Iota Piscium (Iota Psc, ι Piscium, ι Psc) is single,[10]F-type main-sequence star located 45 light years from Earth,[2] in the constellation Pisces. Its spectral type is F7V, which means that it is somewhat larger and brighter than the Sun, but still within the range considered to have the potential for Earth-like planets. It has a surface temperature of about 6,000 to 7,500 K. Iota Piscium is suspected to be a variable star, and was once thought to have one or two stellar companions, but both are line-of-sight coincidences.[11] It displays a far-infrared excess at a wavelength of 70μm, suggesting it is being orbited by a cold debris disk.[10]
^ abcdefvan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600 Vizier catalog entry
^ abGray, R. O.; Napier, M. G.; Winkler, L. I. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal, 121 (4): 2148–2158, Bibcode:2001AJ....121.2148G, doi:10.1086/319956.
^ abMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, Bibcode:1986EgUBV........0M
^Nordström, Andersen; et al. (2004), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs", Publications of the Astronomical Society of Australia, 21 (2): 129–133, arXiv:0811.3982, Bibcode:2004PASA...21..129N, doi:10.1071/AS04013, S2CID 123457673.
^Paunzen, E.; et al. (July 2014), "Investigating the possible connection between λ Bootis stars and intermediate Population II type stars", Astronomy & Astrophysics, 567: 8, arXiv:1406.3936, Bibcode:2014A&A...567A..67P, doi:10.1051/0004-6361/201423817, S2CID 56332289, A67.
^ abcBoyajian, Tabetha S.; et al. (February 2012), "Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars", The Astrophysical Journal, 746 (1): 101, arXiv:1112.3316, Bibcode:2012ApJ...746..101B, doi:10.1088/0004-637X/746/1/101, S2CID 18993744. See Table 10.
^ abRamírez, I.; et al. (February 2013), "Oxygen abundances in nearby FGK stars and the galactic chemical evolution of the local disk and halo", The Astrophysical Journal, 764 (1): 78, arXiv:1301.1582, Bibcode:2013ApJ...764...78R, doi:10.1088/0004-637X/764/1/78, S2CID 118751608
^Martínez-Arnáiz, R.; et al. (September 2010), (PDF), Astronomy and Astrophysics, 520: A79, arXiv:1002.4391, Bibcode:2010A&A...520A..79M, doi:10.1051/0004-6361/200913725, S2CID 43455849, archived from the original (PDF) on 2017-09-22, retrieved 2018-11-04
^ abcNuñez, Paul D.; et al. (September 2017), "A near-infrared interferometric survey of debris-disk stars. VI. Extending the exozodiacal light survey with CHARA/JouFLU", Astronomy & Astrophysics, 608 (113): A113, arXiv:1709.01655, Bibcode:2017A&A...608A.113N, doi:10.1051/0004-6361/201730859, S2CID 44229077
^Kaler, James B., , Stars, University of Illinois, archived from the original on January 25, 2007, retrieved September 27, 2007
^(in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 8 日
October 20, 2023
iota, piscium, iota, piscium, single, type, main, sequence, star, located, light, years, from, earth, constellation, pisces, spectral, type, which, means, that, somewhat, larger, brighter, than, still, within, range, considered, have, potential, earth, like, p. Iota Piscium Iota Psc i Piscium i Psc is single 10 F type main sequence star located 45 light years from Earth 2 in the constellation Pisces Its spectral type is F7V which means that it is somewhat larger and brighter than the Sun but still within the range considered to have the potential for Earth like planets It has a surface temperature of about 6 000 to 7 500 K Iota Piscium is suspected to be a variable star and was once thought to have one or two stellar companions but both are line of sight coincidences 11 It displays a far infrared excess at a wavelength of 70mm suggesting it is being orbited by a cold debris disk 10 Iota Piscium 1 Location