Beta Ophiuchi

{{Short description|Orange giant star in the constellation Ophiuchus}}

{{Starbox begin}}

{{Starbox image

| image =

{{Location mark

| image=Ophiuchus IAU.svg

| float=center | width=250 | position=right

| mark=Red circle.svg | mark_width=10 | mark_link=ι Exa

| x%=41.8 | y%=25.8

}}

| caption=Location of β Ophiuchi (circled)

}}

{{Starbox observe

| epoch = J2000.0 (ICRS)

| ra = {{RA|17|43|28.35191}}

| dec = {{DEC|+04|34|02.2932}}

| appmag_v = 2.749 (2.75 to 2.77){{Citation needed |date=June 2024}}

| constell = Ophiuchus

}}

{{Starbox character

| class = K2 III

| b-v = +1.170

| u-b = +1.253

}}

{{Starbox astrometry

| radial_v = –12.53

| prop_mo_ra = {{val|-41.793}}

| prop_mo_dec = {{val|150.43}}

| pm_footnote =

| parallax = 39.2284

| p_error = 0.2027

| parallax_footnote =

| absmag_v = {{nowrap|+0.77 ± 0.04}}

}}

{{Starbox detail

| source =

| mass = {{val|1.44|0.16}}{{snd}}{{val|1.75|0.174}}

| radius = {{val|12.17|0.06}}

| luminosity = {{val|57.7|2.9}}

| temperature = {{val|4559|67|fmt=commas}}

| gravity = {{val|2.33|0.07}}

| metal_fe = {{val|0.06|0.04}}

| rotational_velocity = 5.4

| age_gyr = {{val|2.75|0.78}}

}}

{{Starbox catalog

| names = {{odlist | name=Cebalrai | name2=Celbalrai | name3=Cheleb | name4=Kelb Alrai | B=Bet Oph, β Oph, β Ophiuchi | F=60 Oph, 60 Ophiuchi | BD=+04°3489 | FK5=665 | HD=161096 | HIP=86742 | HR=6603 | SAO=122671 }}

}}

{{Starbox reference

|Simbad=bet+Oph

}}

{{Starbox end}}

Beta Ophiuchi or β Ophiuchi, also named Cebalrai {{IPAc-en|,|s|E|b|@l|'|r|ei|.|iː}},{{cite journal

|title=The pronunciations, derivations, and meanings of a selected list of star names

|last=Davis |first=George A.

|journal=Popular Astronomy

|volume=52

|number=

|date=1944

|pages = 8–30

|bibcode=1944PA.....52....8D |url=http://adsbit.harvard.edu/full/1944PA.....52....8D

}}{{cite web | url=http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt | title=IAU Catalog of Star Names |accessdate=28 July 2016}} is a star in the equatorial constellation of Ophiuchus. The apparent visual magnitude of this star is 2.7, which is readily visible to the naked eye even from urban skies. The distance to this star can be estimated using parallax measurements, yielding a value of {{Convert|83.4|ly|pc|abbr=off|lk=on}} from the Sun.

Nomenclature

β Ophiuchi (Latinised to Beta Ophiuchi) is the star's Bayer designation.

It bore the traditional names Cebalrai, Celbalrai, Cheleb and Kelb Alrai (or sometimes just Alrai), all derived from the Arabic كلب الراعي kalb al-rā‘ī "the shepherd's dog".{{citation|

url=https://digital.bodleian.ox.ac.uk/inquire/Discover/Search/#/?p=c+0,t+,rsrs+0,rsps+10,fa+,so+ox%3Asort%5Easc,scids+,pid+c1caa84c-f6d2-483f-9eb4-2439cccdc801,vi+62392615-fb52-4c0c-bf97-ed5153a1d509|

title=Book Of Fixed Stars, Al-Sufi, Bodleian Ms.

}} In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN){{citation

| url=https://www.iau.org/science/scientific_bodies/working_groups/280/

| title=IAU Working Group on Star Names (WGSN)

| publisher=International Astronomical Union

| accessdate=22 May 2016 | postscript=. }} to catalogue and standardize proper names for stars. The WGSN approved the name Cebalrai for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.

=Namesake=

Properties

This is a giant star with a stellar classification of K2 III. Although it is only 2.75 billion years old, 60% of the solar age, it has reached a stage in its evolution where the atmosphere has expanded to about 12 times the Sun's radius and is radiating 58 times the luminosity of the Sun. Its outer envelope is relatively cool with an effective temperature of 4,559 K, giving it the orange hue typical of K-type stars. Like some other K-type giants, β Ophiuchi has been found to vary very slightly (0.02 magnitudes) in brightness.,

Cebalrai is a member of the thin disk population. It is following a low eccentricity orbit through the Milky Way galaxy that carries it between a distance of {{Convert|27.3|–|30.9|kly|kpc|abbr=on|lk=on}} from the Galactic Center and up to {{Convert|0.62|kly|kpc|abbr=on}} above or below the galactic plane.

Radial velocity variations with a period of 142 days are likely explained by periodic radial pulsations caused by intrinsic stellar variability.

