Zeta Serpentis: Difference between revisions

Zeta Serpentis
Observation data; Epoch J2000 Equinox J2000
Constellation	Serpens
Right ascension	18h 00m 29.0s
Declination	−03° 41′ 25″
Apparent magnitude (V)	4.63
Characteristics
Spectral type	F2V
B−V color index	+0.36
Astrometry
Radial velocity (Rv)	-50.70 km/s
Proper motion (μ)	RA: +155.51 mas/yr ; Dec.: -44.43 mas/yr
Parallax (π)	42.46 ± 0.34 mas
Distance	76.8 ± 0.6 ly ; (23.6 ± 0.2 pc)
Absolute magnitude (MV)	2.77
Other designations
	57 Serpentis, GC 24503, HIP 88175, HR 6710, HD 164259, SAO 142025
Database references
SIMBAD	data

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Zeta Serpentis (ζ Ser, ζ Serpentis) is a star in the constellation Serpens.

Zeta Serpentis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.63.^[3] It is approximately 76.8 light years from Earth.^[2] This star has nearly double the radius of the Sun and is radiating 6.3 times the Sun's luminosity from its outer atmosphere at an effective temperature of 6,529 K.^[1]

References

^ ^a ^b ^c Boyajian, Tabetha S.; et al. (February 2012), "Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars", The Astrophysical Journal, 746 (1): 101, arXiv:1112.3316, Bibcode:2012ApJ...746..101B, doi:10.1088/0004-637X/746/1/101. See Table 10.
^ ^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. Vizier catalog entry
^ ^a ^b ^c ^d "Zeta Serpentis". SIMBAD Astronomical Database. Retrieved 2015-10-17.
^ Gray, R. O.; et al. (October 2003), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.", The Astronomical Journal, 126 (4): 2048–2059, arXiv:astro-ph/0308182, Bibcode:2003AJ....126.2048G, doi:10.1086/378365
^ 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. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
^ Absolute magnitude calculated as $M=m+5(1+\log _{10}{p})\!\,$ , where $M$ is the star's absolute magnitude, $m$ is the star's apparent magnitude, and $p$ is the star's measured parallax in arcseconds.

This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it.

[apj746_1_101-1] Boyajian, Tabetha S.; et al. (February 2012), "Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars", The Astrophysical Journal, 746 (1): 101, arXiv:1112.3316, Bibcode:2012ApJ...746..101B, doi:10.1088/0004-637X/746/1/101. See Table 10.

[vanLeeuwen2007-2] ^ ^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. Vizier catalog entry

[SIMBAD-3] "Zeta Serpentis". SIMBAD Astronomical Database. Retrieved 2015-10-17.

[Gray2003-4] Gray, R. O.; et al. (October 2003), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.", The Astronomical Journal, 126 (4): 2048–2059, arXiv:astro-ph/0308182, Bibcode:2003AJ....126.2048G, doi:10.1086/378365

[Gontcharov2006-5] 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. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.

[6] Absolute magnitude calculated as $M=m+5(1+\log _{10}{p})\!\,$ , where $M$ is the star's absolute magnitude, $m$ is the star's apparent magnitude, and $p$ is the star's measured parallax in arcseconds.

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[2]

[3]

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[6]

