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| constell = [[Volans]]
| constell = [[Volans]]
| epoch = J2000
| epoch = J2000
| ra = {{RA|07|28|51.41}}<ref name = GaiaDR2/>
| ra = {{RA|07|28|51.4078}}<ref name = EDR3/>
| dec = {{DEC|-64|30|35.30}}<ref name = GaiaDR2/>
| dec = {{DEC|-64|30|35.3006}}<ref name = EDR3/>
| appmag_v = {{val|6.39|0.01}}<ref name = Tycho2/>
| appmag_v = {{val|6.39|0.01}}<ref name = Tycho2000/>
}}
}}
{{Starbox character
{{Starbox character
| class = K5 III<ref name = Houk1975/>
| class = K5 III<ref name = Houk1975/>
| b-v=+1.55<ref name = HIP/>
| b-v = +1.54<ref name = Johnson1966/>
| u-b = +1.84<ref name = Johnson1966/>
}}
}}
{{Starbox astrometry
{{Starbox astrometry
| radial_v = {{val|14.14|0.15}}<ref name = GaiaDR2/>
| radial_v = 13.4{{±|0.4}}<ref name = Gontcharov2006/>
| pm_footnote = <ref name = GaiaDR2/>
| pm_footnote = <ref name = EDR3/>
| parallax = 4.3255
| parallax = 4.419
| p_error = 0.0470
| p_error = 0.029
| parallax_footnote = <ref name = GaiaDR2/>
| parallax_footnote = <ref name = EDR3/>
| prop_mo_ra = 4.817
| prop_mo_ra = +4.940
| prop_mo_dec = −8.825
| prop_mo_dec = −8.876
| absmag_v = −0.34<ref name = XHIP/>
| absmag_v = −0.34<ref name = Anderson2012/>
}}
}}
{{Starbox detail
{{Starbox detail
| radius = {{val|36.77|2.78|1.75}}<ref name = GaiaDR2/>
| radius = 41.18<ref name = Stassun2019/>
| luminosity = {{val|329|5}}<ref name = GaiaDR2/>
| luminosity = {{val|329|5}}<ref name = GaiaDR2/>
| temperature = {{val|4055|100|145|fmt=commas}}<ref name = GaiaDR2/>
| temperature = 4,007{{±|122}}<ref name = Stassun2019/>
| metal_fe = 0.05<ref name = Anders2019/>
| metal_fe = +0.14<ref name = Anders2019/>
| gravity = 1.33<ref name = Anders2019/>
| gravity = 1.24<ref name = Anders2019/>
| mass = 1.56<ref name = Anders2019/>
| mass = 1.2<ref name = Anders2019/>
| rotational_velocity = {{val|1.8|1.2}}<ref name = DeMed2014/>
| rotational_velocity = {{val|1.8|1.2}}<ref name = DeMed2014/>
}}
}}
{{Starbox catalog
{{Starbox catalog
| names = {{odlist|HD=60150|HR=2888|HIP=36346|SAO=249864|CD=-64 273}}
| names = {{odlist|HD = 60150|HR = 2888|HIP = 36346|SAO = 249864|CD = −64°273|CPD = −64°721|FK5 = 2584|GC = 10057|Gould = 12 G. Volantis}}<ref name = SIMBAD/><ref name = Gould1879/>
}}
}}
{{starbox reference
{{starbox reference
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{{starbox end}}
{{starbox end}}


'''HD 60150 (HR 2888)''' is a solitary [[star]] located in the constellation [[Volans]]. With an [[apparent magnitude]] of 6.39, it is close to the [[limiting magnitude]] for naked-eye visibility. The star is located 754 [[Light-year|light years]] away from the [[Solar System]], but is drifting away with a [[radial velocity]] of 14.14&nbsp;km/s.
'''HD 60150''' ('''HR 2888''') is a solitary [[star]] located in the southern [[circumpolar constellation]] [[Volans]]. It has an [[apparent magnitude]] of 6.39, placing it near the [[limiting magnitude]] for naked-eye visibility. [[Parallax]] measurements place the star at a distance of 738 [[light year]]s and it is currently receding with a heliocentric [[radial velocity]] of {{val|13.4|ul=km/s}}.<ref name = Gontcharov2006/>


