Temperature3050 ± 100 K
Age45+11
−7
 Myr
Other designations
WISE J080822.18-644357.3
Database references
SIMBADdata

WISE J080822.18-644357.3, also called J0808, is a 45+11
−7
Myr old star system in the Carina constellation with a circumstellar debris disk orbiting an M-type red dwarf about 331 lightyears from Earth.

On October 21, 2016, NASA's Goddard Space Flight Center announced that its citizen science project, Disk Detective, discovered a debris disk around J0808, using the WISE telescope, a M5.5V dwarf with significant infrared excess at both 12 and 22 μm. Classified as Peter Pan disk number AWI0005x3s in the project databaseor 5x3s for shorta BANYAN II Bayesian analysis revealed (with 93.9% probability) the star's radial velocity as 20.6 ± 1.4 km/s, associating it with Carina's ~45 Myr old young moving group. Since most M-dwarf debris disks fade in less than 30 million years, this would be the oldest M dwarf debris disk detected in a moving group, implying a change in understanding of constraint in M-dwarf debris disk evolution.

A follow-up study with an optical spectrum obtained with the ANU Siding Spring 2.3 meter telescope showed a Li-rich M5-star with strong emission. The data is consistent with a low accretion of 10−10 M yr −1. ALMA observations did not detect any carbon monoxide, but unresolved 1.3 mm dust emission was detected. Observations with CTIO showed a strong flare and variations in the Paschen-β and Brackett-γ lines, which is a clear sign of accretion.