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HIP 67522

From Wikipedia, the free encyclopedia
G-type main-sequence star
HIP 67522
Observation data
EpochJ2000      EquinoxJ2000
ConstellationCentaurus[1]
Right ascension13h 50m 06.280s[2]
Declination−40° 50′ 08.88″[2]
Apparent magnitude (V)9.80±0.03[3]
Characteristics
Evolutionary stageMain sequence[4]
Spectral typeG0V[5]
Astrometry
Radial velocity (Rv)8.26±2.19[2] km/s
Proper motion (μ)RA: −28.907mas/yr[2]
Dec.: −22.248mas/yr[2]
Parallax (π)8.0170±0.0182 mas[2]
Distance406.8 ± 0.9 ly
(124.7 ± 0.3 pc)
Details[4]
Mass1.22±0.05 M
Radius1.38±0.06 R
Luminosity1.75±0.09 L
Temperature5,675±75 K
Rotation1.418±0.016 days
Rotational velocity (v sin i)54.2±0.7 km/s
Age17±Myr
Other designations
CD−40 8189,HD 120411,HIP 67522,TOI-6551,TIC 166527623[6]
Database references
SIMBADdata
Exoplanet Archivedata

HIP 67522 is aG-type main sequence star located at a distance of 407light-years (125parsecs) away in the constellation ofCentaurus. Itsvisual magnitude of 9.8 makes it much too faint to be seen by the unaided eye. It is slightly larger than the Sun (1.38R) but cooler (5,675 K versus 5,772 K for the Sun). It is also very young being only around 17 million years old. It has two exoplanets orbiting it.[4]

Planetary system

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Twoexoplanets,HIP 67522 b and HIP 67522 c, are known to orbit the star and transit its face as seen from Earth. Their orbital periods are much less thanMercury's 88 days around the Sun, being 6.96 days forb and 14.33 days forc.[7]

Detections of frequent flaring of the star during the transit phase of the innermost planet (HIP 67522b) suggest that interacts with the stars magnetic field producing the high rate of flares.[8]

The HIP 67522 planetary system[9][10]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.0434±0.0031 MJ0.0748+0.0016
−0.0018
6.9594731(22)0.064+0.187
−0.049
89.88+1.08
−0.93
°
0.891+0.021
−0.02
 RJ
c0.1228+0.0042
−0.0053
14.334892(12)0.077+0.195
−0.056
89.2+1.75
−0.64
°
0.708+0.031
−0.032
 RJ

References

[edit]
  1. ^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.
  2. ^abcdeVallenari, 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 atVizieR.
  3. ^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.Bibcode:2000A&A...355L..27H.
  4. ^abcRizzuto, Aaron C.; et al. (13) (22 June 2020)."TESS Hunt for Young and Maturing Exoplanets (THYME). II. A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association".The Astronomical Journal.160 (1): 33.arXiv:2005.00013.Bibcode:2020AJ....160...33R.doi:10.3847/1538-3881/ab94b7.
  5. ^Torres, C. A. O.; Quast, G. R.; Da Silva, L.; de la Reza, R.; Melo, C. H. F.; Sterzik, M. (2006). "Search for associations containing young stars (SACY). I. Sample and searching method".Astronomy and Astrophysics.460 (3): 695.arXiv:astro-ph/0609258.Bibcode:2006A&A...460..695T.doi:10.1051/0004-6361:20065602.
  6. ^"HIP 67522".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2024-12-22.
  7. ^"HIP 67522 Overview".
  8. ^Ilin, Ekaterina; Vedantham, Harish K.; Poppenhäger, Katja; Bloot, Sanne; Callingham, Joseph R.; Brandeker, Alexis; Chakraborty, Hritam (2025-07-02)."Close-in planet induces flares on its host star".Nature:1–4.doi:10.1038/s41586-025-09236-z.ISSN 1476-4687.PMID 40604272.
  9. ^Barber, Madyson G.; Thao, Pa Chia; et al. (September 2024)."TESS Investigation—Demographics of Young Exoplanets (TI-DYE). II. A Second Giant Planet in the 17 Myr System HIP 67522".The Astrophysical Journal Letters.973 (1): L30.arXiv:2407.04763.Bibcode:2024ApJ...973L..30B.doi:10.3847/2041-8213/ad77d9.
  10. ^Thao, Pa Chia; Mann, Andrew W.; Feinstein, Adina D.; Gao, Peter; Thorngren, Daniel; Rotman, Yoav; Welbanks, Luis; Brown, Alexander; Duvvuri, Girish M.; France, Kevin; Longo, Isabella; Sandoval, Angeli; Schneider, P. Christian; Wilson, David J.; Youngblood, Allison (2024-12-01)."The Featherweight Giant: Unraveling the Atmosphere of a 17 Myr Planet with JWST".The Astronomical Journal.168 (6): 297.arXiv:2409.16355.Bibcode:2024AJ....168..297T.doi:10.3847/1538-3881/ad81d7.ISSN 0004-6256.

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