Xi Scorpii

{{Short description|Star system}}

{{Sky|16|04|22.1|−|11|22|23|92.5}}

{{Starbox begin}}

{{Starbox observe 3s

|epoch=J2000

|constell=Scorpius

|component1=ξ Sco ABC

|ra1={{RA|16|04|22.191}}{{cite journal|title=A new star catalogue of SAO type|author1=Roeser, S.|author2=Bastian, U.|journal=Astronomy and Astrophysics Supplement Series|volume=74|pages=449–451|date=1988|bibcode=1988A&AS...74..449R}}

|dec1={{DEC|-11|22|22.60}}

|appmag_v1=4.17{{cite simbad|title=* ksi Sco|access-date=2 August 2017}}
(5.16 / 4.87 / 7.30)

|component2=Component D

|ra2={{RA|16|04|25.9260}}

|dec2={{DEC|-11|26|57.778}}

|appmag_v2=7.43{{cite simbad|title=HD 144087|access-date=2 August 2017}}

|component3=Component E

|ra3={{RA|16|04|26.7188}}

|dec3={{DEC|-11|26|59.553}}

|appmag_v3=7.81{{cite simbad|title=HD 144088|access-date=2 August 2017}}

}}

{{Starbox character

|component1=ξ Sco ABC

|class=F4(V) + F6(V) + G1V{{cite journal|title=VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications|author=Skiff, B. A.|journal=VizieR On-line Data Catalog|volume=1|date=2014|bibcode=2014yCat....1.2023S}}

|b-v=+0.45{{cite journal|author1=Mermilliod, J.-C.|title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)|journal=Catalogue of Eggen's UBV Data|url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?1986EgUBV........0M&db_key=AST&nosetcookie=1|date=1986|bibcode= 1986EgUBV........0M}}

|u-b=+0.00

|component2=Components DE

|class2=K1(V) + K1(V){{cite journal|bibcode=1999MSS...C05....0H|title=Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5|journal=Michigan Spectral Survey|volume=5|pages=0|author1=Houk, N.|author2=Swift, C.|year=1999}}

|b-v2=+0.75

|u-b2=+0.315

}}

{{Starbox astrometry

|component1=ξ Sco ABC

|radial_v={{val|-36.33|0.83}}{{cite journal|bibcode=2002A&A...382..118T|doi=10.1051/0004-6361:20011586|title=Statistics of spectroscopic sub-systems in visual multiple stars|journal=Astronomy & Astrophysics|volume=382|pages=118–123|year=2002|last1=Tokovinin|first1=A. A.|last2=Smekhov|first2=M. G.|url=https://zenodo.org/record/896317|doi-access=free}}

|prop_mo_ra=−63.2

|prop_mo_dec=−27.0

|parallax=

|p_error=

|parallax_footnote=

}}

{{Starbox astrometry|no_heading=y

|component1=Component D

|radial_v={{val|-31.96|0.13}}

|prop_mo_ra=−61.607

|prop_mo_dec=−22.227

|parallax=35.8898

|p_error=0.0200

|parallax_footnote={{cite Gaia DR3|4343064577465522816}}

|absmag_v=4.47

|component2=Component E

|radial_v2={{val|-32.28|0.12}}

|prop_mo_ra2=−56.334

|prop_mo_dec2=−20.357

|parallax2=35.8718

|p_error2=0.0237

|parallax_footnote2={{cite Gaia DR3|4343064508746082304}}

|absmag_v2=5.18{{cite journal

| last1=Boro Saikia |first1=S. |last2=Marvin |first2=C. J.

| last3=Jeffers |first3=S. V. |last4=Reiners |first4=Ansgar

| last5=Cameron |first5=R. |last6=Marsden |first6=S. C.

| last7=Petit |first7=P. |last8=Warnecke |first8=J.

| last9=Yadav |first9=A. P. |last10=Teske |first10=J. K.

| last11=Shectman |first11=S. A. |last12=Crane |first12=J. D.

| last13=Thompson |first13=I. |last14=Keiser |first14=S.

| last15=Jenkins |first15=J. S. |last16=Berdiñas |first16=Z.

| last17=Diaz |first17=M. |last18=Kiraga |first18=M.

