| Observation data Epoch MJD 55590.80 Equinox J2000 | |
|---|---|
| Constellation | Draco |
| Right ascension | 18h 41m 24.75s |
| Declination | 70° 00′ 38.54″ |
Characteristics | |
| Whole system | |
| Apparent magnitude (J (2MASS filter system)) | 16.800 ± 0.035 |
| Apparent magnitude (J (MKO filter system)) | 16.64 ± 0.03 |
| Apparent magnitude (H (2MASS filter system)) | 16.912 ± 0.082 |
| Apparent magnitude (H (MKO filter system)) | 16.99 ± 0.04 |
| Apparent magnitude (KS (2MASS filter system)) | >15.626 |
| Component A | |
| Spectral type | T5 |
| Apparent magnitude (J (MKO filter system)) | 17.24 ± 0.10 |
| Apparent magnitude (H (MKO filter system)) | 17.73 ± 0.10 |
| Component B | |
| Spectral type | T5 |
| Apparent magnitude (J (MKO filter system)) | 17.57 ± 0.13 |
| Apparent magnitude (H (MKO filter system)) | 17.75 ± 0.10 |
| Astrometry | |
| Proper motion (μ) | RA: -104 ± 25 mas/yr Dec.: 527 ± 28 mas/yr |
| Distance | 131.1 ± 16 ly (40.2 ± 4.9 pc) |
| Orbit | |
| Primary | A |
| Secondary | B |
| Period (P) | ~11 yr |
| Details | |
| Component A | |
| Mass | ≈60 MJup |
| Component B | |
| Mass | ≈60 MJup |
| Position (relative to A) | |
| Component | B |
| Epoch of observation | UT 2010 Jul 1 |
| Angular distance | 70 ± 14 mas |
| Position angle | 82 ± 9° |
| Projected separation | 2.8 ± 0.7 AU |
| Other designations | |
| WISEPA J184124.74+700038.0 WISE J1841+7000 | |
| Database references | |
| SIMBAD | data |
WISEPA J184124.74+700038.0 (designation is abbreviated to WISE 1841+7000) is a binary system of brown dwarfs of spectral classes T5 + T5, located in constellation Draco at approximately 131 light-years from Earth. It is notable for being one of the first known binary brown dwarf systems.
WISE 1841+7000 was discovered in 2011 from data, collected by Wide-field Infrared Survey Explorer (WISE) Earth-orbiting satellite—NASA infrared-wavelength 40 cm (16 in) space telescope, which mission lasted from December 2009 to February 2011. WISE 1841+7000A has two discovery papers: Gelino et al. (2011) and Kirkpatrick et al. (2011). Gelino et al. examined for binarity nine brown dwarfs using Laser Guide Star Adaptive Optics system (LGS-AO) on Keck II telescope on Mauna Kea; seven of these nine brown dwarfs were also newfound, including WISE 1841+7000. These observations had indicated that two of these nine brown dwarfs, including WISE 1841+7000, are binary. Kirkpatrick et al. presented discovery of 98 new found by WISE brown dwarf systems with components of spectral types M, L, T and Y, among which also was WISE 1841+7000.
Component B of the system was discovered in 2011 Gelino et al. with Laser Guide Star Adaptive Optics system (LGS-AO) on Keck II telescope. It was presented in the same article as the component A.
Trigonometric parallax of WISE 1841+7000 is not yet measured. Therefore, there are only distance estimates of this object, obtained by indirect spectrofotometric means (see table).
WISE 1841+7000 distance estimates
| Source | Parallax, mas | Distance, pc | Distance, ly | Ref. |
|---|---|---|---|---|
| Gelino et al. (2011) | 40.2 ± 4.9 | 131.1 ± 16 | ||
| Kirkpatrick et al. (2011) (not assuming binarity) | ~22,4 | ~73,1 |
Non-trigonometric distance estimates are marked in italic. The best estimate is marked in bold.
The other eight objects, checked for binarity by Gelino et al. (2011) on Keck II: