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Lambda Pictoris information


Lambda Pictoris
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Pictor
Right ascension 04h 42m 46.42350s[1]
Declination −50° 28′ 52.8050″[1]
Apparent magnitude (V) +5.29[2]
Characteristics
Spectral type K0/1 III[3]
U−B color index +0.74[2]
B−V color index +0.98[2]
Astrometry
Radial velocity (Rv)+4.60[4] km/s
Proper motion (μ) RA: −36.02[1] mas/yr
Dec.:  mas/yr
Parallax (π)8.71 ± 0.18 mas[1]
Distance374 ± 8 ly
(115 ± 2 pc)
Details
Mass2.20[4] M
Luminosity112[4] L
Surface gravity (log g)2.77±0.09[5] cgs
Temperature4,851±45[4] K
Metallicity [Fe/H]−0.13±0.03[5] dex
Age2.24[4] Gyr
Other designations
λ Pic, CD−50° 1471, FK5 2351, HD 30185, HIP 21914, HR 1516, SAO 233638[6]
Database references
SIMBADdata

λ Pictoris, Latinised as Lambda Pictoris, is a solitary,[7] orange-hued star in the southern constellation of Pictor. It is visible to the naked eye, having an apparent visual magnitude of +5.29.[2] With an annual parallax shift of 8.71[1] mas as seen from the Earth, it is located around 374 light-years from the Sun. At the estimated age of 2.24[4] billion years old, it is an evolved K-type giant star with a stellar classification of K0/1 III.[3] Lambda Pictoris has 2.2 times the mass of the Sun and is radiating 112 times the Sun's luminosity from its photosphere at an effective temperature of 4,581 K.[4]

  1. ^ a b c d e Cite error: The named reference vanLeeuwen2007 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference Cousins1969 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference houk1978 was invoked but never defined (see the help page).
  4. ^ a b c d e f g Cite error: The named reference Luck2015 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference Alves2015 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference Eggleton2008 was invoked but never defined (see the help page).

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Lambda Pictoris

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planetary systems. The first exocomets were detected in 1987 around Beta Pictoris, a very young A-type main-sequence star. There are now a total of 11 stars...

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List of directly imaged exoplanets

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the Sun. About 107,200 years ago, it made a close approach to the Beta Pictoris system. The estimated separation of the two stars at this time was around...

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hemisphere for the 1908 Revised Harvard Photometry catalogue. The Pole Star and Lambda Ursae Minoris were used for the northern hemisphere. It was then noted that...

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List of brightest natural objects in the sky

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Leporis Star 3.29 Iota Draconis Star Suspected variable star 3.30 Alpha Pictoris Star 3.30 Beta Phoenicis Binary star system 3.30 Xi Puppis Triple star...

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Protoplanetary disk

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stars—most of which have ages in the range of ~10 million years (e.g. Beta Pictoris, 51 Ophiuchi) to billions of years (e.g. Tau Ceti). These systems are usually...

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Stellar kinematics

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protoplanetary disks, such as TW Hydrae or directly imaged exoplanets, such as Beta Pictoris b or GU Psc b. A stellar stream is an association of stars orbiting a galaxy...

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Thuban

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Enclosure, refers to an asterism consisting of Alpha Draconis, Kappa Draconis, Lambda Draconis, 24 Ursae Majoris, 43 Camelopardalis, Alpha Camelopardalis and...

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Pole star

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axes are oriented differently. (See Poles of astronomical bodies.) Alpha Pictoris is the south pole star of Mercury while Omicron Draconis is its north star...

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Brown dwarf

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Vertical Cloud Structure of a Young Low-mass Brown Dwarf, an Analog to the β-Pictoris b Directly Imaged Exoplanet, through Keck I/MOSFIRE Spectrophotometric...

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Main sequence

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080 10,800 Alpha Coronae Borealis A A5 01.7 002.1 000,020 08,620 Beta Pictoris F0 01.3 001.7 000,006 07,240 Gamma Virginis F5 01.2 001.3 000,002.5 06...

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Vega

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scandium below 10%. The unusually low metallicity of Vega makes it a weak Lambda Boötis star. However, the reason for the existence of such chemically peculiar...

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Alpha Circini

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Circini is a candidate member of a stellar kinematic group known as the Beta Pictoris moving group. This group shares a common origin and has an estimated age...

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List of resolved circumstellar disks

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Olofsson, Göran; Liseau, René (2021-02-01). "The far reaches of the β Pictoris debris disk". Astronomy and Astrophysics. 646: A132. arXiv:2101.06281....

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List of brown dwarfs

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Cancri Cancer 09h 12m 14.69s 14°  59 ′  39.6″ 6.77 66 L8 CD 880 2001 AB Pictoris Pictor 06h 19s −58° 03′ 15″ 9.16 66.6 K2V b 13.5 275 2005 CD−33°7795 Hydra...

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