Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cetus |
Right ascension | 02h 26m 24.20s |
Declination | −02° 11′ 37.66″ |
Characteristics | |
Evolutionary stage | brown dwarf |
Spectral type | T8+Y0[2] |
Astrometry | |
Proper motion (μ) | RA: -294.4 ±1.4 mas/yr[3] Dec.: -432.3 ±1.2 mas/yr[3] |
Parallax (π) | 56.3 ± 2.5 mas[3] |
Distance | 58 ± 3 ly (17.8 ± 0.8 pc) |
Details[3] | |
WISE 0226−0211A | |
Temperature | 686 ± 79 K |
WISE 0226−0211B | |
Temperature | 511 ± 79 K |
Position (relative to WISE 0226−0211A)[2] | |
Component | WISE 0226−0211B |
Angular distance | 2.1″ |
Other designations | |
CNS5 617, WISEA J022623.99-021142.7, WISEP J022623.98-021142.8, WISE J022623.98-021142.8, EQ J0226-0211 | |
Database references | |
SIMBAD | data |
WISE 0226−0211 (also known as WISEPA J022623.98−021142.8) is a brown dwarf binary with a combined spectral type of T7.[4] Its individual components have a spectral type that is as of now somewhat uncertain at T8-T8.5 for the primary and T9.5-Y0 for the secondary.[2]
The object was first discovered in 2011 with the Wide-field Infrared Survey Explorer and follow-up observations with Keck revealed a spectral type of T7.[4] In 2019 the same team showed that the object is a common proper motion binary with a separation of 2.1 arcseconds from Spitzer images and one H-band Keck image (acquired by David Ciardi). The H-ch2 colors suggest a spectral type of about T8-T8.5 for the primary and about Y0 for the secondary. The absolute magnitudes on the other hand suggest spectral types of about T8-T8.5 for the primary and about T9.5-Y0 for the secondary. It is suspected that the combined spectral type of T7 is in error.[2]
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