Astronomy:HD 73267

From HandWiki
Short description: Star in the constellation Pyxis
HD 73267
Observation data
Equinox J2000.0]] (ICRS)
Constellation Pyxis
Right ascension  08h 36m 17.77623s[1]
Declination −34° 27′ 35.9196″[1]
Apparent magnitude (V) 8.889[2]
Characteristics
Spectral type G5V[3]
Apparent magnitude (J) 7.493±0.023[4]
Apparent magnitude (H) 7.126±0.031[4]
Apparent magnitude (K) 7.062±0.023[4]
B−V color index 0.827±0.003[2]
Astrometry
Radial velocity (Rv)+51.836±0.0011[5] km/s
Proper motion (μ) RA: −106.336±0.012[1] mas/yr
Dec.: 123.293±0.013[1] mas/yr
Parallax (π)19.9362 ± 0.0130[1] mas
Distance163.6 ± 0.1 ly
(50.16 ± 0.03 pc)
Absolute magnitude (MV)5.24[6]
Details[2]
Mass0.897±0.019 M☉
Radius0.909±0.033 R☉
Luminosity0.783±0.09[3] L☉
Surface gravity (log g)74.447±0.035 cgs
Temperature5,387±10 K
Metallicity [Fe/H]0.07±0.04 dex
Rotation~43 d
Rotational velocity (v sin i)1.65[3] km/s
Age8.140±3.505 Gyr
Other designations
CD−34°5039, HD 73267, HIP 42202, SAO 199418, PPM 285436, NLTT 19895, GSC 07144-01553, 2MASS J08361779-3427358[7]
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia		data

HD 73267 is a star in the southern constellation Pyxis, near the western constellation border with Puppis. It has an apparent visual magnitude of 8.889[2] and can be viewed with a small telescope. The distance to HD 73267 is 164 light years based on parallax, and it is drifting further away with a radial velocity of +51.8 km/s.[5] It has an absolute magnitude of 5.24.[6]

This object is a G-type main-sequence star with a stellar classification of G5V.[3] It is roughly eight billion years old with a near-solar metallicity and is spinning with a projected rotational velocity of 1.65 km/s,[3] giving it a rotation period of around 33 days. The star has 90% of the mass and size of the Sun.[2] It is radiating 78%[3] of the Sun's luminosity from its photosphere at an effective temperature of 5387 K.[2]

Planetary system

In October 2008, a candidate planet was discovered orbiting this star. This object was detected using the radial velocity method by search programs conducted using the HARPS spectrograph.[3] Subsequent analysis of collected data suggests the presence of an additional long-period planet in the system with at least 83% of the mass of Jupiter.[2] In 2022, the inclination and true mass of HD 73267 b were measured, and the presence of a second planet was confirmed using a combination of radial velocity and astrometry.[8]

The HD 73267 planetary system[8]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(years) 		Eccentricity Inclination Radius
b 4.158+0.681
−0.519 MJ 		2.229+0.091
−0.100 		3.444+0.001
−0.002 		0.261±0.004 130.843+7.614
−7.660° 		—
c 5.131+0.912
−0.282 MJ 		12.688+0.631
−0.812 		46.740+2.150
−2.977 		0.089+0.023
−0.022 		91.849+18.586
−24.998° 		—

See also

  • List of extrasolar planets

References

  1. ↑ 1.0 1.1 1.2 1.3 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Barbato, D. et al. (August 2018). "Exploring the realm of scaled solar system analogues with HARPS". Astronomy & Astrophysics 615: 21. doi:10.1051/0004-6361/201832791. A175. Bibcode: 2018A&A...615A.175B. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 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. doi:10.1051/0004-6361:200810941. Bibcode: 2009A&A...496..513M. http://www.aanda.org/articles/aa/full_html/2009/11/aa10941-08/aa10941-08.html. 
  4. ↑ 4.0 4.1 4.2 Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E. et al. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". CDS/ADC Collection of Electronic Catalogues 2246: II/246. Bibcode: 2003yCat.2246....0C. http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=II/246. 
  5. ↑ 5.0 5.1 Soubiran, C. et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars". Astronomy and Astrophysics 616: A7. doi:10.1051/0004-6361/201832795. Bibcode: 2018A&A...616A...7S. 
  6. ↑ 6.0 6.1 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A 
  7. ↑ "HD 73267". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+73267. 
  8. ↑ 8.0 8.1 Feng, Fabo et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series 262 (21): 21. doi:10.3847/1538-4365/ac7e57. Bibcode: 2022ApJS..262...21F. 

External links

Coordinates: Sky map 08h 36m 17.776s, −34° 27′ 35.92″



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:HD_73267&oldid=3426041"