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HD 6434 information


HD 6434 / Nenque
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Phoenix[1]
Right ascension 01h 04m 40.15037s[2]
Declination –39° 29′ 17.5856″[2]
Apparent magnitude (V) 7.71±0.12[3]
Characteristics
Spectral type G2/G3V[4]
B−V color index 0.61±0.01[3]
Astrometry
Radial velocity (Rv)+22.92±0.14[2] km/s
Proper motion (μ) RA: −170.124±0.106[2] mas/yr
Dec.: −527.851±0.078[2] mas/yr
Parallax (π)23.5794 ± 0.0417 mas[2]
Distance138.3 ± 0.2 ly
(42.41 ± 0.08 pc)
Absolute magnitude (MV)4.69[5]
Details[6]
Mass0.83±0.03 M
Radius1.029±0.004 R
Luminosity1.208±0.004 L
Surface gravity (log g)4.31±0.01 cgs
Temperature5,907±71 K
Metallicity [Fe/H]−0.48±0.05[3] dex
Rotation18.6 d[7]
Rotational velocity (v sin i)2.2±0.5[3] km/s
Age12.2±0.8 Gyr
Other designations
CD–40°239, GJ 9037, HD 6434, HIP 5054, SAO 192911, LFT 102, LHS 1188, LPM 57, LTT 610, GCRV 51158, 2MASS J01044015-3929173[8]
Database references
SIMBADdata
ARICNSdata

HD 6434 is a star in the southern constellation of Phoenix. Yellow dwarfs such as this are not very luminous, so at a distance of 138[2] light years it is not visible to the unaided eye. However, with binoculars it is readily visible under ideal observing conditions, having an apparent visual magnitude of 7.71.[3] The star is drifting further from the Sun with a radial velocity of +23 km/s.[2]

The star HD 6434 is named Nenque. The name was selected in the NameExoWorlds campaign by Ecuador, during the 100th anniversary of the IAU. Nenque means the Sun in the language spoken by the Indigenous Waorani tribes.[9][10]

This object is a Sun-like G-type main-sequence star with a stellar classification of G2/G3V.[4] It is an ancient population II[11] star with an estimated age of 12[6] billion years, and is one of the most metal-deficient stars known to host a planet.[3] This star is spinning at a leisurely rate with a projected rotational velocity of 2.2 km/s.[3] It has 88% of the mass of the Sun but is nearly the same size. HD 6434 is radiating 1.2 times the luminosity of the Sun from its photosphere at an effective temperature of 5,907 K.[6]

  1. ^ Cite error: The named reference Roman1987 was invoked but never defined (see the help page).
  2. ^ a b c d e f g h Cite error: The named reference Gaia DR2 was invoked but never defined (see the help page).
  3. ^ a b c d e f g Cite error: The named reference Hinkel2015 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference White2007 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Barbieri2002 was invoked but never defined (see the help page).
  6. ^ a b c Cite error: The named reference Bonfanti2015 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference Mayor2004 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  9. ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
  10. ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  11. ^ Cite error: The named reference Fuhrmann2019 was invoked but never defined (see the help page).

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HD 6434

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HD 6434 is a star in the southern constellation of Phoenix. Yellow dwarfs such as this are not very luminous, so at a distance of 138 light years it is...

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HD 6434 b

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HD 6434 b is an extrasolar planet orbiting the star HD 6434. It has a minimum mass about half that of Jupiter. It orbits the star very close, over 2.5...

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List of proper names of stars

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/ˈnɛmbəs/ Phoenix HD 6434 Nenque IAU new 2019 Ecuadorian proposal; means 'the Sun' in the language of the Waorani tribes. /ˈnɛŋkiː/ Auriga HD 49674 Nervia...

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List of proper names of exoplanets

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language HD 6434 (Nenque) 0.39 21.998 0.14 radial vel. 2000 131.5 0.79 5835 2019 NameExoWorlds Ecuador Cayahuanca "rock looking at the stars" in Nahuatl HD 52265...

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List of stars in Phoenix

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Hipparcos and Tycho Catalogues". Retrieved 2006-12-26. Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26. Roman, N...

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Xi Phoenicis

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N.; et al. (January 2012), "Multi-element Doppler imaging of the CP2 star HD 3980", Astronomy & Astrophysics, 537: 10, arXiv:1303.2703, Bibcode:2012A&A...

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Phi Phoenicis

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inhomogeneities in late B-type stars with Hg and Mn peculiarity. I. Spot evolution in HD 11753 on short and long time scales", Astronomy & Astrophysics, 553: 16, arXiv:1302...

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List of exoplanets detected by radial velocity

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NGC 6231

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O-type stars. NGC 6231 also includes three Wolf-Rayet stars: HD 151932, HD 152270, and HD 152408. The cluster was discovered by Giovanni Batista Hodierna...

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Messier 23

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NGC 6383

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NGC 6122

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WISE 0458+6434 is the first ultra-cool brown dwarf (green dot) discovered by WISE. The green and blue comes from infrared wavelengths mapped to visible...

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NGC 6357

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NGC 6193

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Gosset, E. (2013). "Three-dimensional orbits of the triple-O stellar system HD 150136". Astronomy & Astrophysics. 553: A131. arXiv:1304.3457. Bibcode:2013A&A...

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Messier 9

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NGC 6002

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Hydrogen isotope biogeochemistry

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NGC 6309

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NGC 6284

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NGC 6086

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NGC 6085

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