Atlas (star)

{{Short description|Triple star system in the constellation Taurus}}

{{Starbox begin|name=Atlas}}

{{Starbox image

| image =

{{Location mark

| image = Pleiades large.jpg | width = 280

| alt = Image of the Pleiades star cluster | float = center

| mark = Red circle.svg | mark_width = 30

| x = 115 | y = 430

}}

| caption = Atlas in the Pleiades cluster (circled)

}}

{{Starbox observe

|epoch=J2000

|constell=Taurus

|ra={{RA|03|49|09.74258}}

|dec={{DEC|+24|03|12.3003}}

|appmag_v=3.63{{cite journal|bibcode=2002yCat.2237....0D|title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system|journal=CDS/ADC Collection of Electronic Catalogues|volume=2237|author1=Ducati, J. R.|year=2002}} (3.84 / 5.46){{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=21 June 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}}

}}

{{Starbox character

|class=B8III{{cite journal|bibcode=2015ApJ...804..146D|doi=10.1088/0004-637X/804/2/146|arxiv=1501.03154|title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets|journal=The Astrophysical Journal|volume=804|issue=2|pages=146|year=2015|last1=David|first1=Trevor J.|last2=Hillenbrand|first2=Lynne A.|s2cid=33401607}}

|b-v=−0.08{{cite journal|author1=Mermilliod, J.-C.|title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)|journal=Catalogue of Eggen's UBV Data|date=1986|bibcode= 1986EgUBV........0M}}

|u-b=−0.36

|variable=SPB{{cite web |title=NSV 1345 |url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=39969 |website=The International Variable Star Index |publisher=AAVSO |access-date=8 October 2022}}

}}

{{Starbox astrometry

|radial_v={{val|8.5|2}}{{cite journal|title=General catalogue of stellar radial velocities|journal=Washington|author=Wilson, Ralph Elmer|date=1953|bibcode=1953GCRV..C......0W}}

|prop_mo_ra=+19.079

|prop_mo_dec=−46.193

|pm_footnote=

|parallax=8.1184

|p_error=0.4791

|parallax_footnote={{cite Gaia EDR3|66526127137440128}}

|dist_ly={{cvt|132|±|4|pc|ly|disp=number}}

|dist_pc={{val|132|4}}

|absmag_v=−1.82{{cite journal

| title=XHIP: An extended hipparcos compilation

| last1=Anderson | first1=E. | last2=Francis | first2=Ch.

| journal=Astronomy Letters

| volume=38 | issue=5 | pages=331 | year=2012

| bibcode=2012AstL...38..331A | arxiv=1108.4971

| doi=10.1134/S1063773712050015 | s2cid=119257644 }}

}}

{{Starbox orbit

|reference={{cite journal|bibcode=2004A&A...425L..45Z|doi=10.1051/0004-6361:200400062|arxiv=astro-ph/0408430|title=A purely geometric distance to the binary star Atlas, a member of the Pleiades|journal=Astronomy & Astrophysics|volume=425|issue=3|pages=L45|year=2004|last1=Zwahlen|first1=N.|last2=North|first2=P.|last3=Debernardi|first3=Y.|last4=Eyer|first4=L.|last5=Galland|first5=F.|last6=Groenewegen|first6=M. A. T.|last7=Hummel|first7=C. A.|s2cid=37047575}}

|primary=Aa1

|name=Aa2

|period_unitless={{val|290.984|0.079|ul=d}}

|axis_unitless={{val|13.08|0.12|ul=mas}}

|inclination={{val|107.87|0.49}}

|node={{val|154.0|0.7}}

|periastron=JD {{val|2450583.0|1.9}}

|eccentricity={{val|0.2385|0.0063}}

|periarg={{val|151.9|2.2}}

|k1={{val|26.55|1.41}}

|k2={{val|36.89|0.22}}

}}

{{Starbox detail

|component1=Aa1

|mass={{val|4.74|0.25}}

|radius={{val|7.9|0.8}}

|temperature={{val|13500|300|fmt=commas}}{{cite journal |doi=10.3847/1538-4357/ab04b2 |title=Angular Sizes, Radii, and Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array |year=2019 |last1=Gordon |first1=Kathryn D. |last2=Gies |first2=Douglas R. |last3=Schaefer |first3=Gail H. |last4=Huber |first4=Daniel |last5=Ireland |first5=Michael |journal=The Astrophysical Journal |volume=873 |issue=1 |page=91 |bibcode=2019ApJ...873...91G |s2cid=125181833 |doi-access=free }}

