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词条 Epsilon Serpentis
释义

  1. Etymology

  2. References

{{Starbox begin
| name = Epsilon Serpentis
}}{{Starbox observe
| epoch = J2000.0
| equinox = J2000.0 (ICRS)
| constell = Serpens
| ra = {{RA|15|50|48.96622}}
| dec = {{DEC|+04|28|39.8311}}
| appmag_v = +3.69[3]
}}{{Starbox character
| class = kA2hA5mA7 V[4]
| b-v = +0.14[3]
| u-b = +0.12[3]
| r-i =
| variable =
}}{{Starbox astrometry
| radial_v = {{Val|−9.4|0.6}}[7]
| prop_mo_ra = +128.19
| prop_mo_dec = +62.16
| parallax = 46.30
| p_error = 0.19
| parallax_footnote =
| absmag_v = +2.04[11]
}}{{Starbox detail
| source =
| mass = {{Val|1.820|0.026}}[12]
| radius = {{Val|1.783|0.040}}[12]
| luminosity = {{Val|12.134|0.296}}[12]
| temperature = {{Val|7928|88|fmt=commas}}[15]
| gravity = 4.346[15]
| metal_fe = +0.38[15]
| rotational_velocity = 33.1[15]
| rotation =
| age_myr = {{Val|500|200}}[12]
}}{{Starbox catalog
| names = {{odlist | B=ε Ser | F=37 Serpentis | HD=141795 | HIP=77622 | HR=5892 | SAO=121218 }}[20]
}}{{Starbox reference
| Simbad = eps+Ser
}}{{starbox end}}Epsilon Serpentis, Latinized from ε Serpentis, is a single,[21] white-hued star in the constellation Serpens, in its head (Serpens Caput). It is visible to the naked eye with an apparent visual magnitude of +3.69.[3] Based upon an annual parallax shift of 46.30 mas as seen from Earth, it is located 70 light years from the Sun. It is moving closer to the Sun with a radial velocity of −9 km/s.[7]

This is an Am star[25] on the main-sequence with a stellar classification of kA2hA5mA7 V.[4] This notation indicates the spectrum displays the calcium K-line of an A2 star, the hydrogen lines of an A5 star, and the metal lines of an A7 star.[27] It has been examined for the presence of a magnetic field, but the detected level was not statistically significant.[28]

Epsilon Serpentis has an estimated 1.82 times the mass of the Sun and 1.78 times the Sun's radius.[12] The star is radiating 12[12] times the Sun's luminosity from its photosphere at an effective temperature of around 7,928 K.[15] It is a candidate for an infrared excess at a wavelength of 25 μm, suggesting a circumstellar disk of dust with a temperature of {{Val|250|70|u=K}} may be orbiting roughly 4.2 AU from the host star.[32] The star is around half[12] a billion years old and is spinning with a projected rotational velocity of 33.1 km/s.[15]

Etymology

Epsilon Serpentis was a member of indigenous Arabic asterism al-Nasaq al-Yamānī, "the Southern Line" of al-Nasaqān "the Two Lines".[35] along with α Ser (Unukalhai), δ Ser, δ Oph (Yed Prior), ε Oph (Yed Posterior), ζ Oph and γ Oph.[36]

According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Yamānī or Nasak Yamani were the title for two stars :δ Ser as Nasak Yamani I and ε Ser as Nasak Yamani II (exclude α Ser, δ Oph, ε Oph, ζ Oph and γ Oph).[37]

In Chinese, {{lang|zh|天市右垣}} ({{lang|zh-Latn|Tiān Shì Yòu Yuán}}), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of ε Serpentis, β Herculis, γ Herculis, κ Herculis, γ Serpentis, β Serpentis, α Serpentis, δ Serpentis, δ Ophiuchi, ε Ophiuchi and ζ Ophiuchi.[1] Consequently, ε Serpentis itself is known as {{lang|zh|天市右垣八}} ({{lang|zh-Latn|Tiān Shì Yòu Yuán bā}}, {{lang-en|the Eighth Star of Right Wall of Heavenly Market Enclosure}}), represent the state Ba (巴) (or Pa).[39][2][3]

