Astronomy:HD 41004
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Pictor |
| Right ascension | 05h 59m 49.64736s[1] |
| Declination | −48° 14′ 22.8058″[1] |
| Apparent magnitude (V) | 8.65[2] (8.82 + 12.51)[3] |
| Characteristics | |
| Spectral type | K1V + M2V[4] |
| B−V color index | 0.887±0.013[2] |
| Astrometry | |
| Radial velocity (Rv) | +42.5±0.5[2] km/s |
| Proper motion (μ) | RA: −41.520±0.485[1] mas/yr Dec.: +59.652±0.556[1] mas/yr |
| Parallax (π) | 24.0437 ± 0.2635[1] mas |
| Distance | 136 ± 1 ly (41.6 ± 0.5 pc) |
| Absolute magnitude (MV) | 5.60[2] |
| Details[5] | |
| A | |
| Mass | 0.89±0.07 M☉ |
| Radius | 1.04+0.02 −0.03[1] R☉ |
| Luminosity | 0.629±0.008[1] L☉ |
| Surface gravity (log g) | 4.34±0.11 cgs |
| Temperature | 5,255±52 K |
| Metallicity [Fe/H] | 0.15±0.03 dex |
| Rotational velocity (v sin i) | 1.0±1.2[6] km/s |
| B | |
| Mass | 0.4[7] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 41004 is a visual binary[4] star system in the southern constellation of Pictor. It is too faint to be visible to the naked eye, having a combined apparent visual magnitude of 8.65.[2] The two components have a magnitude difference of 3.7, and share a common proper motion[4] with an angular separation of 0.30″, as of 2018.[3] The distance to this system is approximately 136 light years based on parallax.[1] It is drifting further away from the Sun with a radial velocity of +42.5 km/s, having come to within 44.5 ly some 831,000 years ago.[2]
The primary, component A, is a K-type main-sequence star with a stellar classification of K1V[4] and a visual magnitude of 8.82.[3] Torres et al. (2006) classed it as a K1IV star,[6] suggesting it is a subgiant star that is evolving off the main sequence. It has 89%[4] of the mass of the Sun and 104%[1] of the Sun's radius. The star is radiating 63%[1] of the Sun's luminosity from its photosphere at an effective temperature of 5,255 K.[4] Its smaller companion, designated component B, is a red dwarf with spectral type M2V[4] and apparent magnitude 12.33. It has a projected separation of 23 astronomical unit|AU from the primary.[4]
Companions
A planet, HD 41004 Ab, was discovered by Zucker et al., in but not published until 2004. It has a mass >2.56 times that of Jupiter. It orbits the primary star at a separation of 1.70 astronomical units, taking 2.64 years with a high eccentricity of 0.74.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | >2.56 MJ | 1.70 | 963 | 0.74 | — | — |
| Discovery | |
|---|---|
| Discovered by | Zucker et al. |
| Discovery date | 2004 |
| radial velocity | |
| Orbital characteristics | |
| Periastron | 0.0163 AU |
| Apoastron | 0.0191 AU |
| 0.0177 AU | |
| Eccentricity | 0.081±0.012 |
| Orbital period | 1.3283±1.2e-5 d |
| Average Orbital speed | 145 km/s |
| Angular distance | 0.411 mas |
| 178.5±7.8° | |
| |{{{apsis}}}|helion}} | 2452434.88±0.0029 JD |
| Semi-amplitude | 6114±71 m/s |
| Physical characteristics | |
| Mass | ~16 MJ (most probable)[4] < ~25 MJ[4] |
HD 41004 Bb is a brown dwarf that at the time of the discovery was orbiting closer to the secondary star than any known extrasolar planet or brown dwarf (a=0.0177 AU), at only 145 km/s, because of its low-mass parent star, taking 1.3 days. Its orbit is circular despite the gravitational effect of HD 41004 A because of the tidal effect of the nearby star HD 41004 B.[9] A search for cyclotron radiation from the magnetosphere of Bb in 2020 did not find any, indicating the planet is either weakly magnetized, or the emission cone did not point to Earth at the time of observation.[10]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 3.2 Mason, B. D. et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal 122 (6): 3466. doi:10.1086/323920. Bibcode: 2001AJ....122.3466M. http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=B/wds. Retrieved 2015-07-22.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 4.8 4.9 Zucker, S. et al. (November 2004). "Multi-order TODCOR: Application to observations taken with the CORALIE echelle spectrograph. II. A planet in the system HD 41004". Astronomy and Astrophysics 426 (2): 695–698. doi:10.1051/0004-6361:20040384. Bibcode: 2004A&A...426..695Z.
- ↑ Sousa, S. G. et al. (November 2018). "SWEET-Cat updated. New homogenous spectroscopic parameters". Astronomy & Astrophysics 620: 13. doi:10.1051/0004-6361/201833350. A58. Bibcode: 2018A&A...620A..58S.
- ↑ 6.0 6.1 Torres, C. A. O. et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics 460 (3): 695–708. doi:10.1051/0004-6361:20065602. Bibcode: 2006A&A...460..695T.
- ↑ Quarles, Billy; Li, Gongjie; Kostov, Veselin; Haghighipour, Nader (2020), "Orbital Stability of Circumstellar Planets in Binary Systems", The Astronomical Journal 159 (3): 80, doi:10.3847/1538-3881/ab64fa, Bibcode: 2020AJ....159...80Q
- ↑ "HD 41004". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+41004.
- ↑ Santos, N. C. et al. (2002). "The CORALIE survey for southern extra-solar planets. IX. A 1.3-day period brown dwarf disguised as a planet". Astronomy and Astrophysics 392 (1): 215–229. doi:10.1051/0004-6361:20020876. Bibcode: 2002A&A...392..215S.
- ↑ Narang, Mayank; Manoj, P.; Ishwara Chandra, C. H.; Lazio, Joseph; Henning, Thomas; Tamura, Motohide; Mathew, Blesson; Ujwal, Nitish et al. (2021), "In search of radio emission from exoplanets: GMRT observations of the binary system HD 41004", Monthly Notices of the Royal Astronomical Society 500 (4): 4818–4826, doi:10.1093/mnras/staa3565
External links
- "HD 41004 A". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=HD+41004+A. Retrieved 2008-07-21.
- "HD 41004 B". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=HD+41004+B. Retrieved 2008-07-21.
Coordinates: 
05h 59m 49.64s, −48° 14′ 22.89″
 |  |