| last19=Barnes |first19=J. R. |display-authors=1

| title=Chromospheric activity catalogue of 4454 cool stars. Questioning the active branch of stellar activity cycles

| journal=Astronomy and Astrophysics

| volume=616 | pages=A108 | year=2018

| bibcode=2018A&A...616A.108B | arxiv=1803.11123

| doi=10.1051/0004-6361/201629518 | s2cid=118915212 }}

}}

{{Starbox orbit

|reference=

|primary=ξ Sco A

|name=ξ Sco B

|period={{val|45.90|0.60}}

|periastron=B {{val|1997.22|0.02}}

|eccentricity={{val|0.744|0.001}}

|axis={{val|0.654|0.006}}

|inclination={{val|34.5|1.0}}

|node={{val|25.3|4.0}}

|periarg={{val|163.8|5.0}}

}}

{{Starbox orbit

|reference={{cite web|url=http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|title=Sixth Catalog of Orbits of Visual Binary Stars|publisher=United States Naval Observatory|access-date=2 July 2017|archive-date=1 August 2017|archive-url=https://web.archive.org/web/20170801102553/http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|url-status=dead}}

|primary=ξ Sco AB

|name=ξ Sco C

|period=1514.43

|periastron=B 2226.10

|eccentricity=0.041

|axis=7.755

|inclination=131.5

|node=47.4

|periarg=59.3

}}

{{Starbox detail

|component1 = A

| mass = 1.53{{Cite journal |last=Tokovinin |first=Andrei |date=2020-06-01 |title=Nearby Quintuple Systems κ Tucanae and ξ Scorpii |bibcode=2020AJ....159..265T |journal=The Astronomical Journal |volume=159 |issue=6 |pages=265 |doi=10.3847/1538-3881/ab8af1 |doi-access=free |arxiv=2005.04057 |issn=0004-6256}}

| temperature = 6,532

| component2 = B

| mass2 = 1.53

| temperature2 = 6,532

}}

{{Starbox detail|no_heading=y

| component1 = C

| mass = 1.00

| temperature = 5,705

}}

{{Starbox detail|no_heading=y

|component1=D

|mass=0.89

|temperature=5,529

|luminosity=0.71

|radius=0.94

|gravity=4.49

|age_gyr=2.3

|component2=E

|mass2=0.88

|temperature2=5,217

|luminosity2=0.44

|radius2=0.77

|gravity2=4.54{{cite journal | display-authors = 1 | last1 = Stassun | first1 = Keivan G. | last2 = Oelkers | first2 = Ryan J. | last3 = Paegert | first3 = Martin | last4 = Torres | first4 = Guillermo | last5 = Pepper | first5 = Joshua | last6 = Lee | first6 = Nathan De | last7 = Collins | first7 = Kevin | last8 = Latham | first8 = David W. | last9 = Muirhead | first9 = Philip S. | last10 = Chittidi | first10 = Jay | last11 = Rojas-Ayala | first11 = Bárbara | last12 = Fleming | first12 = Scott W. | last13 = Rose | first13 = Mark E. | last14 = Tenenbaum | first14 = Peter | last15 = Ting | first15 = Eric B. | last16 = Kane | first16 = Stephen R. | last17 = Barclay | first17 = Thomas | last18 = Bean | first18 = Jacob L. | last19 = Brassuer | first19 = C. E. | last20 = Charbonneau | first20 = David | last21 = Ge | first21 = Jian | last22 = Lissauer | first22 = Jack J. | last23 = Mann | first23 = Andrew W. | last24 = McLean | first24 = Brian | last25 = Mullally | first25 = Susan | last26 = Narita | first26 = Norio | last27 = Plavchan | first27 = Peter | last28 = Ricker | first28 = George R. | last29 = Sasselov | first29 = Dimitar | last30 = Seager | first30 = S. | last31 = Sharma | first31 = Sanjib | last32 = Shiao | first32 = Bernie | last33 = Sozzetti | first33 = Alessandro | last34 = Stello | first34 = Dennis | last35 = Vanderspek | first35 = Roland | last36 = Wallace | first36 = Geoff | last37 = Winn | first37 = Joshua N. | title = The Revised TESS Input Catalog and Candidate Target List | journal = The Astronomical Journal | date = 9 September 2019 | volume = 158 | issue = 4 | page = 138 | eissn = 1538-3881 | doi = 10.3847/1538-3881/ab3467 | bibcode = 2019AJ....158..138S | arxiv = 1905.10694 | doi-access = free}}

|age_gyr2=2.3{{cite journal |bibcode=2020ApJ...898...27S |title=BAFFLES: Bayesian Ages for Field Lower-mass Stars |last1=Stanford-Moore |first1=S. Adam |last2=Nielsen |first2=Eric L. |last3=De Rosa |first3=Robert J. |last4=MacIntosh |first4=Bruce |last5=Czekala |first5=Ian |journal=The Astrophysical Journal |date=2020 |volume=898 |issue=1 |page=27 |doi=10.3847/1538-4357/ab9a35 |arxiv=2006.04811 |doi-access=free }}

