Rho2 Cancri: Difference between revisions
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{{Short description|Star in the constellation Cancer}} |
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{{DISPLAYTITLE:Rho<sup>2</sup> Cancri}} |
{{DISPLAYTITLE:Rho<sup>2</sup> Cancri}} |
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{{other stars by Bayer designation|Rho Cancri{{!}}ρ Cancri}} |
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| name = Rho<sup>2</sup> Cancri |
| name = Rho<sup>2</sup> Cancri |
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'''Rho<sup>2</sup> Cancri''' (ρ<sup>2</sup> Cancri) is a solitary,<ref name=Eggleton2008/> yellow-hued [[star]] in the [[constellation]] [[Cancer (constellation)|Cancer]]. With an [[apparent visual magnitude]] of 5.22,<ref name=Fernie1983/> it is visible to the naked eye on a dark night. Based upon an annual [[stellar parallax|parallax shift]] of 6.70 [[milliarcsecond|mas]] as seen from Earth,<ref name=vanLeeuwen2007/> this star is located around 490 [[light |
'''Rho<sup>2</sup> Cancri''' (ρ<sup>2</sup> Cancri) is a solitary,<ref name=Eggleton2008/> yellow-hued [[star]] in the [[constellation]] [[Cancer (constellation)|Cancer]]. With an [[apparent visual magnitude]] of 5.22,<ref name=Fernie1983/> it is visible to the naked eye on a dark night. Based upon an annual [[stellar parallax|parallax shift]] of 6.70 [[milliarcsecond|mas]] as seen from Earth,<ref name=vanLeeuwen2007/> this star is located around 490 [[light-year]]s from the [[Sun]]. At that distance, the visual magnitude is diminished by an [[extinction (astronomy)|extinction factor]] of 0.06 due to [[interstellar dust]].<ref name=Takeda2008/> |
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At the age of about 234<ref name=Takeda2008/> million years, is an [[stellar evolution|evolved]], [[G-type star|G-type]] [[giant star]] with a [[stellar classification]] of G8 III.<ref name=Henry2000/> It has an estimated 3.6<ref name=Takeda2008/> times the [[mass of the Sun]] and has expanded to 24<ref name=Henry2000/> times the [[Sun's radius]]. It is radiating 310<ref name=Henry2000/> times the [[Sun's luminosity]] from its [[photosphere]] at an [[effective temperature]] of |
At the age of about 234<ref name=Takeda2008/> million years, is an [[stellar evolution|evolved]], [[G-type star|G-type]] [[giant star]] with a [[stellar classification]] of G8 III.<ref name=Henry2000/> It has an estimated 3.6<ref name=Takeda2008/> times the [[mass of the Sun]] and has expanded to 24<ref name=Henry2000/> times the [[Sun's radius]]. It is radiating 310<ref name=Henry2000/> times the [[Sun's luminosity]] from its [[photosphere]] at an [[effective temperature]] of {{val|4994|ul=K|fmt=commas}}.<ref name=luck2014/> |
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==See also== |
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* [[55 Cancri]], or Rho<sup>1</sup> Cancri (ρ<sup>1</sup> Cnc) |
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==References== |
==References== |
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| volume=474 | issue=2 | pages=653–664 | date=2007 |
| volume=474 | issue=2 | pages=653–664 | date=2007 |
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| arxiv=0708.1752 | bibcode=2007A&A...474..653V |
| arxiv=0708.1752 | bibcode=2007A&A...474..653V |
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| doi=10.1051/0004-6361:20078357 | postscript=. }}</ref> |
| doi=10.1051/0004-6361:20078357 | s2cid=18759600 | postscript=. }}</ref> |
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<ref name=Takeda2008>{{citation |
<ref name=Takeda2008>{{citation |
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| journal=[[Monthly Notices of the Royal Astronomical Society]] |
| journal=[[Monthly Notices of the Royal Astronomical Society]] |
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| volume=389 | issue=2 | pages=869–879 | date=September 2008 |
| volume=389 | issue=2 | pages=869–879 | date=September 2008 |
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| doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E |
| doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | bibcode=2008MNRAS.389..869E |
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| arxiv=0806.2878 | postscript=. }}</ref> |
| arxiv=0806.2878 | s2cid=14878976 | postscript=. }}</ref> |
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<ref name=deBruijne2012>{{citation |
<ref name=deBruijne2012>{{citation |
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| volume=546 | id=A61 | pages=14 | date=October 2012 |
| volume=546 | id=A61 | pages=14 | date=October 2012 |
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| doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D |
| doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D |
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| arxiv=1208.3048 | postscript=. }}</ref> |