⚫
HD 60150 has a classification of K5 III,<ref name = Houk1975/> indicating that it is a [[red giant]]. It has 1.2 times the [[mass of the Sun]]<ref name = Anders2019/> but has expanded to 41 times its girth.<ref name = Stassun2019/> It radiates 329 times the [[luminosity of the Sun]]<ref name = GaiaDR2/> from its swollen [[photosphere]] at an [[effective temperature]] of 4,007 [[Kelvin|K]],<ref name = Stassun2019/> giving it a reddish orange hue. HD 60150 is metal enriched, with an [[iron]] abundance 38% greater than the [[Sun]].<ref name = Stassun2019/> It spins leisurely with [[projected rotational velocity]] of about {{val|1.8|ul=km/s}}.<ref name = DeMed2014/>
== Properties ==
⚫
HD 60150 has a classification of "K5III", which means it is a [[K-type star]] that has exhausted the [[hydrogen]] at its core, and left the [[main sequence]]. It has 1.56 times the mass of the Sun, but has expanded to 36.77 the Sun's girth. It radiates 329 times the Sun's luminosity from its swollen [[photosphere]] at an [[effective temperature]] of 4,055 K, which gives it a yellow-orange hue. HD 60150 is metal-rich, with 12% more heavy metals than the Sun, and has a [[projected rotational velocity]] of 1.8&nbsp;km/s.


== See also ==
== See also ==
Line 50: Line 50:


== References ==
== References ==
{{Reflist|refs=<ref name = GaiaDR2>{{Cite DR2|5288387527849406592}}</ref>
{{Reflist||refs=


<ref name = EDR3>{{Cite Gaia EDR3|5288387527849406592}}</ref>
⚫
<ref name = Tycho2>{{Cite journal|last1=Høg|first1=E.|last2=Fabricius|first2=C.|last3=Makarov|first3=V. V.|last4=Urban|first4=S.|last5=Corbin|first5=T.|last6=Wycoff|first6=G.|last7=Bastian|first7=U.|last8=Schwekendiek|first8=P.|last9=Wicenec|first9=A.|date=2000-03-01|title=The Tycho-2 catalogue of the 2.5 million brightest stars|bibcode=2000A&A...355L..27H|journal=Astronomy and Astrophysics|volume=355|pages=L27–L30|issn=0004-6361}}</ref>


<ref name = GaiaDR2>{{Cite DR2|5288387527849406592}}</ref>
⚫
<ref name = Houk1975>{{Cite journal|last1=Houk|first1=N.|last2=Cowley|first2=A. P.|date=1975|title=University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_f0.|bibcode=1975mcts.book.....H|journal=University of Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume I. Declinations -90_ to -53_f0., by Houk, N.; Cowley, A. P.. Ann Arbor, MI (USA): Department of Astronomy, University of Michigan, 19 + 452 P.}}</ref>


⚫
<ref name = Tycho2000>{{cite journal |last1=Høg |first1=E. |last2=Fabricius |first2=C. |last3=Makarov |first3=V. V. |last4=Urban |first4=S. |last5=Corbin |first5=T. |last6=Wycoff |first6=G. |last7=Bastian |first7=U. |last8=Schwekendiek |first8=P. |last9=Wicenec |first9=A. |title=The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics |date=March 2000 |volume=355 |pages=L27–L30 |bibcode=2000A&A...355L..27H |issn=0004-6361 }}</ref>
<ref name = HIP>{{Cite journal|last=ESA|date=1997|title=The HIPPARCOS and TYCHO catalogues. Astrometric and photometric star catalogues derived from the ESA HIPPARCOS Space Astrometry Mission|journal=Esa Special Publication|bibcode=1997ESASP1200.....E|volume=1200}}</ref>


⚫
<ref name = Houk1975>{{cite book |last1=Houk |first1=N. |last2=Cowley |first2=A. P. |title=University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. |date=1975 |bibcode=1975mcts.book.....H }}</ref>
<ref name = XHIP>{{Cite journal|last1=Anderson|first1=E.|last2=Francis|first2=Ch.|date=2012-05-01|title=XHIP: An extended hipparcos compilation|bibcode=2012AstL...38..331A|journal=Astronomy Letters|volume=38|issue=5|pages=331–346|doi=10.1134/S1063773712050015|arxiv=1108.4971|s2cid=119257644|issn=1063-7737}}</ref>


