Epsilon Serpentis

{{Short description|Am star in the constellation Serpens}}

{{Starbox begin

| name = ε Serpentis

}}

{{Starbox image

| image=

{{Location mark

|image=Serpens constellation map.svg|alt=|float=center|width=280

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=ε Serpentis

|x=818|y=400

}}

|caption=Location of ε Serpentis (circled)

}}

{{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

}}

{{Starbox character

| class = kA2hA5mA7 V

| b-v = +0.14

| u-b = +0.12

| r-i =

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|−9.4|0.6}}

| prop_mo_ra = +128.19

| prop_mo_dec = +62.16

| parallax = 46.30

| p_error = 0.19

| parallax_footnote =

| absmag_v = +2.04

}}

{{Starbox detail

| source =

| mass = {{Val|1.820|0.026}}

| radius = {{Val|1.783|0.040}}

| luminosity = {{Val|12.134|0.296}}

| temperature = {{Val|7928|88|fmt=commas}}

| gravity = 4.346

| metal_fe = +0.38

| rotational_velocity = 33.1

| rotation =

| age_myr = {{Val|500|200}}

}}

{{Starbox catalog

| names = {{odlist | B=ε Ser | F=37 Serpentis | BD=+04°3069 | HD=141795 | HIP=77622 | HR=5892 | SAO=121218 }}

}}

{{Starbox reference

| Simbad = eps+Ser

}}

{{starbox end}}

Epsilon Serpentis, Latinized from ε Serpentis, is a single, 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. 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.

This is an Am star on the main-sequence with a stellar classification of kA2hA5mA7 V. 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. It has been examined for the presence of a magnetic field, but the detected level was not statistically significant.

Epsilon Serpentis has an estimated 1.82 times the mass of the Sun and 1.78 times the Sun's radius. The star is radiating 12 times the Sun's luminosity from its photosphere at an effective temperature of around 7,928 K. 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. The star is around half a billion years old and is spinning with a projected rotational velocity of 33.1 km/s.

Etymology

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

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).

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 represents eleven old states in China and which marks 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.{{in lang|zh}} 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}}. Consequently, the Chinese name for ε Serpentis itself is {{lang|zh|天市右垣八}} ({{lang|zh-Latn|Tiān Shì Yòu Yuán bā}}, {{langx|en|the Eighth Star of Right Wall of Heavenly Market Enclosure}}), represent the state Ba (巴) (or Pa).{{in lang|zh}} [http://aeea.nmns.edu.tw/2006/0606/ap060624.html AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 24 日] {{Webarchive|url=https://web.archive.org/web/20190404010915/http://aeea.nmns.edu.tw/2006/0606/ap060624.html |date=2019-04-04 }}{{in lang|zh}} [http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/e_research_chinengstarzone_b.htm#HeavenlyMarketEnclosure 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.

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{{cite simbad | mode=cs2

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}}

{{Stars of Serpens|state=collapsed}}

{{DEFAULTSORT:Epsilon Serpentis}}

Category:A-type main-sequence stars

Category:Am stars

Category:Circumstellar disks

Serpentis, Epsilon

Category:Serpens

Category:Durchmusterung objects

Serpentis, 37

141795

077622

5892

Nasak Yamani II