title: WISE 0647−6232
text: # WISE 0647−6232
  
  WISE J064723.23−623235.5 (abbreviated WISE 0647−6232) is a nearby brown dwarf of spectral type Y1 ± 0.5, located in constellation Pictor at approximately 28 light-years from Earth. It is one of the two or three reddest and one of the four latest-type brown dwarfs known.
  
  ## History of observations
  
  ### Discovery
  
  WISE 0647−6232 was discovered by Kirkpatrick et al. 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. The discovery was announced in 2013.
  
  WISE 0647−6232 was first imaged by WISE on 9 May 2010. On 17 June 2010 after preliminary data processing it was uncovered as a very cold brown dwarf candidate.
  
  Then were carried out follow-up observations:
  
  * using the Infrared Array Camera (IRAC) on Spitzer Space Telescope, starting from MJD 55458.43 (possibly 16 September 2010);
  * J- and H-band images using Persson's Auxiliary Nasmyth Infrared Camera (PANIC) at the 6.5-meter Magellan Baade telescope at the Las Campanas Observatory, Chile, on 25 November 2010;
  * with the FourStar infrared camera also at Magellan Baade telescope on 15 January 2013 and 23 March 2013;
  * with the Folded-port InfraRed Echellette (FIRE) spectrograph also at Magellan Baade telescope on 24 March 2013;
  * using the Wide Field Camera 3 (WFC3) on Hubble Space Telescope on 13–14 May 2013, and pre-image was obtained on 11 February 2013.
  
  On 25 August 2013 Kirkpatrick et al. submitted the discovery paper to The Astrophysical Journal.
  
  WISE 0647−6232 became the 17th Y-type dwarf discovered and confirmed spectroscopically (in addition, WD 0806-661B is also almost certainly a Y-type dwarf, which was found before discovery of WISE 0647−6232, but it still lacks a spectroscopical confirmation).
  
  ## Distance
  
  Currently the most accurate distance estimate of WISE 0647−6232 is a trigonometric parallax, published in 2019 by Kirkpatrick et al.: 10.0+0.2 −0.2 pc, or 32.5+0.8 −0.8 ly.
  
  WISE 0647-6232 distance estimates :
  
  | Source | Parallax, mas | Distance, pc | Distance, ly | Ref. |
  | - | - | - | - | - |
  | Kirkpatrick et al. (2013) | 115 ± 12 | $8.7^{+1.0}$ $_{−0.8}$ | $28.4^{+3.3}$ $_{−2.7}$ | |
  | Kirkpatrick et al. (2019) | 100.3 ± 2.4 | $10.0^{+0.2}$ $_{−0.2}$ | $32.5^{+0.8}$ $_{−0.8}$ | |
  
  The best estimate is marked in bold.
  
  ## Properties
  
  WISE 0647−6232 has effective temperature 350–400 K and mass ~5–30 $M_{Jup},$ but its kinematics suggests that it may belong to Columba moving group (probability of this is 92.9%, and corresponding radial velocity should be ~22 km/s), if it is so, it may be very young (~30 Myr) and have even lower mass (<2 $M_{Jup}).$ Its blue J − H color may suggest that its surface gravity may be relatively low (log(g)=3.0–3.5, where g is in units of $cm·s^{−2}).$ For ages from 0.1 to more than 10 Gyr log(g)=4.0–5.0.
  
  The only redder than WISE 0647−6232 confirmed Y dwarf is WISE 1828+2650. WD 0806-661B may also be redder than WISE 0647−6232.
  
  The other three latest-type Y dwarfs are: WISE 0350−5658 (Y1), WISE 0535−7500 (≥Y1) and WISE 1828+2650 (≥Y2).
  
  