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IC 2602
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{{Short description|Open cluster in the constellation Carina}} {{Infobox open cluster |name=IC 2602 |image=[[File:The Southern Pleiades (IC 2602).jpg|250px]] |caption= |epoch=[[J2000]] |constellation=[[Carina (constellation)|Carina]]|ra={{RA|10|42|57.5}}<ref name=ned>{{cite web|url=http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=IC+2602&extend=no&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|title=NED results for object IC 2602|access-date=23 January 2017|publisher=[[National Aeronautics and Space Administration]] / [[Infrared Processing and Analysis Center]] }}</ref> |dec={{DEC|-64|23|39}} |dist_pc=149 pc |dist_ly=486 ly<ref name="SIMBAD"/> |appmag_v=1.9<ref name="seds">{{cite web |title=IC 2602 - SEDS Messier Database |url=https://spider.seds.org/ngc/ngc.cgi?IC+2602 |access-date=23 January 2016}}</ref> |size_v=50{{prime}} × 50{{prime}} |mass_msol= |age=13.7 M.yr<sup>−1</sup> |notes= |names=Theta Carinae Cluster, [[Caldwell catalogue|Caldwell]] 102, [[Collinder catalogue|Cr]] 229, [[Philibert Jacques Melotte|Mel]] 102, VDBH 103<ref name=SIMBAD>{{cite simbad|title=IC 2602}}</ref> }} '''IC 2602''' (also known as the '''Southern Pleiades''', '''Theta Carinae Cluster''', or '''Caldwell 102''')<ref>{{Cite book |last=O'Meara |first=Stephen James |url=https://books.google.com/books?id=evkODQAAQBAJ&dq=deep+sky+companions+caldwell+objects+Southern+Pleiades%2C+Theta+Carinae+Cluster%2C+or+Caldwell+102%29&pg=PA467 |title=Deep-Sky Companions: The Caldwell Objects |date=2016-09-26 |publisher=Cambridge University Press |isbn=978-1-316-03353-1 |language=en}}</ref> is an [[open cluster]] in the [[constellation]] [[Carina (constellation)|Carina]]. Discovered by [[Abbe Lacaille]] in 1751 from [[South Africa]],<ref name=Jones_1969>{{cite journal | title=The search for the nebulae - VI | last=Jones | first=K. G. | journal=Journal of the British Astronomical Association | volume=79 | pages=213–222 | date=March 1969 | bibcode=1969JBAA...79..213J }}</ref> the cluster is easily visible to the [[Naked eye|unaided eye]], and is one of the nearest star clusters, centred about 149 parsecs (486 [[Light-year|light-years]]) away from [[Earth]]. ==Description== IC 2602 has a total [[apparent magnitude]] of 1.9,<ref name="seds"/> and contains about 75 stars. It is the third-brightest open cluster in the sky, following the [[Hyades (star cluster)|Hyades]] and the [[Pleiades]]. Its apparent diameter is about 50 [[arcminutes]]. IC 2602 is likely about the same age as the [[open cluster]] [[IC 2391]],<ref name="Staffer19972">{{cite journal |author=Stauffer, J.R. |last2=Hartmann |first2=Lee W. |last3=Prosser |first3=Charles F. |last4=Randich |first4=Sofia |last5=Balachandran |first5=Suchitra |last6=Patten |first6=Brian M. |last7=Simon |first7=Theodore |last8=Giampapa |first8=Mark |display-authors=1 |date=1997 |title=Rotational Velocities and Chromospheric/Coronal Activity of Low-Mass Stars in the Young Open Clusters IC 2391 and IC 2602 |journal=Astrophysical Journal |volume=479 |issue=2 |pages=776 |bibcode=1997ApJ...479..776S |doi=10.1086/303930 |doi-access=free}},</ref> which has a [[lithium depletion boundary]] age of 50 million years old,<ref name="Barrado20022">{{cite journal |last1=Barrado y Navascues |first1=D |last2=Stauffer |first2=J.R. |last3=Jayawardhana |first3=R. |date=2002 |title=Spectroscopy of Very Low Mass Stars and Brown Dwarfs in IC 2391: Lithium Depletion and Hα Emission |journal=Astrophysical Journal |volume=614 |issue=1 |pages=386–397 |arxiv=astro-ph/0406436 |bibcode=2004ApJ...614..386B |doi=10.1086/423485|s2cid=208867491 }}</ref> though the age estimated from its [[Hertzsprung-Russell diagram]] is about 13.7 million years.