HD 2039

HD 2039 is a G-type star about 86 parsecs (roughly 280 light-years) from the Sun in the southern constellation Phoenix, whose one known confirmed planet, HD 2039 b, is a massive, highly eccentric gas giant discovered by the Anglo-Australian Planet Search in 2002.^{1 • 2}

The star

HD 2039 is cataloged as a G2/G3 IV-V star, meaning a solar-type star slightly evolved off the main sequence toward the subgiant branch.³ The NASA Exoplanet Archive lists an effective temperature of 5941 K and a stellar radius of 1.32 solar radii, with the stellar mass taken from an evolutionary-track mass in Ghezzi et al. 2010.¹ At visual magnitude 9.00 it is too faint for naked-eye viewing but accessible to small telescopes.¹

The star is metal-rich relative to the Sun: the Hypatia Catalog value is [Fe/H] = 0.35 ± 0.18 dex, meaning iron abundance about 2.2 times the solar level at face value.¹ This matches how the star was originally chosen. The Anglo-Australian Planet Search added a sub-sample of twenty metal-enriched, faint (V < 9) stars to its main magnitude-limited sample in October 1998, selecting them by Strömgren photometry, and HD 2039 was one of the stars whose enrichment was later confirmed spectroscopically.⁴

Discovery

HD 2039 b was announced in 2002 in a paper by C. G. Tinney, R. Paul Butler, Geoffrey W. Marcy, Hugh R. A. Jones, Alan J. Penny, Chris McCarthy, Brad D. Carter, and Jade Bond of the Anglo-Australian Planet Search, published in The Astrophysical Journal (587, 423, 2003).^{4 • 1} The same paper reported three other planets around the metal-enriched stars HD 73526, HD 76700, and HD 30177.⁴

The detection method was radial velocity: repeated spectra of the star show a periodic Doppler wobble as the unseen companion pulls it around the system barycenter. The archive holds 36 optical radial-velocity points from the Tinney et al. 2003 solution and 41 from the Butler et al. 2006 orbit update.¹

The planet HD 2039 b

HD 2039 b is classified as a gas giant.² Because radial velocity measurements yield only a minimum mass, the product of mass and the unknown orbital inclination, the published solutions give M sin i values of 4.9 ± 1.0 Jupiter masses (Tinney et al. 2003), 6.11 ± 0.82 (Butler et al. 2006), and 6.29 ± 1.16 (Stassun et al. 2017), the last being the value NASA's catalog quotes.^{1 • 2} Its radius has not been measured; NASA lists an estimated 1.14 times Jupiter's radius, and the Open Exoplanet Catalogue gives an estimated equilibrium temperature of 188.3 K.^{2 • 3}

The orbit is both wide and strongly eccentric. The planet completes one revolution in 1120 ± 23 days at a semi-major axis of 2.20 ± 0.06 AU, but with an eccentricity of 0.71 ± 0.05 its distance from the star swings between roughly 0.64 AU at periastron and 3.76 AU at apastron, computed from the archived elements.¹ The velocity semi-amplitude K is 153 ± 22 m/s in the refined solutions.¹ At this distance the planet receives more stellar radiation than Jupiter receives from the Sun, and catalog assessments classify it as not habitable.^{5 • 2}

System context

Only one planet is known in the system; the archive lists 1 confirmed planet and no stellar companions within 30 arcseconds other than a 2MASS point source.¹ The star carries several catalog designations, including HIP 1931, TYC 8468-177-1, SAO 232025, and Gaia DR3 4919009555730599936, and the planet is correspondingly listed under aliases such as HIP 1931 b.^{6 • 3} Published distance estimates differ slightly among catalogs: the Exoplanet Archive gives 85.69 pc from Gaia parallax, the Exoplanet Data Explorer lineage 87.0 pc, and the Open Exoplanet Catalogue 89.8 pc (293 light-years).^{1 • 5 • 3}

References

1. HD 2039 Overview, NASA Exoplanet Archive
2. HD 2039 b, NASA Science Exoplanet Catalog
3. HD 2039 b, Open Exoplanet Catalogue
4. Tinney et al. (2002). Four new planets orbiting somewhat metal-enriched stars. arXiv:astro-ph/0207128
5. HD 2039 b, Exoplanet Kyoto database
6. HD 2039, SIMBAD Astronomical Database

Topic: Encyclopedia › Places and geography › Extraterrestrial places › Exoplanets and nearby star systems › HD catalog stars with planets › Eccentric giant planet hosts

Initially written Oct 21, 2026

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