HD 20868
In the modern world, HD 20868 has gained unprecedented relevance. Since its emergence, HD 20868 has captured the attention of experts and hobbyists alike, becoming a topic of interest to a wide range of people. In this article, we will explore in detail the importance of HD 20868 in various contexts, analyzing its influence in different areas of society. Through in-depth analysis, we will discover how HD 20868 has impacted the way we live, work and relate. Additionally, we will examine the current trends related to HD 20868 and its projection in the future. Without a doubt, HD 20868 has proven to be a topic of global relevance, playing a fundamental role in shaping the contemporary world.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Fornax |
| Right ascension | 03h 20m 42.69371s[1] |
| Declination | −33° 43′ 48.3735″[1] |
| Apparent magnitude (V) | 9.92[2] |
| Characteristics | |
| Spectral type | K3/4 III/V[3] |
| Apparent magnitude (B) | 11.07[4] |
| Apparent magnitude (J) | 8.138±0.032[5] |
| Apparent magnitude (H) | 7.641±0.031[5] |
| Apparent magnitude (K) | 7.543±0.015[5] |
| B−V color index | 1.037±0.005[2] |
| Astrometry | |
| Radial velocity (Rv) | 46.207±0.0011[6] km/s |
| Proper motion (μ) | RA: 292.619 mas/yr[1] Dec.: 96.116 mas/yr[1] |
| Parallax (π) | 20.9561±0.0128 mas[1] |
| Distance | 155.64 ± 0.10 ly (47.72 ± 0.03 pc) |
| Absolute magnitude (MV) | 6.61[2] |
| Details[7] | |
| Mass | 0.76±0.02 M☉ |
| Radius | 0.73±0.01 R☉ |
| Luminosity | 0.255±0.002 L☉ |
| Surface gravity (log g) | 4.59±0.02 cgs |
| Temperature | 4,811±14 K |
| Metallicity | 0.04±0.1 dex |
| Age | 8.4±3.7 Gyr |
| Other designations | |
| Intan, CD−34°1218, HD 20868, HIP 15578, PPM 278952, LTT 1589, 2MASS J03204266-3343484[8] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 20868 is a star in the southern constellation Fornax. With an apparent visual magnitude of 9.92,[2] it is much too dim to be visible to the naked eye. Parallax measurements give a distance estimate of 156 light-years from the Sun. It is drifting further away with a radial velocity of +46.2 km/s,[6] having come to within about 124 ly around 312,000 years ago.[2]
This object is a K-type star with a stellar classification of K3/4 III/V. The luminosity class is poorly constrained; the star's evolutionary status appear to be either main sequence or a giant star.[3] It is around eight billion years old with 76% of the mass of the Sun and 73% of the Sun's radius. It is radiating 25.5% of the luminosity of the Sun from its photosphere at an effective temperature of 4,811 K. The metallicity of the star is near solar, meaning it has about the same abundance of iron as in the Sun. Its properties are consistent with those of a main sequence star.[7]
The star HD 20868 is named Intan. The name was selected in the NameExoWorlds campaign by Malaysia, during the 100th anniversary of the IAU. Intan means diamond in the Malay language.[9][10]
Planetary system
In October 2008 a planet, HD 20868 b, was discovered. This object was detected using the radial velocity method by search programs conducted using the HARPS spectrograph. The orbital solution indicates this is a giant planet in a highly elliptical orbit around the host star.[11]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b / Baiduri | ≥1.99±0.05 MJ | 0.947±0.012 | 380.85±0.09 | 0.75±0.002 | — | — |
See also
References
- ^ a b c d Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b c d e Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.
- ^ a b Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 3. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode:1982mcts.book.....H.
- ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H.
- ^ a b c Cutri, R. M.; et al. (June 2003). 2MASS All Sky Catalog of point sources. NASA/IPAC. Bibcode:2003tmc..book.....C.
- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b 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.
- ^ "HD 20868". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-23.
- ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
- ^ "International Astronomical Union | IAU". www.iau.org. Archived from the original on 2022-12-05. Retrieved 2020-01-02.
- ^ a b Moutou, C.; et al. (2009). "The HARPS search for southern extra-solar planets XVII. Six long-period giant planets around BD -17 0063, HD 20868, HD 73267, HD 131664, HD 145377, HD 153950". Astronomy and Astrophysics. 496 (2): 513–519. arXiv:0810.4662. Bibcode:2009A&A...496..513M. doi:10.1051/0004-6361:200810941. S2CID 116707055.
External links
- "HD 20868". Exoplanets. Archived from the original on 2016-11-30. Retrieved 2009-06-10.
