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(6 revisi perantara oleh 5 pengguna tidak ditampilkan)
Baris 1: Baris 1:
{{Starbox begin
[[Berkas:Sadr_Region_rgb.jpg|jmpl|Lokasi KY Cygni (paling bercahaya).]]
| name = KY Cygni
}}
{{Starbox image
| image=
{{Location mark
|image=Sadr Region rgb.jpg|alt=|float=center|width=250
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=KY Cyg
|x=215|y=193
}}
|caption=Lokasi KY Cygni (dilingkari, timur berada di atas)
}}
{{Starbox observe
| epoch = [[J2000.0]]
| equinox = [[J2000.0]] ([[International Celestial Reference System|ICRS]])
| constell = [[Cygnus (constellation)|Cygnus]]
| ra = {{RA|20|25|58.04}}<ref name=edr3>{{Cite journal|last=Gaia Collaboration|last2=Brown|first2=A. G. A.|last3=Vallenari|first3=A.|last4=Prusti|first4=T.|last5=de Bruijne|first5=J. H. J.|last6=Babusiaux|first6=C.|last7=Biermann|first7=M.|last8=Creevey|first8=O. L.|last9=Evans|first9=D. W.|date=2021-05-01|title=Gaia Early Data Release 3. Summary of the contents and survey properties|url=https://ui.adsabs.harvard.edu/abs/2021A&A...649A...1G|journal=Astronomy and Astrophysics|volume=649|pages=A1|doi=10.1051/0004-6361/202039657|issn=0004-6361}} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?Gaia%20EDR3%202058131491974019968 Catatan Gaia DR3 untuk sumber ini] di [[VizieR]].</ref>
| dec = {{DEC|+38|21|07.7}}<ref name=edr3/>
| appmag_v=11.14<ref name=mauron>{{cite journal|bibcode=2011A&A...526A.156M|title=The mass-loss rates of red supergiants and the de Jager prescription|journal=Astronomy and Astrophysics|volume=526|pages=A156|last1=Mauron|first1=N.|last2=Josselin|first2=E.|year=2011|doi=10.1051/0004-6361/201013993|arxiv = 1010.5369 |s2cid=119276502}}</ref> {{nowrap|(10.60 - 11.74<ref name=alfonso-garzon>{{cite journal |bibcode=2012A&A...548A..79A |title=The first INTEGRAL-OMC catalogue of optically variable sources |journal=Astronomy & Astrophysics |volume=548 |page=A79 |last1=Alfonso-Garzón |first1=J. |last2=Domingo |first2=A. |last3=Mas-Hesse |first3=J. M. |last4=Giménez |first4=A. |year=2012 |arxiv=1210.0821 |doi=10.1051/0004-6361/201220095|s2cid=118428054 }}</ref>)}}
}}
{{Starbox character
| class = M3 Ia<ref name=white>{{cite journal|bibcode=1978ApJ...222..209W|title=Photoelectric two-dimensional spectral classification of M supergiants|journal=Astrophysical Journal|volume=222|pages=209|last1=White|first1=N. M.|last2=Wing|first2=R. F.|year=1978|doi=10.1086/156136}}</ref> (M3.5 Ia<ref name=gcvs1>KY Cyg, database entry, [http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/iii.dat The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars] {{Webarchive|url=https://web.archive.org/web/20170620004609/http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/iii.dat |date=2017-06-20 }}, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line November 12, 2010.</ref> (M3.5 Ia<ref name=gcvs1/>)
| b-v = +3.39<ref name=mauron/>
| u-b = +2.91<ref name=mauron/>
| variable = [[Slow irregular variable|Lc]]<ref name=gcvs1/>
}}
{{Starbox astrometry
| prop_mo_ra = –3.556<ref name=edr3/>
| prop_mo_dec = –6.061<ref name=edr3/>
| parallax = 0.6687
| p_error = 0.0517
| parallax_footnote = <ref name=edr3/>
| dist_pc =
| dist_ly =
| absmag_v = –8.18<ref name=levesque>{{cite journal|bibcode=2005ApJ...628..973L|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought|journal=The Astrophysical Journal|volume=628|issue=2|pages=973–985|author1-link=Emily Levesque|last1=Levesque|first1=Emily M.|last2=Massey|first2=Philip|last3=Olsen|first3=K. A. G.|last4=Plez|first4=Bertrand|last5=Josselin|first5=Eric|last6=Maeder|first6=Andre|last7=Meynet|first7=Georges|year=2005|doi=10.1086/430901|arxiv = astro-ph/0504337 |s2cid=15109583}}</ref>
}}
{{Starbox detail
| mass = 19<ref name="Comeron"/>
| radius = 1,033<ref name="Comeron">{{Cite journal|last1=Comerón|first1=F.|last2=Djupvik|first2=A. A.|last3=Schneider|first3=N.|last4=Pasquali|first4=A.|date=October 2020|title=The historical record of massive star formation in Cygnus|journal=Astronomy & Astrophysics|volume=644|pages=A62|arxiv=2009.12779|bibcode=2020A&A...644A..62C|doi=10.1051/0004-6361/202039188|s2cid=221970180}}</ref>
| temperature=3,550<ref name=messinio2019>{{cite journal |bibcode=2019AJ....158...20M |title=A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2 |last1=Messineo |first1=M. |last2=Brown |first2=A. G. A. |journal=The Astronomical Journal |year=2019 |volume=158 |issue=1 |pages=20 |doi=10.3847/1538-3881/ab1cbd |arxiv=1905.03744 |s2cid=148571616 }}</ref>
| luminosity = 138,000<ref name=mauron/> – 270,000<ref name=levesque/><ref name=trevor>{{cite journal|arxiv=2008.11723|last1=Dorn-Wallenstein|first1=Trevor Z.|last2=Levesque|first2=Emily M.|last3=Neugent|first3=Kathryn F.|last4=Davenport|first4=James R. A.|last5=Morris|first5=Brett M.|last6=Gootkin|first6=Keyan|title=Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants|journal=The Astrophysical Journal|year=2020|volume=902|issue=1|page=24|doi=10.3847/1538-4357/abb318|bibcode=2020ApJ...902...24D|s2cid=221340538}}</ref>
| metal=
| gravity=−0.5 (−0.9?)<ref name=levesque/>
| rotation=
| age=
}}
{{Starbox catalog
| names=[[Variable star designation|KY]]&nbsp;Cyg, [[Guide Star Catalog|GSC]]&nbsp;03152-01140, [[IRAS]]&nbsp;20241+3811, IRC+40415, [[Tycho Catalogue|TYC]]&nbsp;3152-1140-1, [[RAFGL]]&nbsp;2575, [[USNO CCD Astrograph Catalog|UCAC2]]&nbsp;45230193, [[2MASS]]&nbsp;J20255805+3821076
}}
{{Starbox reference
| Simbad=KY+Cyg}}
{{Starbox end}}