<ref name="webda20172">{{cite web |title=WEBDA page for open cluster IC 2602 |url=http://cbat.eps.harvard.edu/CBAT_M31.html |access-date=2017-04-11 |publisher=WEBDA}}</ref> IC 2602 is thought to form part of the Lower [[Scorpius–Centaurus association]].<ref name="Whiteoak19612">{{cite journal |last1=Whiteoak |first1=J.B. |date=1961 |title=A study of the galactic cluster IC 2602. I. A photoelectric and spectroscopic investigation |journal=Monthly Notices of the Royal Astronomical Society |volume=123 |pages=245–256 |bibcode=1961MNRAS.123..245W |doi=10.1093/mnras/123.3.245 |doi-access=free}}</ref><ref name="Blaauw19642">{{cite journal |last1=Blaauw |first1=A. |date=1964 |title=The O Associations in the Solar Neighborhood |journal=Annual Review of Astronomy and Astrophysics |volume=2 |pages=213–246 |bibcode=1964ARA&A...2..213B |doi=10.1146/annurev.aa.02.090164.001241}}</ref> == Components == [[Θ Carinae|Theta Carinae]] is the brightest [[star]] within the open cluster, with the [[Apparent magnitude|apparent]] [[visual magnitude]] of +2.74.<ref>{{Cite web |title=Theta Carinae |url=https://simbad.u-strasbg.fr/simbad/sim-id |access-date=2022-12-12 |website=simbad.u-strasbg.fr}}</ref> Theta Carinae is part of the [[Asterism (astronomy)|asterism]] known as the [[Diamond Cross]], which is often mistaken for the Southern Cross asterism in the constellation of [[Crux]]. [[PP Carinae|p Carinae]] (PP Carinae) is another third-magnitude star known to be a member of IC 2602, although it lies well outside the main visible grouping of stars. p Carinae exhibits a variable apparent magnitude ranging from 3.22 to 3.55. All other members the cluster are of the fifth magnitude and fainter, but several are naked-eye objects, including [[HR 4196]] (V518 Car), HR 4204, [[HD 93194]], HR 4219, HR 4220, [[HR 4222]], HD 92536, HD 93738, and V364 Carinae. An [[exoplanet]] has been found orbiting the star TOI-837 in this cluster.<ref name="Bouma2020"/> {| class="wikitable sortable" |+IC 2602 brightest stars !Designation ![[Apparent magnitude]]<ref name=":0">{{Cite web |title=Gaia Archive |url=https://gea.esac.esa.int/archive/ |access-date=2022-12-24 |website=gea.esac.esa.int}}</ref> ![[Stellar classification]]<ref>{{Cite web |title=Theta Carinae |url=https://simbad.u-strasbg.fr/simbad/sim-id |access-date=2022-12-24 |website=simbad.u-strasbg.fr}}</ref> !Distance (pc) |- |[[Theta Carinae]] |2.735 |style="background:#{{Color temperature|20000|hexval}};"|B0Vp |142<ref>{{Cite journal |last=Whitman |first=Alan |date=June 1998 |title=At The Eyepiece: Eclipse-Chasing Perfection - The Caribbean |journal=Journal of the Royal Astronomical Society of Canada |volume=92 |page=158 |bibcode=1998JRASC..92..158W}}</ref> |- |[[PP Carinae|p Carinae]] (PP Carinae) |3.247 |style="background:#{{Color temperature|20000|hexval}};"|B4Vne |104.645<ref name=":0" /> |- |HR 4204 |5.719 |style="background:#{{Color temperature|20000|hexval}};"|B3IV/V |309.598<ref>{{Cite web |title=Catalogues - Hipparcos - Cosmos |url=https://www.cosmos.esa.int/web/hipparcos/catalogues |access-date=2022-12-24 |website=www.cosmos.esa.int}}</ref><ref>Equated from parallax in [[Milliarc-second|milliarcseconds]] (mas).