| arxiv=1208.3048 | s2cid=59451347 | postscript=. }}</ref> |
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<ref name=luck2014>{{citation |
<ref name=luck2014>{{citation |
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| journal=The Astrophysical Journal Supplement Series |
| journal=The Astrophysical Journal Supplement Series |
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| volume=130 | issue=1 | pages=201–225 | date=September 2000 |
| volume=130 | issue=1 | pages=201–225 | date=September 2000 |
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| doi=10.1086/317346 | bibcode=2000ApJS..130..201H | citeseerx=10.1.1.40.8526}}</ref> |
| doi=10.1086/317346 | bibcode=2000ApJS..130..201H | citeseerx=10.1.1.40.8526| s2cid=17160805 }}</ref> |
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<ref name=Fernie1983>{{citation |
<ref name=Fernie1983>{{citation |
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| journal=Astrophysical Journal Supplement Series |
| journal=Astrophysical Journal Supplement Series |
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| volume=52 | pages=7–22 | date=May 1983 |
| volume=52 | pages=7–22 | date=May 1983 |
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| doi=10.1086/190856 | bibcode=1983ApJS...52....7F }}</ref> |
| doi=10.1086/190856 | bibcode=1983ApJS...52....7F | doi-access=free }}</ref> |
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<ref name=SIMBAD>{{cite simbad |
<ref name=SIMBAD>{{cite simbad |
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| title=rho02 Cnc |
| title=rho02 Cnc |
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| access-date=2017-06-13 }}</ref> |
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}} |
}} |
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[[Category:Henry Draper Catalogue objects|076219]] |
[[Category:Henry Draper Catalogue objects|076219]] |
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[[Category:Hipparcos objects|043834]] |
[[Category:Hipparcos objects|043834]] |
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[[Category: |
[[Category:Bright Star Catalogue objects|3540]] |
Latest revision as of 12:04, 11 November 2024
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Cancer |
Right ascension | 08h 55m 39.68055s[1] |
Declination | +27° 55′ 38.9299″[1] |
Apparent magnitude (V) | 5.22[2] |
Characteristics | |
Spectral type | G8 III[3] or G8 II-III[4] |
U−B color index | +0.78[2] |
B−V color index | +1.00[2] |
Astrometry | |
Radial velocity (Rv) | +16.3±0.3[5] km/s |
Proper motion (μ) | RA: −12.24[1] mas/yr Dec.: −33.79[1] mas/yr |
Parallax (π) | 6.70 ± 0.32 mas[1] |
Distance | 490 ± 20 ly (149 ± 7 pc) |
Absolute magnitude (MV) | −1.13[3] |
Details | |
Mass | 3.59[6] M☉ |
Radius | 24.2[3] R☉ |
Luminosity | 310[3] L☉ |
Surface gravity (log g) | 2.46[7] cgs |
Temperature | 4,994[7] K |
Metallicity [Fe/H] | 0.11[7] dex |
Rotational velocity (v sin i) | 8.1[3] km/s |
Age | 234[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Rho2 Cancri (ρ2 Cancri) is a solitary,[4] yellow-hued star in the constellation Cancer. With an apparent visual magnitude of 5.22,[2] it is visible to the naked eye on a dark night. Based upon an annual parallax shift of 6.70 mas as seen from Earth,[1] this star is located around 490 light-years from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.06 due to interstellar dust.[6]
At the age of about 234[6] million years, is an evolved, G-type giant star with a stellar classification of G8 III.[3] It has an estimated 3.6[6] times the mass of the Sun and has expanded to 24[3] times the Sun's radius. It is radiating 310[3] times the Sun's luminosity from its photosphere at an effective temperature of 4,994 K.[7]
See also
[edit]- 55 Cancri, or Rho1 Cancri (ρ1 Cnc)
References
[edit]- ^ 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&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
- ^ a b c d Fernie, J. D. (May 1983), "New UBVRI photometry for 900 supergiants", Astrophysical Journal Supplement Series, 52: 7–22, Bibcode:1983ApJS...52....7F, doi:10.1086/190856.
- ^ a b c d e f g h Henry, Gregory W.; et al. (September 2000), "Photometric Variability in a Sample of 187 G and K Giants", The Astrophysical Journal Supplement Series, 130 (1): 201–225, Bibcode:2000ApJS..130..201H, CiteSeerX 10.1.1.40.8526, doi:10.1086/317346, S2CID 17160805
- ^ a b Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
- ^ a b c d e Takeda, Yoichi; et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants", Publications of the Astronomical Society of Japan, 60 (4): 781–802, arXiv:0805.2434, Bibcode:2008PASJ...60..781T, doi:10.1093/pasj/60.4.781.
- ^ a b c d Luck, R. Earle (2014), "Parameters and Abundances in Luminous Stars", The Astronomical Journal, 147 (6): 137, Bibcode:2014AJ....147..137L, doi:10.1088/0004-6256/147/6/137.
- ^ "rho02 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-13.