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HD 1502

From Wikipedia, the free encyclopedia
K-type subgiant star in the constellation Pisces
HD 1502 / Citadelle
Location of HD 1502 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationPisces[1]
Right ascension00h 19m 17.0660s[2]
Declination+14° 03′ 17.123″[2]
Apparent magnitude (V)8.36[3]
Characteristics
Evolutionary stagesubgiant[4][2]
Spectral typeK0 IV[3][4][5]
B−Vcolor index0.92[3]
Astrometry
Radial velocity (Rv)−9.98±0.12[2] km/s
Proper motion (μ)RA: +74.472[2]1547mas/yr
Dec.: −17.069[2]mas/yr
Parallax (π)5.2018±0.0341 mas[2]
Distance627 ± 4 ly
(192 ± 1 pc)
Absolute magnitude (MV)+2.39[1]
Details
Mass1.46±0.15[5] M
Radius4.67±0.57[5] R
Luminosity11.75+15.14
−9.12
[5] L
Surface gravity (log g)3.18[5] cgs
Temperature4947[5] K
Metallicity[Fe/H]0.09±0.03[3] dex
Rotational velocity (v sin i)2.70±0.5[3] km/s
Age3.0+1.2
−0.8
[5] Gyr
Other designations
BD+13°34,Gaia DR2 2768172019308167296,HD 1502,HIP 1547,SAO 91845,TYC 601-636-1,GSC 00601-00636,2MASS J00191704+1403172[6]
Database references
SIMBADdata

HD 1502 (proper nameCitadelle) is an 8th-magnitudeK-typesubgiant star in the constellation ofPisces, located at a distance of approximately 630light-years. Asuper-Jupiter planet, HD 1502 b (proper name Indépendance), is known to orbit the star.

Nomenclature

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In 2019, theRepublic of Haiti was assigned to giving the HD 1502 system a proper name as part of theIAU100 NameExoWorlds Project, planned to celebrate the hundredth anniversary of theInternational Astronomical Union (IAU), which grants the right to name an exoplanetary system to every state and territory in the world.[7] Names were submitted and selected within Haiti, which were then presented to the IAU to be officially recognized.[8] On 17 December 2019, the IAU announced that HD 1502 and its planet, b, were named Citadelle and Indépendance, respectively.[9]

Citadelle refers to theCitadelle Laferrière, a fortress located inMilot in northern Haiti, which was built in 1820 and declared aWorld Heritage Site in 1982 as part of theNational History Park. Indépendance was named after theHaitian Declaration of Independence, in celebration of thecountry's independence on 1 January 1804.[9]

Stellar characteristics

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The star hasevolved past themain sequence stage and is now a subgiant with a mass of 1.46M, a radius of 4.67R, and a spectral type of K0.[3][4][5] The star is slightly richer than theSun in elements heavier thanhydrogen andhelium, with ametallicity of0.09±0.03.[a][3]

The star has aneffective temperature of 4,947 K (4,674 °C; 8,445 °F),[5] making it cooler than the Sun (5,772 K).[10] Despite this, its large size makes it roughly 12 times brighter.[5] At around 3.0 billion years old,[5] the star is about two-thirds theage of the Sun (4.6Gyr).[11] Due to its high mass, however, it is further evolved than the Sun, which will spend a total of 10 billion years as a main sequence star.[12]

Planetary system

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In 2011, anexoplanet orbiting HD 1502, designated HD 1502 b, was discovered using theradial-velocity method.[3] HD 1502 b revolves around its host star at a distance of 1.262 AU (188,800,000 km) with a period of little over one year in a near-circular orbit (i.e., with a loweccentricity),[4] similarly to planets in theSolar System.[13] It is a super-Jupiter planet with a minimum mass of 2.75MJ and a predicted radius of 1.183RJ.[4]

The HD 1502 planetary system[4]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b (Indépendance)≥2.75±0.16 MJ1.262±0.092428.5±1.20.031±0.0221.183 (predicted) RJ

See also

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References

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  1. ^abAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdefgVallenari, 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. ^abcdefghJohnson, John Asher; et al. (2011). "Retired A Stars and Their Companions. VII. 18 New Jovian Planets".The Astrophysical Journal Supplement Series.197 (2): 26.arXiv:1108.4205.Bibcode:2011ApJS..197...26J.doi:10.1088/0067-0049/197/2/26.ISSN 0067-0049.
  4. ^abcdefLuhn, Jacob K.; et al. (2019)."Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts".The Astronomical Journal.157 (4): 149.arXiv:1811.03043.Bibcode:2019AJ....157..149L.doi:10.3847/1538-3881/aaf5d0.ISSN 1538-3881.
  5. ^abcdefghijkBrewer, John M.; Fischer, Debra A.; Valenti, Jeff A.; Piskunov, Nikolai (2016)."Spectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars".The Astrophysical Journal Supplement Series.225 (2): 32.arXiv:1606.07929.Bibcode:2016ApJS..225...32B.doi:10.3847/0067-0049/225/2/32.ISSN 1538-4365.
  6. ^"HD 1502".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2025-05-18.
  7. ^"List of stars and planets | IAU100 Name ExoWorlds - An IAU100 Global Event".Name Exoworlds. International Astronomical Union. Retrieved2019-07-17.
  8. ^"Methodology | IAU100 Name ExoWorlds - An IAU100 Global Event".Name Exoworlds. International Astronomical Union. Retrieved2019-07-17.
  9. ^ab"Haiti | NameExoworlds".Name Exoworlds. International Astronomical Union. 2019-12-17. Retrieved2020-01-26.
  10. ^Williams, D. R. (1 July 2013)."Sun Fact Sheet".NASA Goddard Space Flight Center.Archived from the original on 15 July 2010. Retrieved12 August 2013.
  11. ^Connelly, J. N.; Bizzarro, M.; Krot, A. N.; Nordlund, Å.; Wielandt, D.; Ivanova, M. A. (2 November 2012). "The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk".Science.338 (6107):651–655.Bibcode:2012Sci...338..651C.doi:10.1126/science.1226919.PMID 23118187.S2CID 21965292.(registration required)
  12. ^"Main Sequence Stars".Australia Telescope National Facility. Retrieved2024-07-17.
  13. ^Limbach, MA; Turner, EL (2015)."Exoplanet orbital eccentricity: multiplicity relation and the Solar System".Proc Natl Acad Sci U S A.112 (1):20–4.arXiv:1404.2552.Bibcode:2015PNAS..112...20L.doi:10.1073/pnas.1406545111.PMC 4291657.PMID 25512527.

Footnotes

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  1. ^This translates to an abundance ofiron 100.09≈1.23 times that of the Sun. The margin of error (0.06–0.12) corresponds to a comparative abundance of 115–132% (100.06–100.12).

Further reading

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