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词条 3 Serpentis
释义

  1. References

{{Starbox begin
| name = 3 Serpentis
}}{{Starbox observe
| epoch = J2000
| constell = Serpens
| ra = {{RA|15|15|11.352}}[1]
| dec = {{DEC|+04|56|21.71}}[1]
| appmag_v = 5.337[3]
}}{{Starbox character
| class = K0III[4]
| r-i =
| v-r =
| b-v =
| u-b =
| variable =
}}{{Starbox astrometry
| radial_v =
| prop_mo_ra = {{val|−24.90|0.81}}[1]
| prop_mo_dec = {{val|4.80|0.54}}[1]
| parallax = 8.74
| p_error = 0.75
| parallax_footnote = [1]
| absmag_v = +1.15[8]
}}{{Starbox orbit
| reference = [9]
| period = {{val|66|5}}
| axis = {{val|229|2}}
| inclination = {{val|132|4}}
| eccentricity = {{val|0.962|0.005}}
}}{{Starbox detail
| mass =
| radius =
| luminosity =
| temperature = 4,550
| metal_fe = +0.03
| gravity = +2.77
| rotational_velocity = 1.5[13]
| age_gyr =
}}{{Starbox catalog
| names = {{ odlist | BD=+05° 2985 | FK5=562 | HD=135482 | HIP=74649 | HR=5675 | SAO=120916 }}[14]
}}{{Starbox reference
| Simbad = HD+135482
}}{{Starbox end}}

3 Serpentis is a binary star in the constellation Serpens with an orbital period of approximately 66 years. It is dimly visible to the naked eye with an apparent magnitude of 5.337. Located around {{convert|114|pc|ly}} distant, it is an orange giant of spectral type K0III, a star that has used up its core hydrogen.

The two components of 3 Serpentis can be resolved using speckle interferometry and were separated by 0.23" in 2014. The orbit is highly eccentric and at periastron passage in 1997, the two are calculated to have been only 6 mas apart.[9]

Individual spectra for the two components of 3 Serpentis cannot be obtained and the spectral type of K0III is for the two stars combined. The primary is 2.5 magnitudes brighter than the secondary and cooler. The combined spectral type indicates that the primary is likely to have evolved away from the main sequence, but comparison of the colour and brightness of the secondary suggest it is still a main sequence star.[9]

References

1. ^{{cite journal | title=Observations of Binary Stars with the Differential Speckle Survey Instrument. VI. Measures during 2014 at the Discovery Channel Telescope | url=http://iopscience.iop.org/article/10.1088/0004-6256/150/5/151/meta | journal=The Astronomical Journal | volume=150 | issue=5 | page=151 | year=2015 | last1=Horch | first1=Elliott P. | last2=Belle | first2=Gerard T. van | last3=Davidson, Jr. | first3=James W. | last4=Ciastko | first4=Lindsay A. | last5=Everett | first5=Mark E. | last6=Bjorkman | first6=Karen S. | display-authors=1 | arxiv=1509.03498 | bibcode=2015AJ....150..151H | doi=10.1088/0004-6256/150/5/151 }}
2. ^{{ cite simbad | title=* 3 Ser | accessdate=20 July 2014 }}
3. ^{{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 | year=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 }}Vizier catalog entry
4. ^{{cite journal|bibcode=2000A&A...363..239D|title=Rotation and lithium in single giant stars|arxiv=astro-ph/0010273}}
5. ^{{cite journal|doi=10.1086/191527|title=High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances|journal=The Astrophysical Journal Supplement Series|volume=74|pages=1075|year=1990|last1=McWilliam|first1=Andrew|bibcode=1990ApJS...74.1075M}}
6. ^{{cite journal|bibcode=2000A&A...355L..27H|title=The Tycho-2 catalogue of the 2.5 million brightest stars}}
7. ^{{cite journal|bibcode= 2007MNRAS.374..664C|title=Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters|arxiv=astro-ph/0611618|doi=10.1111/j.1365-2966.2006.11196.x}}
[1][2][3][4][5][6][7]
}}{{Stars of Serpens}}

7 : Serpens (constellation)|Flamsteed objects|K-type giants|Durchmusterung objects|HR objects|Henry Draper Catalogue objects|Hipparcos objects

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