of i Piscium circled Observation dataEpoch J2000 0 Equinox J2000 0Constellation PiscesRight ascension 23h 39m 57 04138s 2 Declination 05 37 34 6475 2 Apparent magnitude V 4 13 3 CharacteristicsSpectral type F7 V 3 U B color index 0 01 4 B V color index 0 50 4 AstrometryRadial velocity Rv 5 4 5 km sProper motion m RA 377 15 0 19 2 mas yr Dec 437 43 0 15 2 mas yrParallax p 72 92 0 15 mas 2 Distance44 73 0 09 ly 13 71 0 03 pc Absolute magnitude MV 3 43 6 DetailsRadius1 595 0 014 7 R Luminosity3 555 0 058 7 L Surface gravity log g 4 11 8 cgsTemperature6 288 37 7 KMetallicity Fe H 0 12 8 dexRotational velocity v sin i 6 67 9 km sAge5 2 10 GyrOther designationsi Piscium i Psc Iota Psc 17 Piscium BD 04 5035 CCDM J23399 0538A FK5 892 GC 32879 HD 222368 HIP 116771 HR 8969 IDS 23348 0505 A PPM 174312 SAO 128310 WDS J23399 0538A 1 Database referencesSIMBADdataNaming EditIn Chinese 霹靂 Pi Li meaning Thunderbolt refers to an asterism consisting of i Piscium b Piscium g Piscium 8 Piscium and w Piscium Consequently the Chinese name for i Piscium itself is 霹靂四 Pi Li si English the Fourth Star of Thunderbolt 12 References Edit a b iot Psc SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved April 4 2007 a b c d e f van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 Vizier catalog entry a b Gray R O Napier M G Winkler L I April 2001 The Physical Basis of Luminosity Classification in the Late A F and Early G Type Stars I Precise Spectral Types for 372 Stars The Astronomical Journal 121 4 2148 2158 Bibcode 2001AJ 121 2148G doi 10 1086 319956 a b Mermilliod J C 1986 Compilation of Eggen s UBV data transformed to UBV unpublished Catalogue of Eggen s UBV Data Bibcode 1986EgUBV 0M Nordstrom Andersen et al 2004 The Geneva Copenhagen survey of the Solar neighbourhood Ages metallicities and kinematic properties of 14000 F and G dwarfs Publications of the Astronomical Society of Australia 21 2 129 133 arXiv 0811 3982 Bibcode 2004PASA 21 129N doi 10 1071 AS04013 S2CID 123457673 Paunzen E et al July 2014 Investigating the possible connection between l Bootis stars and intermediate Population II type stars Astronomy amp Astrophysics 567 8 arXiv 1406 3936 Bibcode 2014A amp A 567A 67P doi 10 1051 0004 6361 201423817 S2CID 56332289 A67 a b c Boyajian Tabetha S et al February 2012 Stellar Diameters and Temperatures I Main sequence A F and G Stars The Astrophysical Journal 746 1 101 arXiv 1112 3316 Bibcode 2012ApJ 746 101B doi 10 1088 0004 637X 746 1 101 S2CID 18993744 See Table 10 a b Ramirez I et al February 2013 Oxygen abundances in nearby FGK stars and the galactic chemical evolution of the local disk and halo The Astrophysical Journal 764 1 78 arXiv 1301 1582 Bibcode 2013ApJ 764 78R doi 10 1088 0004 637X 764 1 78 S2CID 118751608 Martinez Arnaiz R et al September 2010 Chromospheric activity and rotation of FGK stars in the solar vicinity An estimation of the radial velocity jitter PDF Astronomy and Astrophysics 520 A79 arXiv 1002 4391 Bibcode 2010A amp A 520A 79M doi 10 1051 0004 6361 200913725 S2CID 43455849 archived from the original PDF on 2017 09 22 retrieved 2018 11 04 a b c Nunez Paul D et al September 2017 A near infrared interferometric survey of debris disk stars VI Extending the exozodiacal light survey with CHARA JouFLU Astronomy amp Astrophysics 608 113 A113 arXiv 1709 01655 Bibcode 2017A amp A 608A 113N doi 10 1051 0004 6361 201730859 S2CID 44229077 Kaler James B Iota Piscium Stars University of Illinois archived from the original on January 25 2007 retrieved September 27 2007 in Chinese AEEA Activities of Exhibition and Education in Astronomy 天文教育資訊網 2006 年 7 月 8 日 Retrieved from https en wikipedia org w index php title Iota Piscium amp oldid 1176953853, wikipedia, wiki, book, books, library,
