Jump to content

HIP 5158

Coordinates: Sky map 01h 06m 02.0482s, −22° 27′ 11.350″
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Citation bot (talk | contribs) at 05:15, 2 December 2020 (Add: year, s2cid, pages, volume, journal, doi, author pars. 1-3. Removed parameters. Formatted dashes. Some additions/deletions were actually parameter name changes. | You can use this bot yourself. Report bugs here. | Suggested by Abductive | Category:2MASS objects | via #UCB_Category 456/509). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

HIP 5158
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 01h 06m 02.05s[1]
Declination –22° 27′ 11.3″[1]
Apparent magnitude (V) 10.21
Characteristics
Spectral type K5V
Apparent magnitude (B) 11.29
B−V color index 1.08
Astrometry
Radial velocity (Rv)15.28 km/s
Proper motion (μ) RA: 203.899±0.087[2] mas/yr
Dec.: -106.761±0.065[2] mas/yr
Parallax (π)19.3500 ± 0.0388 mas[2]
Distance168.6 ± 0.3 ly
(51.7 ± 0.1 pc)
Absolute magnitude (MV)6.95
Details
Mass0.780 ± 0.021[3] M
Radius0.71 ± 0.12 R
Luminosity0.11[3] L
Surface gravity (log g)4.37 ± 0.20[3] cgs
Temperature4962 ± 89[3] K
Metallicity[Fe/H] = 0.10 ± 0.07[3]
Age4.9 ± 3.7[4] Gyr
Rotation1.57
(42.3 days)[3]
Other designations
CD–23°395, LTT 617, NLTT 3632, PPM 243575, SAO 166798, 2MASS J01060202-2227111, DR2 2351405057377686272
Database references
SIMBADdata
Exoplanet Archivedata

HIP 5158 is a 10th magnitude K-type main sequence star located approximately 130 light years away in the constellation Cetus. This star is smaller, cooler, fainter, and less massive than our Sun, but it is more metal rich, having concentration of heavy elements equal to 125% of solar abundance.

Planetary system

In 2009, a gas giant planet was found in orbit around the star. The quadratic drift in the radial velocities did indicate the presence of an additional outer planet in the system,[3] which was confirmed in 2011 as brown dwarf HIP 5158 c.[5]

The HIP 5158 planetary system[3][5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥1.42 MJ 0.89 345.72 ± 5.37 0.52 ± 0.08
c ≥15.04 MJ 7.7±1.88 9018±3181 0.14±0.1

See also

References

  1. ^ a b 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. Vizier catalog entry
  2. ^ a b c CD-23 395 -- High proper-motion Star
  3. ^ a b c d e f g h Lo Curto, G.; et al. (2015). "The HARPS search for southern extra-solar planets. XXII. Multiple planet systems from the HARPS volume limited sample". Astronomy and Astrophysics. 512. A48. arXiv:1411.7048. Bibcode:2010A&A...512A..48L. doi:10.1051/0004-6361/200913523.
  4. ^ Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951. S2CID 54555839.
  5. ^ a b Feroz, F.; Balan, S. T.; Hobson, M. P. (2011), "Bayesian evidence for two companions orbiting HIP 5158", Monthly Notices of the Royal Astronomical Society: Letters, 416: L104–L108, arXiv:1105.1150, doi:10.1111/j.1745-3933.2011.01109.x, S2CID 118517956