<ref name = Gontcharov2006>{{cite journal |last1=Gontcharov |first1=G. A. |title=Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system |journal=Astronomy Letters |date=November 2006 |volume=32 |issue=11 |pages=759–771 |doi=10.1134/S1063773706110065 |issn=1063-7737 |bibcode=2006AstL...32..759G |arxiv=1606.08053|s2cid=119231169 }}</ref>
⚫
<ref name = Anders2019>{{Cite journal|last1=Anders|first1=F.|last2=Khalatyan|first2=A.|last3=Chiappini|first3=C.|last4=Queiroz|first4=A. B.|last5=Santiago|first5=B. X.|last6=Jordi|first6=C.|last7=Girardi|first7=L.|last8=Brown|first8=A. G. A.|last9=Matijevic|first9=G.|last10=Monari|first10=G.|last11=Cantat-Gaudin|first11=T.|date=2019-08-01|title=Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18|bibcode=2019A&A...628A..94A|journal=Astronomy and Astrophysics|volume=628|pages=A94|doi=10.1051/0004-6361/201935765|arxiv=1904.11302|s2cid=131780028|issn=0004-6361}}</ref>


<ref name = DeMed2014>{{Cite journal|last1=De Medeiros|first1=J. R.|last2=Alves|first2=S.|last3=Udry|first3=S.|last4=Andersen|first4=J.|last5=Nordström|first5=B.|last6=Mayor|first6=M.|date=2014-01-01|title=A catalog of rotational and radial velocities for evolved stars. V. Southern stars|bibcode=2014A&A...561A.126D|journal=Astronomy and Astrophysics|volume=561|pages=A126|doi=10.1051/0004-6361/201220762|arxiv=1312.3474|s2cid=54046583|issn=0004-6361}}</ref>}}
<ref name = Anderson2012>{{cite journal |last1=Anderson |first1=E. |last2=Francis |first2=Ch. |title=XHIP: An extended hipparcos compilation |journal=Astronomy Letters |date=May 2012 |volume=38 |issue=5 |pages=331–346 |doi=10.1134/S1063773712050015 |language=en |issn=1063-7737 |bibcode=2012AstL...38..331A |arxiv=1108.4971|s2cid=119257644 }}</ref>


⚫
<ref name = Anders2019>{{cite journal |display-authors=1 |last1=Anders |first1=F. |last2=Khalatyan |first2=A. |last3=Chiappini |first3=C. |last4=Queiroz |first4=A. B. |last5=Santiago |first5=B. X. |last6=Jordi |first6=C. |last7=Girardi |first7=L. |last8=Brown |first8=A. G. A. |last9=Matijevič |first9=G. |last10=Monari |first10=G. |last11=Cantat-Gaudin |first11=T. |last12=Weiler |first12=M. |last13=Khan |first13=S. |last14=Miglio |first14=A. |last15=Carrillo |first15=I. |last16=Romero-Gómez |first16=M. |last17=Minchev |first17=I. |last18=de Jong |first18=R. S. |last19=Antoja |first19=T. |last20=Ramos |first20=P. |last21=Steinmetz |first21=M. |last22=Enke |first22=H. |title=Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18 |journal=Astronomy & Astrophysics |date=August 2019 |volume=628 |pages=A94 |doi=10.1051/0004-6361/201935765 |issn=0004-6361 |bibcode=2019A&A...628A..94A |arxiv=1904.11302 |doi-access=free}}</ref>

<ref name = DeMed2014>{{cite journal |last1=De Medeiros |first1=J. R. |last2=Alves |first2=S. |last3=Udry |first3=S. |last4=Andersen |first4=J. |last5=Nordström |first5=B. |last6=Mayor |first6=M. |title=A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆ |journal=Astronomy & Astrophysics |date=January 2014 |volume=561 |pages=A126 |doi=10.1051/0004-6361/201220762 |issn=0004-6361 |bibcode=2014A&A...561A.126D |arxiv=1312.3474|doi-access=free}}</ref>

<ref name = Stassun2019>{{cite journal |display-authors=1 |last1=Stassun |first1=Keivan G. |last2=Oelkers |first2=Ryan J. |last3=Paegert |first3=Martin |last4=Torres |first4=Guillermo |last5=Pepper |first5=Joshua |last6=Lee |first6=Nathan De |last7=Collins |first7=Kevin |last8=Latham |first8=David W. |last9=Muirhead |first9=Philip S. |last10=Chittidi |first10=Jay |last11=Rojas-Ayala |first11=Bárbara |last12=Fleming |first12=Scott W. |last13=Rose |first13=Mark E. |last14=Tenenbaum |first14=Peter |last15=Ting |first15=Eric B. |last16=Kane |first16=Stephen R. |last17=Barclay |first17=Thomas |last18=Bean |first18=Jacob L. |last19=Brassuer |first19=C. E. |last20=Charbonneau |first20=David |last21=Ge |first21=Jian |last22=Lissauer |first22=Jack J. |last23=Mann |first23=Andrew W. |last24=McLean |first24=Brian |last25=Mullally |first25=Susan |last26=Narita |first26=Norio |last27=Plavchan |first27=Peter |last28=Ricker |first28=George R. |last29=Sasselov |first29=Dimitar |last30=Seager |first30=S. |last31=Sharma |first31=Sanjib |last32=Shiao |first32=Bernie |last33=Sozzetti |first33=Alessandro |last34=Stello |first34=Dennis |last35=Vanderspek |first35=Roland |last36=Wallace |first36=Geoff |last37=Winn |first37=Joshua N. |title=The Revised TESS Input Catalog and Candidate Target List |journal=The Astronomical Journal |date=9 September 2019 |volume=158 |issue=4 |pages=138 |doi=10.3847/1538-3881/ab3467 |issn=0004-6256 |bibcode=2019AJ....158..138S |arxiv=1905.10694 |doi-access=free}}</ref>