}}

{{Starbox catalog

|component1=Components ABC

|names1={{odlist|B=ξ Sco|ADS=9909|BD=−10°4237|GJ=9540|HIP=78727|SAO=159665 (only AB)}}

|component2=ξ Sco A

|names2={{odlist|HD=144070|HR=5978}}

|component3=ξ Sco B

|names3={{odlist|HD=144069|HR=5977}}

|component4=ξ Sco C

|names4={{odlist|SAO=159666}}

}}

{{Starbox catalog

|component1=Components DE

|names1={{odlist|ADS=9910|GJ=9541|}}

|component2=Component D

|names2={{odlist|BD=−11°4057|HD=144087|HIP=78738|SAO=159668}}

|component3=Component E

|names3={{odlist|BD=−11°4058|HD=144088|HIP=78739|SAO=159670}}

}}

{{Starbox reference

|Simbad=*+ksi+Sco|sn=ξ Sco ABC

|Simbad2=NAME+*+ksi+Sco+AB|sn2=ξ Sco AB

|Simbad3=*+ksi+Sco+A|sn3=ξ Sco A

|Simbad4=*+ksi+Sco+B|sn4=ξ Sco B

|Simbad5=*+ksi+Sco+C|sn5=ξ Sco C

|Simbad6=HD+144087|sn6=Component D

|Simbad7=HD+144088|sn7=Component E

|ARICNS=02736|an=ξ Sco A

|ARICNS2=02737|an2=ξ Sco B

|ARICNS3=02738|an3=ξ Sco C

|ARICNS4=02739|an4=ξ Sco D

|ARICNS5=02740|an5=ξ Sco E

}}

{{Starbox end}}

Xi Scorpii (ξ Sco) is part of a quintuple star system in the constellation Scorpius. It was assigned this designation by Bayer, although Ptolemy had catalogued the star in Libra. Flamsteed assigned it the designation 51 Librae, but this has fallen out of use since modern constellation boundaries assign the star to Scorpius.

Nomenclature

ξ Scorpii (Latinized to Xi Scorpii) is the star's Bayer designation. Xi Scorpii has no proper name, though it was erroneously known as Graffias before that name was applied to Beta Scorpii.{{cite book|author=Allen, R. H.|date=1899|url=https://archive.org/details/bub_gb_5xQuAAAAIAAJ|title=Star-names and Their Meanings|location=New York|publisher=G. E. Stechert|page=[https://archive.org/details/bub_gb_5xQuAAAAIAAJ/page/n393 371]}} Its Flamsteed designation is 51 Librae.{{cite journal|last=Wagman|first=M.|title=Flamsteed's Missing Stars|journal=Journal for the History of Astronomy|volume=18|number=3|page=209|date=August 1987|bibcode=1987JHA....18..209W|doi=10.1177/002182868701800305|s2cid=118445625}} When the modern constellation boundaries were drawn, Xi Scorpii was assigned to Scorpius, and the Flamsteed designation fell out of use.

The five stars of the Xi Scorpii system all have different designations, plus some designations that apply to more than one star. Xi Scorpii A, B, and C appear very close together in the sky and are typically grouped under a single multiple star designation, while components D and E are usually grouped under a separate multiple star designation designation. For example, Struve's catalogue of multiple stars includes the pair AB and C as Σ1998{{cite simbad|title=** STF 1998|access-date=14 October 2017}} and the pair D and E as Σ1999.{{cite simbad|title=** STF 1999AB|access-date=14 October 2017}}

class="wikitable"
ComponentBayerHRHDSAOHIPGJ
Arowspan="3" | ξ Scorpii5978144070rowspan="2" | 159665rowspan="3" | 78727rowspan="3" | 9540
B5977144069
Cnonenone159666
Dnonenone14408715966878738rowspan="2" | 9541
Enonenone14408815967078739

Properties

The Xi Scorpii system consists of five stars in two groups separated by about 4.7 arcminutes (or 0.08°) on the sky.{{cite journal|bibcode=1997A&AS..124...75T|doi=10.1051/aas:1997181|title=MSC - a catalogue of physical multiple stars|journal=Astronomy and Astrophysics Supplement Series|volume=124|pages=75–84|year=1997|last1=Tokovinin|first1=A. A.|doi-access=free}}

The brighter group contains Xi Scorpii A, B, and C. A and B are both yellow-white F-type stars. A is slightly brighter and warmer. They are separated by 0.744 arcseconds on average, and orbit around a common center once every 45.9 years. The dimmer, seventh-magnitude Xi Scorpii C orbits this pair at about ten times the distance, having a separation of around 7.6 arcseconds.

The second group contains components D and E, both K-type main-sequence stars, separated by about 11.9 arcseconds. They are known to be associated to each other and with the rest of the stars, because all stars share similar proper motions.

References

{{Reflist}}