</ref> |- |HR 4219 |5.297 |style="background:#{{Color temperature|20000|hexval}};"|B6Vnn |156.674<ref name=":0" /> |- |HR 4222 |4.807 |style="background:#{{Color temperature|20000|hexval}};"|B4V |154.007<ref name=":0" /> |- |HD 92536 |6.313 |style="background:#{{Color temperature|20000|hexval}};"|B8V |156.823<ref name=":0" /> |- |[[HD 93194]] |4.777 |style="background:#{{Color temperature|20000|hexval}};"|B3/5Vn |169.146<ref name=":0" /> |- |HD 93738 |8.571 |style="background:#{{Color temperature|20000|hexval}};"|B9.5V |417.168<ref name=":0" /> |- |V364 Carinae |5.465 |style="background:#{{Color temperature|8750|hexval}};"|ApSi |160.013<ref name=":0" /> |- |[[V518 Carinae]] |4.758 |style="background:#{{Color temperature|20000|hexval}};"|B3V |140.634<ref name=":0" /> |} == History == IC 2602 was first discovered by French [[astronomer]] and [[abbot]] [[Nicolas-Louis de Lacaille]] on March 3, 1751 while in [[Cape of Good Hope]], [[South Africa]].<ref>{{Cite journal |last=Jones |first=K. G. |date=March 1969 |title=The Search for the Nebulae - VI |journal=Journal of the British Astronomical Association |volume=79 |page=213 - 222 |bibcode=1969JBAA...79..213J}}</ref> In Lacaille's initial discovery, he classified Theta Carinae (referred as "Theta Navis", or alternatively "Theta Argus"{{Citation needed|date=December 2022}}) as a [[Magnitude (astronomy)|third magnitude]] star, whilst citing the cluster's resemblance to the northern Pleiades. == Observation == Positioned at a [[declination]] of -64º on the night sky,<ref name="ned2">{{cite web |title=NED results for object IC 2602 |url=http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=IC+2602&extend=no&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES |access-date=23 January 2017 |publisher=[[National Aeronautics and Space Administration]] / [[Infrared Processing and Analysis Center]]}}</ref> IC 2602 is most clearly visible from the [[Southern Hemisphere|southern hemisphere]], and appears [[Circumpolar star|circumpolar]] from southern [[subtropics]] and [[Temperate climate|temperate climates]]; the cluster is observable from a limited selection of [[Northern Hemisphere|north hemispherical]] regions, mainly [[Tropical rainforest|tropical]] areas.{{efn|IC 2602 is located at a declination of {{val|-64|ul=°}}, which equates to an angular distance of 26º from the [[Celestial pole|south celestial pole]].}} IC 2602 is identifiable a few degrees south of the southern [[Milky Way]], surrounded by various [[Fifth magnitude star|fifth]] and [[Sixth magnitude star|sixth magnitude]] stars. To the unaided eye, several faint stars are distinguishable to the east of the blue Theta Carinae. ==Notes== {{notelist}} ==References== {{reflist|refs= <ref name="Bouma2020">{{cite journal |last1=Bouma |first1=L. G. |last2=Hartman |first2=J. D. |display-authors=etal |date=November 2020 |title=Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602 |journal=[[The Astronomical Journal]] |volume=160 |issue=5 |pages=239 |doi=10.3847/1538-3881/abb9ab |arxiv=2009.07845 |bibcode=2020AJ....160..239B |doi-access=free }}</ref> }} == External links == {{commonscat}} * [http://messier.seds.org/xtra/ngc/i2602.html The Southern Pleaides @ SEDS IC objects pages] * [http://www.starrynightphotos.com/southern_sky/southern_pleiades_ic_2602.htm Image Southern Pleiades(IC 2602)] {{Caldwell catalogue}} {{Carina (constellation)}} {{sky|10|42|56|-|64|23|42|479}} {{DEFAULTSORT:IC 2602}} [[Category:IC 2602| ]] [[Category:Carina (constellation)]] [[Category:Open clusters]] [[Category:Caldwell objects|102b]] [[Category:Astronomical objects discovered in 1751|?]]
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