'''KY Cygni''' adalah bintang [[Superraksasa]] merah dari [[kelas spektrum]] M3.5la yang terletak di rasi bintang [[Cygnus]].<ref>{{Cite web|url=https://www.universeguide.com/star/kycygni|title=KY Cygni (Supergiant Star) Star Facts|website=Universe Guide|language=en|access-date=2020-02-15}}</ref> KY Cygni merupakan salah satu bintang terbesar dan paling bercahaya yang pernah diketahui, dengan luminositas sekitar 300.000 kali lebih dari matahari dengan radius 1.000 kali ruas jari jari matahari. Jika ditempatkan di Tata Surya maka fotosfernya akan mencapai orbit Jupiter atau mungkin Saturnus.
'''KY Cygni''' adalah bintang [[Superraksasa]] merah dari [[kelas spektrum]] M3.5la yang terletak di rasi bintang [[Cygnus]].<ref>{{Cite web|url=https://www.universeguide.com/star/kycygni|title=KY Cygni (Supergiant Star) Star Facts|website=Universe Guide|language=en|access-date=2020-02-15}}</ref> KY Cygni merupakan salah satu bintang terbesar dan paling bercahaya yang pernah diketahui, dengan luminositas sekitar 300.000 kali lebih dari matahari dengan radius 1.000 kali ruas jari jari matahari. Jika ditempatkan di Tata Surya maka fotosfernya akan mencapai orbit Jupiter atau mungkin Saturnus.
Baris 6: Baris 58:
<references />
<references />


== Tautan eksternal ==
== Pranala luar ==


* http://jumk.de/astronomie/big-stars/ky-cygni.shtml
* http://jumk.de/astronomie/big-stars/ky-cygni.shtml
*http://www.astronomy.com/asy/default.aspx?c=a&id=2772
* http://www.astronomy.com/asy/default.aspx?c=a&id=2772

[[Kategori:Maharaksasa merah]]
[[Kategori:Rasi bintang Cygnus]]

