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词条 30 Piscium
释义

  1. References

{{Starbox begin
| name = 30 Piscium
}}{{Starbox image
| image={{Location mark
|image=Pisces constellation map.svg|alt=|float=center|width=240
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=30 Piscium
|x=632|y=870
}}
|caption=Location of 30 Piscium (circled)
}}{{Starbox observe
| epoch = J2000
| constell = Pisces
| ra = {{RA|00|01|57.61523}}
| dec = {{DEC|-06|00|50.6684}}
| appmag_v = 4.31 – 4.41[3]
}}{{Starbox character
| class = M3 III[4]
| b-v = {{Val|1.631|0.011}}[5]
| u-b =
| variable = LPV,[6] LB?[3]
}}{{Starbox astrometry
| radial_v = {{Val|−11.7|0.5}}[8]
| prop_mo_ra = +51.158
| prop_mo_dec = −39.551
| parallax = 7.8859
| p_error = 0.4358
| parallax_footnote =
| absmag_v = −1.20[6]
}}{{Starbox detail
| source =
| mass =
| radius = {{Val|73.66|16.69|6.79}}
| luminosity = {{Val|1148.5|71.1|fmt=commas}}
| gravity = 2[15]
| temperature = 3,647[15]
| metal_fe =
| rotational_velocity =
| age_myr =
}}{{Starbox catalog
| names = {{odlist | V=YY Psc | F=30 Psc | BD=−06° 6345 | FK5=1630 | HD=224935 | HIP=154 | HR=9089 | SAO=147042 }}[17]
}}{{Starbox reference
| Simbad = 30+Psc
}}{{Starbox end}}30 Piscium (HIP 154) is a solitary[18] variable star in the zodiac constellation of Pisces. It is visible to the naked eye with an apparent visual magnitude of 4.37.[15] The distance to this star, based upon an annual parallax shift of {{Val|7.8859|ul=mas}}, is around 410 light years. It is moving closer with a heliocentric radial velocity of −12 km/s.[8]

This is an aging red giant star with a stellar classification of M3 III,[4] indicating it has exhausted the hydrogen at its core and evolved off the main sequence. It is a candidate long-period variable star[6] and has been given the designation YY Psc.[23] Its varies in brightness between magnitudes 4.31 and 4.41 with no clear period. Possible periods of 23.1, 32.0, 53.6, and 167.8 days have been identified.[24] The star has 74 times the Sun's radius and is radiating 1,148.5 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,647 K.[15]

References

1. ^{{cite simbad | title=30 Psc | access-date=2018-03-10 }}
2. ^{{cite journal|doi=10.1111/j.1365-2966.2009.15588.x|arxiv=0908.3228|title=Long-term photometry and periods for 261 nearby pulsating M giants|journal=Monthly Notices of the Royal Astronomical Society|volume=400|issue=4|pages=1945|year=2009|last1=Tabur|first1=V|last2=Bedding|first2=T. R|last3=Kiss|first3=L. L|last4=Moon|first4=T. T|last5=Szeidl|first5=B|last6=Kjeldsen|first6=H|bibcode=2009MNRAS.400.1945T}}
3. ^{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 |date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | postscript=. |arxiv = 0806.2878 }}
4. ^{{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | postscript=. }}
5. ^{{citation | title=Automated classification of Hipparcos unsolved variables | display-authors=1 | last1=Rimoldini | first1=L. | last2=Dubath | first2=P. | last3=Süveges | first3=M. | last4=López | first4=M. | last5=Sarro | first5=L. M. | last6=Blomme | first6=J. | last7=De Ridder | first7=J. | last8=Cuypers | first8=J. | last9=Guy | first9=L. | last10=Mowlavi | first10=N. | last11=Lecoeur-Taïbi | first11=I. | last12=Beck | first12=M. | last13=Jan | first13=A. | last14=Nienartowicz | first14=K. | last15=Ordóñez-Blanco | first15=D. | last16=Lebzelter | first16=T. | last17=Eyer | first17=L. | journal=Monthly Notices of the Royal Astronomical Society | volume=427 | issue=4 | pages=2917–2937 | date=December 2012 | doi=10.1111/j.1365-2966.2012.21752.x | bibcode=2012MNRAS.427.2917R | arxiv=1301.1545 | postscript=. }}
6. ^{{citation | last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C. | title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project | journal=Astronomy & Astrophysics | volume=546 | id=A61 | pages=14 | date=October 2012 | doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D | arxiv=1208.3048 | postscript=. }}
7. ^{{citation | postscript=. | title=The non-active stellar chromosphere: Ca II basal flux | display-authors=1 | last1=Pérez Martínez | first1=M. I. | last2=Schröder | first2=K.-P. | last3=Hauschildt | first3=P. | journal=Monthly Notices of the Royal Astronomical Society | volume=445 | issue=1 | pages=270–279 | date=November 2014 | doi=10.1093/mnras/stu1706 | bibcode=2014MNRAS.445..270P }}
8. ^{{citation | title=60th Name-List of Variable Stars | last1=Kukarkin | first1=B. V. | last2=Kholopov | first2=P. N. | last3=Kukarkina | first3=N. P. | last4=Perova | first4=N. B. | journal=Information Bulletin on Variable Stars | volume=961 | page=1 | date=January 1975 | display-authors=1 | bibcode=1975IBVS..961....1K | postscript=. }}
9. ^{{citation | first1=P. | last1=Keenan | first2=R. | last2=McNeil | title=The Perkins catalog of revised MK types for the cooler stars | journal=Astrophysical Journal Supplement Series | volume=71 | pages=245–266 | date=October 1989 | bibcode=1989ApJS...71..245K | doi=10.1086/191373 | postscript=. }}
10. ^{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S|volume=1|display-authors=etal|author1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}
[1][2][3][4][5][6][7][8][9][10]
}}{{Stars of Pisces}}

9 : M-type giants|Slow irregular variables|Pisces (constellation)|Durchmusterung objects|Flamsteed objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects|Objects with variable star designations

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