References

{{Reflist|30em|refs=

{{citation

| title=Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer

| last1=Baines | first1=Ellyn K. | last2=Armstrong | first2=J. Thomas | last3=Schmitt | first3=Henrique R. | last4=Zavala | first4=R. T. | last5=Benson | first5=James A. | last6=Hutter | first6=Donald J. | last7=Tycner | first7=Christopher | last8=Belle | first8=Gerard T. van

| display-authors=1 | journal=The Astronomical Journal

| volume=155 | at=30 | year=2018 | issue=1 | postscript=.

| arxiv=1712.08109 | bibcode=2018AJ....155...30B

| doi=10.3847/1538-3881/aa9d8b | s2cid=119427037 | doi-access=free }}

{{Cite DR3|4473334474604992384}}

{{citation | first1=Peter D. | last1=Edmonds | first2=Roland L. | last2=Gilliland | title=K Giants in 47 Tucanae: Detection of a New Class of Variable Stars | journal=Astrophysical Journal Letters | volume=464 |date=June 1996 | issue=2 | pages=L157–L160 | bibcode=1996ApJ...464L.157E |doi = 10.1086/310108 | doi-access=free }}

{{citation | display-authors=1 | last1=Soubiran | first1=C. | last2=Bienaymé | first2=O. | last3=Mishenina | first3=T. V. | last4=Kovtyukh | first4=V. V. | title=Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants | journal=Astronomy and Astrophysics | year=2008 | volume=480 | issue=1 | pages=91–101 | bibcode=2008A&A...480...91S | doi=10.1051/0004-6361:20078788 |arxiv = 0712.1370 | s2cid=16602121 }}

{{citation | first1=Artie P. | last1=Hatzes | first2=William D. | last2=Cochran | title=The Radial Velocity Variability of the K Giant beta Ophiuchi. II. Long-Period Variations | journal=Astrophysical Journal | volume=468 |date=September 1996 | pages=391–397 | bibcode=1996ApJ...468..391H |doi = 10.1086/177699 | doi-access=free }}

{{citation | display-authors=1 | last1=Famaey | first1=B. | last2=Jorissen | first2=A. | last3=Luri | first3=X. | last4=Mayor | first4=M. | last5=Udry | first5=S. | last6=Dejonghe | first6=H. | last7=Turon | first7=C. | title=Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters | journal=Astronomy and Astrophysics | volume=430 | issue=1 | pages=165–186 |date=January 2005 | doi=10.1051/0004-6361:20041272 | bibcode=2005A&A...430..165F |arxiv = astro-ph/0409579 | s2cid=17804304 }}

{{citation | display-authors=1 | last1=Massarotti | first1=Alessandro | last2=Latham | first2=David W. | last3=Stefanik | first3=Robert P. | last4=Fogel | first4=Jeffrey | title=Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity | journal=The Astronomical Journal | volume=135 | issue=1 | pages=209–231 |date=January 2008 | doi=10.1088/0004-6256/135/1/209 | bibcode=2008AJ....135..209M | s2cid=121883397 | doi-access=free }}

{{Cite journal |last1=Soubiran |first1=C. |last2=Creevey |first2=O. L. |last3=Lagarde |first3=N. |last4=Brouillet |first4=N. |last5=Jofré |first5=P. |last6=Casamiquela |first6=L. |last7=Heiter |first7=U. |last8=Aguilera-Gómez |first8=C. |last9=Vitali |first9=S. |last10=Worley |first10=C. |last11=de Brito Silva |first11=D. |date=2024-02-01 |title=Gaia FGK benchmark stars: Fundamental Teff and log g of the third version |url=https://ui.adsabs.harvard.edu/abs/2024A&A...682A.145S |journal=Astronomy and Astrophysics |volume=682 |pages=A145 |doi=10.1051/0004-6361/202347136 |bibcode=2024A&A...682A.145S |issn=0004-6361}} [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A%2BA/682/A145&recno=164 Cebalrai's database entry] at VizieR.

{{citation | last1=Oja | first1=T. | title=UBV photometry of stars whose positions are accurately known. III | journal=Astronomy and Astrophysics Supplement Series | year=1986 | volume=65 | issue=2 | pages=405–4 | bibcode=1986A&AS...65..405O }}

{{citation |title=The Colour of Stars |date=December 21, 2004 |work=Australia Telescope, Outreach and Education |publisher=Commonwealth Scientific and Industrial Research Organisation |url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |accessdate=2012-01-16 |url-status=dead |archiveurl=https://web.archive.org/web/20120318151427/http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |archivedate=2012-03-18 }}

{{citation | title=rho Per -- Semi-regular pulsating Star | work=SIMBAD | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Beta+Ophiuchi | accessdate=2012-01-29 }}

{{citation | first1=Richard Hinckley | last1=Allen | title=Star-names and their meanings | publisher=G. E. Stechert | year=1899 | page=301 | url=https://books.google.com/books?id=5xQuAAAAIAAJ&pg=PA301 }}

{{citation | display-authors=1 | last1=Carney | first1=Bruce W. | last2=Gray | first2=David F. | last3=Yong | first3=David | last4=Latham | first4=David W. | last5=Manset | first5=Nadine | last6=Zelman | first6=Rachel | last7=Laird | first7=John B. | title=Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars | journal=The Astronomical Journal | volume=135 | issue=3 | pages=892–906 |date=March 2008 | doi=10.1088/0004-6256/135/3/892 | bibcode=2008AJ....135..892C |arxiv = 0711.4984 | s2cid=2756572 }}

}}

{{Stars of Ophiuchus}}

{{DEFAULTSORT:Beta Ophiuchi}}

Category:K-type giants

Category:Ophiuchus

Ophiuchi, Beta

Category:Durchmusterung objects

Ophiuchi, 60

161096

086742

6603

Cebalrai