Galaksi Triangulum: Perbedaan antara revisi
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{{Infobox galaxy
| name = Galaksi Triangulum
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| names = [[New General Catalogue|NGC]] 0598, MCG +05-04-069, 1ES 0131+303, RX J0133.8+3039, PGC 005818<ref name=ned/>
}}
'''Galaksi Triangulum''' (nama lain: '''Messier 33/NGC 598/PGC 5818/Galaksi Roda Peniti''') adalah [[galaksi#Spiral|galaksi spiral]] kira-kira 3 juta [[tahun cahaya]] dari bumi di rasi bintang [[Triangulum]]
Galaksi triangulum merupakan benda langit terbaik yang bisa dilihat dengan binokular yang besar maupun teleskop pada perbesaran yang kecil. Galaksi tersebut juga merupakan target benda langit terpopuler untuk [[Astrofotografi|astrofotografer]] karena lengan spiral dan [[Nebula]] H II yang lebih terang (khususnya [[NGC 604]])
Pada tahun 2004, ditemukan aliran hidrogen yang menghubungkan Galaksi Triangulum dengan [[Galaksi Andromeda]] dan dikonfirmasi pada tahun 2011.
== Pranala luar ==
* [http://www.seds.org/messier/m/m033.html Messier 33, SEDS Messier pages] {{Webarchive|url=https://web.archive.org/web/20061205054824/http://seds.org/messier/m/m033.html |date=2006-12-05 }}
* [http://www.spacetelescope.org/bin/images.pl?searchtype=freesearch&string=m33 M33 at ESA/Hubble] {{Webarchive|url=https://web.archive.org/web/20070930014801/http://www.spacetelescope.org/bin/images.pl?searchtype=freesearch&string=m33 |date=2007-09-30 }}
* [http://starrymirror.com/m331103.htm Triangulum Galaxy High In Northern Skies] {{Webarchive|url=https://web.archive.org/web/20071110000208/http://starrymirror.com/m331103.htm |date=2007-11-10 }}
* [http://www.darkatmospheres.com/astro/gallery/galaxies/enlarge.php?fileBase=galaxies_4 Dark Atmospheres Photography - M33 (dust lane enhancement)] {{Webarchive|url=https://web.archive.org/web/20171223215924/http://www.darkatmospheres.com/astro/gallery/galaxies/enlarge.php?fileBase=galaxies_4 |date=2017-12-23 }}
* [http://www.starpointing.com/dslr/m33.html Pointing to the Universe - M33] {{Webarchive|url=https://web.archive.org/web/20171119142808/http://www.starpointing.com/dslr/m33.html |date=2017-11-19 }}
* [http://www.messier-objects.com/messier-33-triangulum-galaxy/ Messier Object-Messier 33] {{Webarchive|url=https://web.archive.org/web/20230330004742/https://www.messier-objects.com/messier-33-triangulum-galaxy/ |date=2023-03-30 }}
== Referensi ==
{{Reflist|colwidth=25em|refs=
<ref name="SIMBAD-M33">{{cite web | title=M 33 -- Galaxy | work=SIMBAD | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=M33 | accessdate=2009-11-28 | archive-date=2014-09-13 | archive-url=https://web.archive.org/web/20140913102508/http://simbad.u-strasbg.fr/simbad/sim-id?Ident=M33 | dead-url=no }}</ref>
<ref name=ned>{{cite web | work=NASA/IPAC Extragalactic Database | title=Results for NGC 598 | publisher=NASA/IPAC/JPL | url=http://nedwww.ipac.caltech.edu/ | accessdate=2006-12-01 | archive-date=2000-10-19 | archive-url=https://web.archive.org/web/20001019032134/http://nedwww.ipac.caltech.edu/ | dead-url=no }}</ref>
<ref name=aass06>{{cite journal | author=Bonanos, A. Z. |coauthors=''et al''. | year=2006 | title=The First DIRECT Distance to a Detached Eclipsing Binary in M33 | doi=10.1007/s10509-006-9112-1 | journal=Astrophysics and Space Science | volume= 304 | issue=1-4| pages=207 |bibcode = 2006Ap&SS.304..207B }}</ref>
<ref name=apj696>{{cite journal | author=Magrini, Laura; Stanghellini, Letizia; Villaver, Eva | title=The Planetary Nebula Population of M33 and its Metallicity Gradient: A Look Into the Galaxy's Distant Past | journal=The Astrophysical Journal | volume=696 | issue=1 | pages=729–740 | month=May | year=2009 | doi=10.1088/0004-637X/696/1/729 | bibcode=2009ApJ...696..729M
}}</ref>
}}{{Galaksi Triangulum}}{{Obyek Messier}}
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[[Kategori:Objek Messier|033]]
[[Kategori:Objek NGC|Messier 033]]
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