@@ Line 1: / Line 1: @@
 {{Refimprove|date=August 2009}}
-{{Starbox short
+{{Starbox begin
- | name=ζ Serpentis
+| name = Zeta Serpentis
- | epoch=[[J2000.0]]
- | constell=[[Serpens]]
- | ra={{RA|18|00|29.0}}<ref name=apj746_1_101/>
- | dec={{DEC|-03|41|25}}<ref name=apj746_1_101/>
- | spectral=F3V
- | appmag_v=+4.62
- | dist_ly=75.7 ± 1.3
- | dist_pc=23.2 ± 0.4
- | names=57&nbsp;Serpentis, [[Star catalogue#BS, BSC, HR|HR]]&nbsp;6710,<BR/>[[Henry Draper Catalogue|HD]]&nbsp;164259, [[Star catalogue#SAO|SAO]]&nbsp;142025,<BR/>[[Hipparcos|HIP]]&nbsp;88175
 }}
+{{Starbox observe
+| epoch = J2000
+| constell = [[Serpens (constellation)|Serpens]]
+| ra={{RA|18|00|29.0}}<ref name=apj746_1_101/> <ref name=vanLeeuwen2007>{{cite journal | title=Validation of the new Hipparcos reduction | url=http://www.aanda.org/articles/aa/full/2007/41/aa8357-07/aa8357-07.html | last1=van Leeuwen | first1=F. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | date=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2088175 Vizier catalog entry]</ref>
+| dec={{DEC|-03|41|25}}<ref name=apj746_1_101/> <ref name=vanLeeuwen2007/>
+| appmag_v = 4.63 <ref name=SIMBAD>{{cite web | title=Zeta Serpentis | work=SIMBAD Astronomical Database | url=http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=Zeta+Serpentis | accessdate=2015-10-17 }}</ref>
+}}
+{{Starbox character
+| class = F2V <ref name=Gray2003>{{citation | display-authors=1 | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Robinson | first5=P. E. | title=Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I. | journal=The Astronomical Journal | volume=126 | issue=4 | pages=2048–2059 |date=October 2003 | doi=10.1086/378365 | bibcode=2003AJ....126.2048G |arxiv = astro-ph/0308182 }}</ref>
+| b-v = +0.36 <ref name=SIMBAD/>
+}}
+{{Starbox astrometry
+| radial_v = -50.70<ref name=Gontcharov2006>{{Cite journal | doi = 10.1134/S1063773706110065 | bibcode=2006AstL...32..759G | title = Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system | journal = Astronomy Letters | volume = 32 | issue = 11 | pages = 759–771 | date = November 2006 | last1 = Gontcharov | first1 = G. A.}}</ref>
+| prop_mo_ra = +155.51<ref name=vanLeeuwen2007/>
+| prop_mo_dec = -44.43<ref name=vanLeeuwen2007/>
+| parallax = 42.46
+| p_error = 0.34
+| parallax_footnote = <ref name=vanLeeuwen2007/>
+| absmag_v = 2.77 <ref>Absolute magnitude calculated as <math> M = m + 5 (1 + \log_{10}{p})\!\,</math>, where <math>M</math> is the star's absolute magnitude, <math>m</math> is the star's apparent magnitude, and <math>p</math> is the star's measured parallax in arcseconds.</ref>
+}}
+{{Starbox catalog
+| names = 57&nbsp;Serpentis, [[Boss General catalogue|GC]]&nbsp;24503, [[Hipparcos catalogue|HIP]]&nbsp;88175, [[Harvard Revised catalogue|HR]]&nbsp;6710, [[Henry Draper Catalogue|HD]]&nbsp;164259, [[Smithsonian Astrophysical Observatory catalogue|SAO]]&nbsp;142025 <ref name=SIMBAD/>
+}}
+{{Starbox reference
+| Simbad = Zeta+Serpentis
+}}
+{{Starbox end}}
 '''Zeta Serpentis''' (ζ Ser, ζ Serpentis) is a [[star]] in the [[constellation]] [[Serpens]].
-Zeta Serpentis is a yellow-white [[stellar classification|F-type]] [[main sequence|main sequence dwarf]] with an [[apparent magnitude]] of +4.62.  It is approximately 75.7 [[light years]] from [[Earth]]. This star has nearly double the radius of the Sun and is radiating 6.3 times the Sun's luminosity from its [[stellar atmosphere|outer atmosphere]] at an [[effective temperature]] of 6,529&nbsp;K.<ref name=apj746_1_101/>
+Zeta Serpentis is a yellow-white [[stellar classification|F-type]] [[main sequence|main sequence dwarf]] with an [[apparent magnitude]] of +4.63.<ref name=SIMBAD/>  It is approximately 76.8 [[light years]] from [[Earth]].<ref name=vanLeeuwen2007/> This star has nearly double the radius of the Sun and is radiating 6.3 times the Sun's luminosity from its [[stellar atmosphere|outer atmosphere]] at an [[effective temperature]] of 6,529&nbsp;K.<ref name=apj746_1_101/>
 ==References==
@@ Line 28: / Line 46: @@
 [[Category:Serpens (constellation)]]
 [[Category:F-type main-sequence stars]]
+[[Category:Hipparcos objects|088175]]
+[[Category:HR objects|6710]]
+[[Category:Henry Draper Catalogue objects|164259]]

Observation data Epoch J2000 Equinox J2000
Constellation	Serpens
Right ascension	18^h 00^m 29.0^s^[1] ^[2]
Declination	−03° 41′ 25″^[1] ^[2]
Apparent magnitude (V)	4.63 ^[3]
Characteristics
Spectral type	F2V ^[4]
B−V color index	+0.36 ^[3]
Astrometry

Radial velocity (R_v)	-50.70^[5] km/s
Proper motion (μ)	RA: +155.51^[2] mas/yr Dec.: -44.43^[2] mas/yr
Parallax (π)	42.46 ± 0.34 mas^[2]
Distance	76.8 ± 0.6 ly (23.6 ± 0.2 pc)
Absolute magnitude (M_V)	2.77 ^[6]

Other designations
57 Serpentis, GC 24503, HIP 88175, HR 6710, HD 164259, SAO 142025 ^[3]
Database references
SIMBAD	data