LP 944-20

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Coordinates: Sky map 03h 39m 35.22s, −35° 25′ 44.09″

LP 944-20
Observation data
Epoch J2000      Equinox J2000
Constellation Fornax
Right ascension 03h 39m 35.220s[1]
Declination –35° 25′ 44.09″[1]
Apparent magnitude (V) 18.69[2]
Characteristics
Spectral type M9[1]
Apparent magnitude (B) ~20.17[1]
Apparent magnitude (I) ~13.288[1]
Apparent magnitude (J) 10.725±0.021[1]
Apparent magnitude (H) 10.017±0.021[1]
Apparent magnitude (K) 9.548±0.023[1]
Astrometry
Proper motion (μ) RA: 317±60[1] mas/yr
Dec.: 276±52[1] mas/yr
Parallax (π) 155.89 ± 1.03[3][4]:{{{3}}} mas
Distance 20.9 ± 0.1 ly
(6.41 ± 0.04 pc)
Absolute magnitude (MV) 20.02
Details
Mass 0.07[2] M
Other designations
LP 944-20,
SIPS J0339−3525,
LEHPM 3451,
2MASSI J0339352−352544,
[B2006] J033935.2−352544,
APMPM J0340−3526,
2MASS J03393521−3525440,
2MASSW J0339352−352544,
BRI B0337−3535,
BRI 0337−3535,
2MUCD 10201
Database references
SIMBAD data

LP 944-20 is a dim brown dwarf of spectral class M9 located about 21 light-years from the Solar System in the constellation of Fornax. With a visual apparent magnitude of 18,[2] it has one of the dimmest visual magnitudes listed on the RECONS page.

On 15 December 1999 a flare was detected.[5]

Distance

The first parallax measurement from 1996 found that LP 944-20 (designated there as BRI 0337−3535) has a relative parallax of \pi_r=200.0\pm4.2 mas, and its correction from relative to absolute parallax (i.e. mean parallax of the reference frame stars) is \pi_{ref}=1.4\pm0.3 mas. This yields an absolute parallax of \pi_r+\pi_{ref}=200.0+1.4=201.4 mas, with a standard deviation (according to \sigma_{X+Y}^2=\sigma_X^2+\sigma_Y^2[6]) of \sqrt{\sigma_{\pi_r}^2+\sigma_{\pi_{ref}}^2}=\sqrt{4.2^2+0.3^2}=4.21 mas, which corresponds to a distance of 5±0.1 pc, or 16.2±0.3 ly.[7] (The same values of absolute parallax and its standard deviation are in the RECONS' TOP100 list.[2][note 1]

A newer parallax, published in 2013, is 155.89±1.03 mas (6.41±0.04 pc or 20.92±0.14 ly).[3]

Lithium and clouds

Observations published in 2007 showed that the atmosphere of LP 944-20 contains much lithium and that it has dusty clouds.[8]

Notes

  1. In RECONS' TOP100 older versions the standard deviation value was 4.20 mas, not 4.21 mas.

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
  3. 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found.
  4. Lua error in package.lua at line 80: module 'strict' not found.
  5. http://www.solstation.com/stars/lp944-20.jpg
  6. Mean and Variance of Random Variables
  7. Lua error in package.lua at line 80: module 'strict' not found.
  8. Lua error in package.lua at line 80: module 'strict' not found.

External links