HD 73534
Today we want to talk about HD 73534. It is a topic that interests us all, since HD 73534 has a great impact on our lives. Throughout history, HD 73534 has been the subject of study, debate and controversy. Today, HD 73534 is still relevant and continues to generate interest in different areas. In this article, we will explore different aspects related to HD 73534, from its origin to its influence on today's society. We hope to offer an interesting and enriching perspective on HD 73534 and contribute to the debate around this topic.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cancer |
| Right ascension | 08h 39m 15.803s[1] |
| Declination | +12° 57′ 37.35″[1] |
| Apparent magnitude (V) | 8.23[2] |
| Characteristics | |
| Spectral type | G5 IV[2] |
| Apparent magnitude (B) | 9.192[3] |
| Apparent magnitude (J) | 6.524±0.018[3] |
| Apparent magnitude (H) | 6.072±0.020[3] |
| Apparent magnitude (K) | 5.962±0.026[3] |
| B−V color index | 0.962±0.021[3] |
| Astrometry | |
| Radial velocity (Rv) | +9.76±0.13[1] km/s |
| Proper motion (μ) | RA: −114.147 mas/yr[1] Dec.: −93.787 mas/yr[1] |
| Parallax (π) | 11.9576±0.0254 mas[1] |
| Distance | 272.8 ± 0.6 ly (83.6 ± 0.2 pc) |
| Absolute bolometric magnitude (Mbol) | 3.42[2] |
| Details[2] | |
| Mass | 1.228±0.060 M☉ |
| Radius | 2.39±0.16 R☉ |
| Luminosity | 3.33±0.43 L☉ |
| Surface gravity (log g) | 3.780±0.060 cgs |
| Temperature | 5,041±44 K |
| Metallicity | 0.232±0.030 dex |
| Rotation | ~53 d |
| Rotational velocity (v sin i) | < 1.0 km/s |
| Age | 7.1±0.8[4] Gyr |
| Other designations | |
| Gakyid, BD+13°1956, HD 73534, HIP 42446, SAO 98004, PPM 125542[5] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HD 73534 is star with an orbiting exoplanet companion in the northern constellation of Cancer. With an apparent visual magnitude of 8.23,[2] it is too faint to be visible to the naked eye. The distance to this system is 273 light-years based on parallax measurements, and it is drifting further away with a heliocentric radial velocity of +10 km/s.[1]
The star HD 73534 has the proper name Gakyid. The name was selected by Bhutan during the 100th anniversary of the IAU as part of the IAU's NameExoWorlds project. Gakyid means happiness. The planet HD 73534 b is named Drukyul, which means 'land of the thunder dragon', the native name for Bhutan.[6][7]
This is a G-type subgiant star with a stellar classification of G5 IV. It has consumed the hydrogen at its core and begun to evolve off the main sequence, which is why it is much more luminous than the Sun. The star has a negligible level of magnetic activity in its chromosphere. It has 23% more mass than the Sun, and has expanded to 2.4 times the Sun's radius. The star is radiating 3.3 times the luminosity of the Sun from its photosphere at an effective temperature of 5,041 K.[2] It is roughly 7 billion[4] years old and is spinning slowly with a rotation period of around 53 days.[2]
In August 2009, it was announced that an exoplanet had been discovered using Doppler spectroscopy.[2] It is the first planetary system discovered in Cancer since that of 55 Cancri in April 1996, and the sixth planet, as 55 Cancri has five known planets.[citation needed]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥1.01±0.21 MJ | 2.95±0.22 | 1721±36 | 0 (fixed) | — | — |
See also
References
- ^ a b c d e f 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 f g h Valenti, Jeff A.; et al. (2009). "Two Exoplanets Discovered at Keck Observatory". The Astrophysical Journal. 702 (2): 989–997. arXiv:0908.1612. Bibcode:2009ApJ...702..989V. doi:10.1088/0004-637X/702/2/989. S2CID 16707072.
- ^ 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 Bonfanti, A.; Ortolani, S.; Nascimbeni, V. (2016). "Age consistency between exoplanet hosts and field stars". Astronomy & Astrophysics. 585: 14. arXiv:1511.01744. Bibcode:2016A&A...585A...5B. doi:10.1051/0004-6361/201527297. S2CID 53971692. A5.
- ^ "HD 73534". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-14.
{{cite web}}: CS1 maint: postscript (link) - ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
- ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
- ^ Ment, Kristo; et al. (2018). "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810". The Astronomical Journal. 156 (5). 213. arXiv:1809.01228. Bibcode:2018AJ....156..213M. doi:10.3847/1538-3881/aae1f5. S2CID 119243619.
