# HD 114613

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Star in the constellation Centaurus

HD 114613 Location of HD 114613 (circled) Observation data Epoch J2000.0 Equinox J2000.0 Constellation Centaurus[1] Right ascension 13h 12m 03.18430s[2] Declination −37° 48′ 10.8799″[2] Apparent magnitude (V) 4.852±0.011[3] Characteristics Evolutionary stage subgiant[2] Spectral type G4 IV[4] B−V color index 0.659±0.020[3] Astrometry Radial velocity (Rv) −13.03±0.13[2] km/s Proper motion (μ) RA: −382.409 mas/yr[2] Dec.: −46.147 mas/yr[2] Parallax (π) 48.8691±0.1058 mas[2] Distance 66.7 ± 0.1 ly (20.46 ± 0.04 pc) Absolute magnitude (MV) 3.29[5] Details Mass 1.25±0.03[6] M☉ Radius 2.01±0.06[6] R☉ Luminosity 4.057±0.014[7] L☉ Surface gravity (log g) 3.97±0.02[7] cgs Temperature 5,729±17[7] K Metallicity [Fe/H] 0.19±0.01[7] dex Rotation 34.1±3.5 d[8] Rotational velocity (v sin i) 2.4±0.5[9] km/s Age 5.20±0.24[6] Gyr Other designations CD−37°8437, FK5 3051, GJ 501.2, HD 114613, HIP 64408, HR 4979, SAO 204227 Database references SIMBAD data

**HD 114613** (**Gliese 501.2**) is a fifth magnitude yellow [subgiant](/source/Subgiant) star that lies 66.7 [light-years](/source/Light-year) (20.5 [parsecs](/source/Parsec)) away in the [constellation](/source/Constellation) of [Centaurus](/source/Centaurus).

## Stellar characteristics

HD 114613 lies about two degrees south-east of [Iota Centauri](/source/Iota_Centauri), towards the middle of Centaurus. Though it is fairly easily observable with the naked eye, the star does not have a [Bayer](/source/Bayer_designation) or [Flamsteed](/source/Flamsteed_designation) designation as the constellation of Centaurus contains many brighter stars.

The B-V colour and spectroscopic temperature of HD 114613 correspond with its spectral type of G4. This means that the star is only slightly cooler than the Sun, and has the yellow hue typical of G-type stars. On the [Hertzsprung-Russell diagram](/source/Hertzsprung-Russell_diagram) (left) the star lies significantly above the main sequence, and is close to the [subgiant](/source/Subgiant) branch; this means that HD 114613 has depleted the hydrogen in its core through [nuclear fusion](/source/Nuclear_fusion), and is increasing in radius while decreasing in temperature as it moves towards the giant branch.

As HD 114613 is ending hydrogen fusion, the star must be fairly old. When combined with a spectroscopically derived mass of 1.25 ± 0.03 M☉ and a surface gravity of log 3.95 ± 0.03 g the implied age of the star is 5.20 ± 0.24 billion years,[6] making it slightly older than the Sun. Though stellar metallicities typically decrease with increasing stellar age, within the age range of the [thin disk](/source/Thin_disk) a wide range of metallicities are common; HD 114613's high iron abundance of 0.19 ± 0.01 dex (155 ± 4% of the solar abundance) is therefore not unusual. The rate of giant planet occurrence for Fe/H = 0.2 dex stars is about 15%,[10] which makes it fairly unsurprising that the star could host a giant planet.

HD 114613 has a magnetic cycle with a period of 897 ± 61 days, about four-and-a-half times shorter than the [Solar magnetic cycle](/source/Solar_cycle) and one of the shortest magnetic cycles known.[8]

## Planet searches

Being bright and solar-type, HD 114613 is an attractive target for [radial velocity (RV)-based planet searches](/source/Doppler_spectroscopy).

HD 114613 was one of the 37 targets of the first RV-based planet search in the southern hemisphere, the [ESO](/source/ESO)-CES survey that spanned between 1992 and 1998.[11] This survey did not detect any companion with several Jovian masses out to a few AU. An extension of this survey to the [HARPS](/source/High_Accuracy_Radial_Velocity_Planet_Searcher) spectrograph provides further constraint, suggesting that there are no Jupiter-mass companions out to about 5 AU.[12]

HD 114613 is included in the samples of the ESO-[CORALIE](/source/CORALIE_spectrograph)[10] and [AAT](/source/Anglo-Australian_Telescope)-UCLES[13] planet searches that both began in 1998. Seemingly finding the star to be RV-stable and suitable for higher precision, HD 114613 was included in a subset of the CORALIE sample that became the sample of the ESO-HARPS high precision planet search that began in 2004,[7] while the star was elevated in importance in the AAT sample in 2005.[14][15] Though apparently not included in its main sample, HD 114613 is included in the sample of the [Keck](/source/W._M._Keck_Observatory)-HIRES Eta-Earth low-mass planet search that also began in 2004.[16]

In Wittenmyer et al. 2012,[17] HD 114613 is indicated to be a low-mass planet host. Though this references a Tuomi et al. 2012 (*Tuomi, M., et al. 2012, MNRAS, submitted*), no such paper was published that year. More recently, in a Tuomi et al. 2013,[18] [Tau Ceti](/source/Tau_Ceti) is noted to have a similar activity index distribution to HD 114613. Again, a Tuomi et al. 2012 is referenced, though somewhat more completely (*Tuomi, M., Jones, H. R. A., Jenkins, J. S., et al. 2012, MNRAS, submitted*). No paper announcing HD 114613 as a *low-mass* planet host has been published as of 2014.