|rotational_velocity=182

|luminosity=

|gravity={{val|3.32|0.09}}

|metal_fe=

|age_gyr=

|component2=Aa2

|mass2={{val|3.42|0.25}}

|radius2={{val|3.2|0.3}}

|temperature2=13,660

|gravity2={{val|3.96|0.09}}

}}

{{Starbox detail|no_heading=y

|component1 = Ab

|mass=2.09

}}

{{Starbox catalog

|names={{odlist|F=27 Tau|BD=+23°557|FK5=142|HD=23850|HIP=17847|HR=1178|SAO=76228}}

}}

{{Starbox reference

|Simbad=27+Tau

}}

{{Starbox end}}

Atlas {{IPAc-en|'|æ|t|l|@|s}},{{cite book

|last1=Kunitzsch |first1=Paul

|last2=Smart |first2=Tim

|date = 2006 |edition = 2nd rev.

|title = A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations

|publisher = Sky Pub |location = Cambridge, Massachusetts

|isbn = 978-1-931559-44-7

}} designation 27 Tauri, is a triple star system in the constellation of Taurus. It is a member of the Pleiades, an open star cluster (M45). It is 431 light-years (132 parsecs) away, and is 3.92 degrees north of the ecliptic.

Nomenclature

27 Tauri is the star's Flamsteed designation.

In 2016 the International Astronomical Union organized a Working Group on Star Names (WGSN){{cite web

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

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

| publisher=International Astronomical Union

| access-date=22 May 2016 }} to catalogue and standardize proper names for stars. The WGSN approved the name Atlas for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.{{cite web | url=http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt | title=IAU Catalog of Star Names |access-date=28 July 2016}}

Mythology

{{main|Atlas (mythology)}}

Atlas was a Titan and the father of the Pleiades sisters in Greek mythology.

Properties

Atlas is a triple star system, with the inner pair orbiting in under a year and the outer star orbiting in 260 years. The outer star, component Ab (sometimes component B, such as in CCDM and SIMBAD{{Cite web |title=27 Tau B |url=http://simbad.cds.unistra.fr/simbad/sim-basic |access-date=2023-10-01 |website=simbad.cds.unistra.fr}}), has been resolved at a distance of {{val|0.784|ul="}} from the unresolved spectroscopic binary. It is too close to have been assigned a spectral class, but has an apparent magnitude of 6.8, three magnitudes fainter than the combined magnitude of the closer pair. Its mass is estimate to be twice that of the Sun. In the WDS catalog, there are 8 other stars, ranging from B-I, which have been classed as companions of Atlas.{{Cite journal |last=Tokovinin |first=Andrei |date=2018-03-01 |title=The Updated Multiple Star Catalog |journal=The Astrophysical Journal Supplement Series |volume=235 |issue=1 |pages=6 |arxiv=1712.04750 |bibcode=2018ApJS..235....6T |doi=10.3847/1538-4365/aaa1a5 |issn=0067-0049 |s2cid=119047709 |doi-access=free }}

File:AtlasLightCurve.png for Atlas, adapted from White et al. (2017){{cite journal |last1=White |first1=T. R. |display-authors=etal |title=Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades |journal=Monthly Notices of the Royal Astronomical Society |date=November 2017 |volume=471 |issue=3 |pages=2882–2901 |doi=10.1093/mnras/stx1050 |arxiv=1708.07462 |bibcode=2017MNRAS.471.2882W |doi-access=free }}]]

The inner pair have a well-defined orbit with a period of 291 days, a semi-major axis of {{val|13|ul=mas}}, and an eccentricity of 0.24. At an inclination of 108°, it is not thought to show eclipses. Although the two stars cannot be resolved, the primary, component Aa1, is calculated to be 1.6 magnitudes brighter than the secondary, component Aa2.

Low amplitude variability of the brightness of Atlas was tentatively detected in observations by STEREO and clearly detected by Kepler/K2. The light curve varies with several periods, the most prominent being 2.427, 0.7457 and 1.214 days.

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References

{{Reflist}}