Revisi terkini sejak 10 Juni 2024 14.33

KY Cygni

Lokasi KY Cygni (dilingkari, timur berada di atas)
Data pengamatan
Epos J2000.0      Ekuinoks J2000.0 (ICRS)
Rasi bintang Cygnus
Asensio rekta  20j 25m 58.04d[1]
Deklinasi  +38° 21′ 07.7″[1]
Magnitudo tampak (V) 11.14[2] (10.60 - 11.74[3])
Ciri-ciri
Kelas spektrum M3 Ia[4] (M3.5 Ia[5] (M3.5 Ia[5])
Indeks warna U−B +2.91[2]
Indeks warna B−V +3.39[2]
Jenis variabel Lc[5]
Astrometri
Gerak diri (μ) RA: –3.556[1] mdb/thn
Dek.: –6.061[1] mdb/thn
Paralaks (π)0,6687±0,0517[1] mdb
Jarak4.900 ± 400 tc
(1.500 ± 100 pc)
Magnitudo mutlak (MV)–8.18[6]
Detail
Massa19[7] M☉
Radius1,033[7] R☉
Luminositas138,000[2] – 270,000[6][8] L☉
Gravitasi permukaan (log g)−0.5 (−0.9?)[6]
Suhu3,550[9] K
Penamaan lain
KY Cyg, GSC 03152-01140, IRAS 20241+3811, IRC+40415, TYC 3152-1140-1, RAFGL 2575, UCAC2 45230193, 2MASS J20255805+3821076
Referensi basis data
SIMBADdata

KY Cygni adalah bintang Superraksasa merah dari kelas spektrum M3.5la yang terletak di rasi bintang Cygnus.[10] KY Cygni merupakan salah satu bintang terbesar dan paling bercahaya yang pernah diketahui, dengan luminositas sekitar 300.000 kali lebih dari matahari dengan radius 1.000 kali ruas jari jari matahari. Jika ditempatkan di Tata Surya maka fotosfernya akan mencapai orbit Jupiter atau mungkin Saturnus.

Referensi

[sunting | sunting sumber]
  1. ^ a b c d e Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; Babusiaux, C.; Biermann, M.; Creevey, O. L.; Evans, D. W. (2021-05-01). "Gaia Early Data Release 3. Summary of the contents and survey properties". Astronomy and Astrophysics. 649: A1. doi:10.1051/0004-6361/202039657. ISSN 0004-6361.  Catatan Gaia DR3 untuk sumber ini di VizieR.
  2. ^ a b c d Mauron, N.; Josselin, E. (2011). "The mass-loss rates of red supergiants and the de Jager prescription". Astronomy and Astrophysics. 526: A156. arXiv:1010.5369 alt=Dapat diakses gratis. Bibcode:2011A&A...526A.156M. doi:10.1051/0004-6361/201013993. 
  3. ^ Alfonso-Garzón, J.; Domingo, A.; Mas-Hesse, J. M.; Giménez, A. (2012). "The first INTEGRAL-OMC catalogue of optically variable sources". Astronomy & Astrophysics. 548: A79. arXiv:1210.0821 alt=Dapat diakses gratis. Bibcode:2012A&A...548A..79A. doi:10.1051/0004-6361/201220095. 
  4. ^ White, N. M.; Wing, R. F. (1978). "Photoelectric two-dimensional spectral classification of M supergiants". Astrophysical Journal. 222: 209. Bibcode:1978ApJ...222..209W. doi:10.1086/156136. 
  5. ^ a b c KY Cyg, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars Diarsipkan 2017-06-20 di Wayback Machine., Sternberg Astronomical Institute, Moscow, Russia. Accessed on line November 12, 2010.
  6. ^ a b c Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought". The Astrophysical Journal. 628 (2): 973–985. arXiv:astro-ph/0504337 alt=Dapat diakses gratis. Bibcode:2005ApJ...628..973L. doi:10.1086/430901. 
  7. ^ a b Comerón, F.; Djupvik, A. A.; Schneider, N.; Pasquali, A. (October 2020). "The historical record of massive star formation in Cygnus". Astronomy & Astrophysics. 644: A62. arXiv:2009.12779 alt=Dapat diakses gratis. Bibcode:2020A&A...644A..62C. doi:10.1051/0004-6361/202039188. 
  8. ^ Dorn-Wallenstein, Trevor Z.; Levesque, Emily M.; Neugent, Kathryn F.; Davenport, James R. A.; Morris, Brett M.; Gootkin, Keyan (2020). "Short Term Variability of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants". The Astrophysical Journal. 902 (1): 24. arXiv:2008.11723 alt=Dapat diakses gratis. Bibcode:2020ApJ...902...24D. doi:10.3847/1538-4357/abb318. 
  9. ^ Messineo, M.; Brown, A. G. A. (2019). "A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2". The Astronomical Journal. 158 (1): 20. arXiv:1905.03744 alt=Dapat diakses gratis. Bibcode:2019AJ....158...20M. doi:10.3847/1538-3881/ab1cbd. 
  10. ^ "KY Cygni (Supergiant Star) Star Facts". Universe Guide (dalam bahasa Inggris). Diakses tanggal 2020-02-15. 

Pranala luar

[sunting | sunting sumber]
Diperoleh dari "https://wiki-indonesia.club/w/index.php?title=KY_Cygni&oldid=25815347"