However, that does not mean the star is not a planet host. Wittenmyer et al. (2014) found HD 114613 to show a moderate-amplitude variation in its radial velocity with a period of 10.5 years, indicative of a long-period companion.[19] The radial velocity semi-amplitude of 5.5 m/s translates to a planet with a minimum mass about half a Jupiter mass. The planet has an intermediate orbital eccentricity of 0.25, which means that it can be somewhat loosely considered a Jupiter analogue.

A study in 2023 did not detect this radial velocity signal, but instead detected a signal with a longer period of about 18 years, which shows indications of originating from a long-period magnetic activity cycle. This suggests that the previously detected signal is not planetary, but is related to stellar activity.[20]: 28[20]: 44

## References

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v t e Constellation of Centaurus List of stars in Centaurus Centaurus in Chinese astronomy Stars Bayer α A (Rigil Kentaurus) B (Toliman) C (Proxima Centauri) β (Hadar) γ δ ε ζ (Leepwal) η θ (Menkent) ι (Kulou) κ λ μ ν (Heng) ξ1 ξ2 ο1 ο2 π ρ σ τ υ1 υ2 φ χ ψ x1 x2 C3 D E F G H J K M N Q Flamsteed 1 (i) 2 (g) 3 (k) 4 (h) Variable R T V Y RR SV SX BV DY UY V346 V553 V744 V752 V761 (a) V763 (C1) V766 V779 (Krzemiński's star) V803 V810 V816 (Przybylski's Star) V831 V842 V885 V886 V863 V1032 V1369 V1400 V1935 HR 4460 (A) 4466 (C2) 4499 4522 4523 4537 (j) 4546 (B) 4721 4748 (u) 4796 4817 (l) 4831 (w) 4874 (p) 4888 (e) 4889 (n) 4940 (f) 4979 4989 5006 (r) 5041 (m) 5089 (d) 5174 (z) 5222 (y) 5224 5241 5297 5358 (v) 5371 5471 (b) 5485 (c1) 5489 (c2) HD 97413 98176 100453 101581 101930 102117 (Uklun) 103197 107914 108236 109749 110113 113538 113766 114386 114729 115600 116434 (Matza) 117207 117618 (Dofida) 117939 120411 121228 121504 124448 (Popper's Star) 125072 125595 131399 Other 2MASS J1126−5003 2M1207 Gaia BH2 HD 131399 Ab PSR B1259−63 PSR J1311−3430 TOI-763 WASP-15 (Nyamien) WASP-41 WASP-42 WASP-167/KELT-13 Exoplanets 2M1207b b Centauri b HD 101930 b HD 102117 b (Leklsullun) HD 103197 b HD 109749 b HD 113538 b c HD 114386 b HD 114729 b HD 117207 b HD 117618 b (Noifasui) HD 121504 b HIP 65426 b (Najsakopajk) HIP 67522 b NGTS-13b Proxima Centauri b c d WASP-15b (Asye) Star clusters NGC 3766 4230 4507 5281 5286 5316 5460 5617 5662 Other IC 2944 ω Centauri Scorpius–Centaurus association Stock 16 Nebulae NGC 3918 5307 Other Boomerang Nebula Fleming 1 G292.0+1.8 G306.3-0.9 Gum 41 IC 2944 IRAS 13208−6020 RCW 79 RCW 86 Southern Crab Nebula SuWt 2 Galaxies NGC 3557 3568 3749 3783 4444 4603 4622 4650A 4683 4696 4706 4709 4729 4730 4743 4744 4909 4930 4945 4976 5011 A 5026 5064 5082 5090 5091 5102 5114 5121 5128 (Centaurus A) 5161 5206 5253 5266 5291 5398 5408 5419 5483 5516 Other ESO 269-57 ESO 325-4 ESO 383-76 ESO 444-46 Fourcade-Figueroa Object IC 3370 IC 4214 IC 4329A IRAS 13224−3809 J1144−4308 LEDA 677373 PKS 1144−379 PKS 1353−341 PKS 1424−418 Galaxy clusters Abell S740 Centaurus Cluster Shapley Supercluster Astronomical events GW190521 SN 185 SN 1895B (Z) SN 1972E SN 1986G J1407b SN 2019so Category

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Adapted from the Wikipedia article [HD 114613](https://en.wikipedia.org/wiki/HD_114613) by Wikipedia contributors ([contributor history](https://en.wikipedia.org/wiki/HD_114613?action=history)). Available under [Creative Commons Attribution-ShareAlike 4.0 International](https://creativecommons.org/licenses/by-sa/4.0/). Changes may have been made.