AB Pictoris

AB Pictoris (abbreviated AB Pic, also catalogued as HD 44627) is a K-type main-sequence star, located 163.5 light-years away in the southern constellation of Pictor. It has been identified as a member of the young (30 million years old) Tucana–Horologium association. The star has been classified as a BY Draconis variable, indicating it has an active chromosphere. It is an X-ray source and displays emission lines in its spectrum.

AB Pictoris

Coronagraphic image of AB Pictoris showing its tiny companion (bottom left). The data was obtained on 16 March 2003 with NACO on the VLT, using a 1.4 arcsec occulting mask on top of AB Pictoris.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pictor
Right ascension 06h 19m 12.913s
Declination −58° 03 15.53
Apparent magnitude (V) 9.13 (9.21 to 9.35)
Characteristics
Spectral type K1V(e)
B−V color index 0.861±0.027
Variable type BY Dra
Astrometry
Radial velocity (Rv)22.6±0.3 km/s
Proper motion (μ) RA: 14.314±0.015 mas/yr
Dec.: 45.234±0.017 mas/yr
Parallax (π)19.9452 ± 0.0124 mas
Distance163.5 ± 0.1 ly
(50.14 ± 0.03 pc)
Absolute magnitude (MV)5.82
Details
Mass0.90±0.10 M
Radius0.92±0.03 R
Luminosity0.51 L
Surface gravity (log g)4.67±0.09 cgs
Temperature5,188±50 K
Metallicity [Fe/H]−0.54 dex
Rotation3.90±0.08 d
Rotational velocity (v sin i)10.87±0.08 km/s
Age30–40 Myr
Other designations
AB Pic, CD−58 1409, CPD−58 670, HD 44627A, 44627, HIP 30034, SAO 234448, PPM 335089
Database references
SIMBADdata

In 2005 it was announced that an astronomical object (AB Pictoris b, abbreviated AB Pic b) had been imaged in 2003 and 2004 close to and apparently in orbit around the star. Its mass suggests that it is at the borderline between being a brown dwarf or a planet.

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