<ref name = Gould1879>{{cite journal | last=Gould | first=Benjamin Apthorp | title=Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas | journal=Resultados del Observatorio Nacional Argentino | volume=1 | bibcode=1879RNAO....1.....G | year=1878 | page=}}</ref>

<ref name = SIMBAD>{{Cite simbad|title = HR 2888|access-date = June 21, 2022}}</ref>

<ref name = Johnson1966>{{cite journal |last1=Johnson |first1=H. L. |last2=Mitchell |first2=R. I. |last3=Iriarte |first3=B. |last4=Wisniewski |first4=W. Z. |title=UBVRIJKL Photometry of the Bright Stars |journal=Communications of the Lunar and Planetary Laboratory |year=1966 |volume=4 |pages=99–110 |bibcode=1966CoLPL...4...99J}}</ref>

}}
{{Volans}}
{{Volans}}
{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}
{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}

Revision as of 15:57, 21 June 2022

HD 60150
Observation data
Epoch J2000      Equinox J2000
Constellation Volans
Right ascension 07h 28m 51.4078s[1]
Declination −64° 30′ 35.3006″[1]
Apparent magnitude (V) 6.39±0.01[2]
Characteristics
Spectral type K5 III[3]
U−B color index +1.84[4]
B−V color index +1.54[4]
Astrometry
Radial velocity (Rv)13.4±0.4[5] km/s
Proper motion (μ) RA: +4.940 mas/yr[1]
Dec.: −8.876 mas/yr[1]
Parallax (π)4.419 ± 0.029 mas[1]
Distance738 ± 5 ly
(226 ± 1 pc)
Absolute magnitude (MV)−0.34[6]
Details
Mass1.2[7] M☉
Radius41.18[8] R☉
Luminosity329±5[9] L☉
Surface gravity (log g)1.24[7] cgs
Temperature4,007±122[8] K
Metallicity [Fe/H]+0.14[7] dex
Rotational velocity (v sin i)1.8±1.2[10] km/s
Other designations
12 G. Volantis, CD−64°273, CPD−64°721, FK5 2584, GC 10057, HD 60150, HIP 36346, HR 2888, SAO 249864[11][12]
Database references
SIMBADdata

HD 60150 (HR 2888) is a solitary star located in the southern circumpolar constellation Volans. It has an apparent magnitude of 6.39, placing it near the limiting magnitude for naked-eye visibility. Parallax measurements place the star at a distance of 738 light years and it is currently receding with a heliocentric radial velocity of 13.4 km/s.[5]

HD 60150 has a classification of K5 III,[3] indicating that it is a red giant. It has 1.2 times the mass of the Sun[7] but has expanded to 41 times its girth.[8] It radiates 329 times the luminosity of the Sun[9] from its swollen photosphere at an effective temperature of 4,007 K,[8] giving it a reddish orange hue. HD 60150 is metal enriched, with an iron abundance 38% greater than the Sun.[8] It spins leisurely with projected rotational velocity of about 1.8 km/s.[10]

See also

References

  1. ^ a b c d Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
  3. ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0. Bibcode:1975mcts.book.....H.
  4. ^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
  5. ^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
  6. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. ISSN 1063-7737. S2CID 119257644.
  7. ^ a b c d Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. ISSN 0004-6361.
  8. ^ a b c d e Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256.
  9. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  10. ^ a b De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics. 561: A126. arXiv:1312.3474. Bibcode:2014A&A...561A.126D. doi:10.1051/0004-6361/201220762. ISSN 0004-6361.
  11. ^ "HR 2888". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 21, 2022.
  12. ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.
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