Mu Pictoris

Mu Pictoris
Observation data; Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation	Pictor
Right ascension	06h 31m 58.31021s
Declination	−58° 45′ 13.8117″
Apparent magnitude (V)	5.69 (5.71 + 9.43)
Characteristics
Spectral type	B9 Ve or B9 IVn + A8 V:p?
U−B color index	−0.17
B−V color index	−0.06
Astrometry
Radial velocity (Rv)	+0.40±1.00 km/s
Proper motion (μ)	RA: −1.34 mas/yr ; Dec.: +1.77 mas/yr
Parallax (π)	4.31 ± 0.38 mas
Distance	760 ± 70 ly ; (230 ± 20 pc)
Absolute magnitude (MV)	0.20/3.75
Details
μ Pic A
Mass	3.60±0.09 M☉
Luminosity	355 L☉
Temperature	10,568 K
Rotational velocity (v sin i)	228 km/s
Other designations
	μ Pic, CPD−58° 722, HD 46860, HIP 31137, HR 2412, SAO 234564
Database references
SIMBAD	data

μ Pictoris, Latinised as Mu Pictoris, is a binary star^[3] system in the southern constellation Pictor. It is bright enough to be dimly visible to the naked eye, having a combined apparent visual magnitude of 5.69.^[2] Based upon an annual parallax shift of 4.31 mas as seen from Earth,^[1] the system is located roughly 760 light years distant from the Sun. As of 2010, the pair have an angular separation of 2.46 arc seconds along a position angle of 221°.^[4]

The primary, designated component A, is a blue-white star with a visual magnitude of 5.71^[3] and a stellar classification of B9 Ve^[4] or B9 IVn.^[5] The first classification suggests is a B-type main-sequence star, with the 'e' suffix indicating a Be star. The second may instead indicate a somewhat more evolved B-type star that is spinning rapidly, resulting in "nebulous" absorption lines. Photometrically, it shows a pulsation period of 0.397 days, which is likely the same as the rotation period.^[10]

The secondary companion, component B, is a white-hued star of magnitude 9.43^[3] with a classification of A8 V:p?.^[5] This indicates it is an A-type main-sequence star, with the 'p?' suffix suggesting it may be chemically peculiar while the ':' notation says there is some uncertainty about the general classification.

References

^ ^a ^b ^c ^d ^e ^f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
^ ^a ^b ^c ^d Hurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7, Bibcode:1975MNSSA..34....7H.
^ ^a ^b ^c ^d Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
^ ^a ^b ^c Oudmaijer, René D.; Parr, Andrew M. (July 2010), "The binary fraction and mass ratio of Be and B stars: a comparative Very Large Telescope/NACO study", Monthly Notices of the Royal Astronomical Society, 405 (4): 2439–2446, arXiv:1003.0618, Bibcode:2010MNRAS.405.2439O, doi:10.1111/j.1365-2966.2010.16609.x, S2CID 119209332.
^ ^a ^b ^c Corbally, C. J. (1984), "Close visual binaries. I - MK classifications", Astrophysical Journal Supplement Series, 55: 657, Bibcode:1984ApJS...55..657C, doi:10.1086/190973.
^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
^ Corbally, C. J. (December 1984), "Close visual binaries. III - Parameters and evolutionary status", Astronomical Journal, 89: 1887–1896, Bibcode:1984AJ.....89.1887C, doi:10.1086/113700.
^ ^a ^b ^c ^d Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
^ "mu. Pic". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-08-08.{{cite web}}: CS1 maint: postscript (link)
^ Balona, L. A. (December 1995), "Tests of the Pulsation and Starspot Models for the Periodic Be-Stars", Monthly Notices of the Royal Astronomical Society, 277 (4): 1547, Bibcode:1995MNRAS.277.1547B, doi:10.1093/mnras/277.4.1547.

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[vanLeeuwen2007-1] ^ ^a ^b ^c ^d ^e ^f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.

[Hurly1975-2] Hurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7, Bibcode:1975MNSSA..34....7H.

[Eggleton2008-3] Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.

[Oudmaijer2010-4] Oudmaijer, René D.; Parr, Andrew M. (July 2010), "The binary fraction and mass ratio of Be and B stars: a comparative Very Large Telescope/NACO study", Monthly Notices of the Royal Astronomical Society, 405 (4): 2439–2446, arXiv:1003.0618, Bibcode:2010MNRAS.405.2439O, doi:10.1111/j.1365-2966.2010.16609.x, S2CID 119209332.

[corbally1984-5] Corbally, C. J. (1984), "Close visual binaries. I - MK classifications", Astrophysical Journal Supplement Series, 55: 657, Bibcode:1984ApJS...55..657C, doi:10.1086/190973.

[deBruijne2012-6] Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.

[Corbally1984-7] Corbally, C. J. (December 1984), "Close visual binaries. III - Parameters and evolutionary status", Astronomical Journal, 89: 1887–1896, Bibcode:1984AJ.....89.1887C, doi:10.1086/113700.

[Zorec2012-8] Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.

[SIMBAD-9] "mu. Pic". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-08-08.{{cite web}}: CS1 maint: postscript (link)

[Balona1995-10] Balona, L. A. (December 1995), "Tests of the Pulsation and Starspot Models for the Periodic Be-Stars", Monthly Notices of the Royal Astronomical Society, 277 (4): 1547, Bibcode:1995MNRAS.277.1547B, doi:10.1093/mnras/277.4.1547.

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Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation	Pictor
Right ascension	06^h 31^m 58.31021^s^[1]
Declination	−58° 45′ 13.8117″^[1]
Apparent magnitude (V)	5.69^[2] (5.71 + 9.43)^[3]
Characteristics
Spectral type	B9 Ve^[4] or B9 IVn + A8 V:p?^[5]
U−B color index	−0.17^[2]
B−V color index	−0.06^[2]
Astrometry

Radial velocity (R_v)	+0.40±1.00^[6] km/s
Proper motion (μ)	RA: −1.34^[1] mas/yr Dec.: +1.77^[1] mas/yr
Parallax (π)	4.31 ± 0.38 mas^[1]
Distance	760 ± 70 ly (230 ± 20 pc)
Absolute magnitude (M_V)	0.20/3.75^[7]

Details
μ Pic A
Mass	3.60±0.09^[8] `M`_☉
Luminosity	355^[8] `L`_☉
Temperature	10,568^[8] K
Rotational velocity (v sin i)	228^[8] km/s

Other designations
μ Pic, CPD−58° 722, HD 46860, HIP 31137, HR 2412, SAO 234564^[9]
Database references
SIMBAD	data