| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Serpens |
| Right ascension | 15h 51m 15.90985s [3] |
| Declination | +20° 58′ 40.5166″ [3] |
| Apparent magnitude (V) | 4.78 [4] |
| Characteristics | |
| Spectral type | K4.5III [5] |
| U−B color index | +1.88 [4] |
| B−V color index | +1.54 [4] |
| Astrometry | |
| Radial velocity (Rv) | −61.96 [6] km/s |
| Proper motion (μ) |
RA: −53.32
[3]
mas/
yr Dec.: +18.87 [3] mas/ yr |
| Parallax (π) | 8.70 ± 0.30 mas [3] |
| Distance | 370 ± 10
ly (115 ± 4 pc) |
| Absolute magnitude (MV) | −0.56 [7] |
| Details | |
| Radius | 47.84+0.49 −1.19 [8] R☉ |
| Luminosity | 491.9±22.3 [8] L☉ |
| Surface gravity (log g) | 1.68 [9] cgs |
| Temperature | 3,930+50 −20 [8] K |
| Metallicity [Fe/H] | −0.08 [7] dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
Rho Serpentis, Latinized from ρ Serpentis, is a single [11] star in the Caput section of the equatorial Serpens constellation. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.78. [4] The distance to this star is approximately 375 light years based on parallax, [3] but it is drifting closer to the Sun with a radial velocity of −62 km/s. [6]
This is an aging giant star with a stellar classification of K4.5III. [5] It is a suspected variable star of unknown type, with an I-band brightness ranging from 3.29 down to 3.44 magnitude. [12] Hipparcos photometry revealed a microvariability with a frequency of 0.17017 cycles per day and an amplitude of 0.0080. [2] With the supply of hydrogen exhausted at its core, it has expanded and now has 48 [8] times the Sun's girth. The star is radiating 492 [8] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,930 K. [8]
- ^ "/ftp/cats/more/HIP/cdroms/cats", Centre de Données astronomiques de Strasbourg, Strasbourg astronomical Data Center, retrieved 15 October 2022.
- ^ a b Koen, Chris; Eyer, Laurent (2002). "New periodic variables from the Hipparcos epoch photometry". Monthly Notices of the Royal Astronomical Society. 331 (1): 45–59. arXiv: astro-ph/0112194. Bibcode: 2002MNRAS.331...45K. doi: 10.1046/j.1365-8711.2002.05150.x. S2CID 10505995.
- ^ 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. Vizier catalog entry
- ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode: 2002yCat.2237....0D.
- ^ a b Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode: 1989ApJS...71..245K. doi: 10.1086/191373.
- ^ a b Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv: astro-ph/0409579, Bibcode: 2005A&A...430..165F, doi: 10.1051/0004-6361:20041272, S2CID 17804304
- ^ a b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d e f 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.
- ^ McWilliam, Andrew (December 1990). "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances". Astrophysical Journal Supplement Series. 74: 1075–1128. Bibcode: 1990ApJS...74.1075M. doi: 10.1086/191527.
- ^ "rho Ser". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-17.
- ^ 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.
- ^ Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017), "General catalogue of variable stars: Version GCVS 5.1", Astronomy Reports, 61 (1): 80, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
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Star clusters |
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| Nebulae |
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| Galaxies |
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Serpens |
| Right ascension | 15h 51m 15.90985s [3] |
| Declination | +20° 58′ 40.5166″ [3] |
| Apparent magnitude (V) | 4.78 [4] |
| Characteristics | |
| Spectral type | K4.5III [5] |
| U−B color index | +1.88 [4] |
| B−V color index | +1.54 [4] |
| Astrometry | |
| Radial velocity (Rv) | −61.96 [6] km/s |
| Proper motion (μ) |
RA: −53.32
[3]
mas/
yr Dec.: +18.87 [3] mas/ yr |
| Parallax (π) | 8.70 ± 0.30 mas [3] |
| Distance | 370 ± 10
ly (115 ± 4 pc) |
| Absolute magnitude (MV) | −0.56 [7] |
| Details | |
| Radius | 47.84+0.49 −1.19 [8] R☉ |
| Luminosity | 491.9±22.3 [8] L☉ |
| Surface gravity (log g) | 1.68 [9] cgs |
| Temperature | 3,930+50 −20 [8] K |
| Metallicity [Fe/H] | −0.08 [7] dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
Rho Serpentis, Latinized from ρ Serpentis, is a single [11] star in the Caput section of the equatorial Serpens constellation. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.78. [4] The distance to this star is approximately 375 light years based on parallax, [3] but it is drifting closer to the Sun with a radial velocity of −62 km/s. [6]
This is an aging giant star with a stellar classification of K4.5III. [5] It is a suspected variable star of unknown type, with an I-band brightness ranging from 3.29 down to 3.44 magnitude. [12] Hipparcos photometry revealed a microvariability with a frequency of 0.17017 cycles per day and an amplitude of 0.0080. [2] With the supply of hydrogen exhausted at its core, it has expanded and now has 48 [8] times the Sun's girth. The star is radiating 492 [8] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,930 K. [8]
- ^ "/ftp/cats/more/HIP/cdroms/cats", Centre de Données astronomiques de Strasbourg, Strasbourg astronomical Data Center, retrieved 15 October 2022.
- ^ a b Koen, Chris; Eyer, Laurent (2002). "New periodic variables from the Hipparcos epoch photometry". Monthly Notices of the Royal Astronomical Society. 331 (1): 45–59. arXiv: astro-ph/0112194. Bibcode: 2002MNRAS.331...45K. doi: 10.1046/j.1365-8711.2002.05150.x. S2CID 10505995.
- ^ 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. Vizier catalog entry
- ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode: 2002yCat.2237....0D.
- ^ a b Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode: 1989ApJS...71..245K. doi: 10.1086/191373.
- ^ a b Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv: astro-ph/0409579, Bibcode: 2005A&A...430..165F, doi: 10.1051/0004-6361:20041272, S2CID 17804304
- ^ a b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b c d e f 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.
- ^ McWilliam, Andrew (December 1990). "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances". Astrophysical Journal Supplement Series. 74: 1075–1128. Bibcode: 1990ApJS...74.1075M. doi: 10.1086/191527.
- ^ "rho Ser". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-17.
- ^ 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.
- ^ Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017), "General catalogue of variable stars: Version GCVS 5.1", Astronomy Reports, 61 (1): 80, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
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|
Star clusters |
| ||||||||||||
| Nebulae |
| ||||||||||||
| Galaxies |
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