References

1. ^{{zh icon}} 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, {{ISBN|978-986-7332-25-7}}.
2. ^{{zh icon}} AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 24 日
3. ^{{zh icon}} English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name {{webarchive |url=https://web.archive.org/web/20100810114313/http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/e_research_chinengstarzone_b.htm#HeavenlyMarketEnclosure |date=August 10, 2010 }}, Hong Kong Space Museum. Accessed on line November 23, 2010.
4. ^{{citation | title=Spectral Atlas for Amateur Astronomers: A Guide to the Spectra of Astronomical Objects and Terrestrial Light Sources | first1=Richard | last1=Walker | postscript=. | publisher=Cambridge University Press | year=2017 | isbn=1316738760 | page=116 | url=https://books.google.com/books?id=oQQvDwAAQBAJ&pg=PA116 }}
5. ^{{citation | title=A highly sensitive search for magnetic fields in B, A and F stars | display-authors=1 | last1=Shorlin | first1=S. L. S. | last2=Wade | first2=G. A. | last3=Donati | first3=J.-F. | last4=Landstreet | first4=J. D. | last5=Petit | first5=P. | last6=Sigut | first6=T. A. A. | last7=Strasser | first7=S. | journal=Astronomy and Astrophysics | postscript=. | volume=392 | pages=637–652 | date=September 2002 | doi=10.1051/0004-6361:20021192 | bibcode=2002A&A...392..637S }}
6. ^{{citation | title=Elemental abundance analyses with DAO spectrograms - XX | last1=Adelman | first1=Saul J. | last2=Albayrak | first2=Berahitdin | journal=Monthly Notices of the Royal Astronomical Society | volume=300 | issue=2 | pages=359–372 | date=October 1998 | doi=10.1046/j.1365-8711.1998.01859.x | bibcode=1998MNRAS.300..359A }}
7. ^{{citation | title=Warm dusty discs: exploring the A star 24 μm debris population | last1=Smith | first1=R. | last2=Wyatt | first2=M. C. | journal=Astronomy and Astrophysics | volume=515 | id=A95 | pages=16 | date=June 2010 | doi=10.1051/0004-6361/200913481 | bibcode=2010A&A...515A..95S | arxiv=1004.0644 | postscript=. }}
8. ^{{citation | last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C. | title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project | journal=Astronomy & Astrophysics | volume=546 | id=A61 | pages=14 | date=October 2012 | doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D | arxiv=1208.3048 | postscript=. }}
9. ^{{citation | display-authors=1 | last1=Rodriguez | first1=David R. | last2=Duchêne | first2=Gaspard | last3=Tom | first3=Henry | last4=Kennedy | first4=Grant M. | last5=Matthews | first5=Brenda | last6=Greaves | first6=Jane | last7=Butner | first7=Harold | title=Stellar multiplicity and debris discs: an unbiased sample | journal=Monthly Notices of the Royal Astronomical Society | volume=449 | issue=3 | pages=3160–3170 | date=May 2015 | doi=10.1093/mnras/stv483 | arxiv=1503.01320 | bibcode=2015MNRAS.449.3160R | postscript=. }}
10. ^{{citation | title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets | last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A. | journal=The Astrophysical Journal | volume=804 | issue=2 | pages=146 | year=2015 | bibcode=2015ApJ...804..146D | doi=10.1088/0004-637X/804/2/146 | arxiv=1501.03154 | postscript=. }}
11. ^{{citation | title=Photoelectric UBVRI observations of Am stars | journal=Astronomical Journal |volume=79|pages=1290 | last1=Feinstein | first1=A. | postscript=. | year=1974 | bibcode=1974AJ.....79.1290F | doi=10.1086/111675 }}
12. ^{{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=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=The Astronomical Journal | volume=132 | issue=1 | pages=161–170 | date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | postscript=. }}
13. ^{{citation | last=Kunitzsch, P. | first=Smart, T., | year=2006 | title=A Dictionary of Modern Star names: A Short Guide to 254 Star names and Their Derivations | edition=Second Revised | publisher=Sky Publishing | location=Cambridge, MA | isbn=1-931559-44-9 | page=31 | postscript=. }}
14. ^{{cite book | last=Allen | first=R. H. | year=1963 | authorlink=Richard Hinckley Allen | title=Star Names: Their Lore and Meaning | url=http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Hercules*.html | accessdate=2010-12-12 | edition=Reprint | publisher=Dover Publications Inc | location=New York, NY | isbn=0-486-21079-0 | page=243 }}
15. ^{{citation | url=http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Serpens*.html | title=Star Names | chapter=Serpens | first1=Richard Hinckley | last1=Allen | pages=376 | date=1963 }}
16. ^{{citation | url=https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19720005197_1972005197.pdf | first1=Jack W. | last1=Rhoads | title=Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars | location=Jet Propulsion Laboratory, California Institute of Technology | date=November 15, 1971 | postscript=. }}
17. ^{{citation | display-authors=1 | last1=Boyajian | first1=Tabetha S. | last2=McAlister | first2=Harold A. | last3=van Belle | first3=Gerard | last4=Gies | first4=Douglas R. | last5=ten Brummelaar | first5=Theo A. | last6=von Braun | first6=Kaspar | last7=Farrington | first7=Chris | last8=Goldfinger | first8=P. J. | last9=O'Brien | first9=David | last10=Parks | first10=J. Robert | last11=Richardson | first11=Noel D. | last12=Ridgway | first12=Stephen | last13=Schaefer | first13=Gail | last14=Sturmann | first14=Laszlo | last15=Sturmann | first15=Judit | last16=Touhami | first16=Yamina | last17=Turner | first17=Nils H. | last18=White | first18=Russel | title=Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars | journal=The Astrophysical Journal | postscript=. | volume=746 | issue=1 | page=101 | date=February 2012 | doi=10.1088/0004-637X/746/1/101 | bibcode=2012ApJ...746..101B | arxiv=1112.3316 }}. See Table 10.
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19. ^{{cite simbad | title=eps Ser | accessdate=2017-09-26 | postscript=. }}
[4][5][6][7][8][9][10][11][12][13][14][15][16][17][18][19]
}}{{Stars of Serpens|state=collapsed}}

10 : A-type main-sequence stars|Am stars|Circumstellar disks|Bayer objects|Serpens (constellation)|Durchmusterung objects|Flamsteed objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

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