Loading...

This page describes an image Sombrero galaxy

Download File ( image 4.93 MB)

Image caption: This prominent galaxy M 104 is often called the Sombrero galaxy due to its resemblance to the Mexican hat. This look is created by the thin disk oriented nearly edge-on, which appears illuminated by the dominant bulge. Both, the disk and bulge contain stars, but the stars in the bulge tend to be older, while the disk also harbors large amounts of dust and gas creating shadows. M 104 is located in the constellation Virgo approximately 50 light-years away. While some of the dots visible in the picture are foreground stars and others background galaxies, the majority are actually globular clusters, dense massive clusters of stars, associated with the Sombrero Galaxy.
Scroll to captions in other languages


Image credit: ESO/P. Barthel Credit Link
Related glossary terms: Disk Galaxy , Galaxy
Categories: Galaxies

Image license: Creative Commons Attribution 4.0 International (CC BY 4.0) Creative Commons Attribution 4.0 International (CC BY 4.0) icons

The media file captions presented on the OAE website were written, translated and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits for our translation project here. All media file captions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE". The media files themselves may have different licenses (see above) and should be credited as listed above under "credit".

Captions in Different Languages:

Arabic
Image caption: غالبًا ما تسمى هذه المجرة البارزة M 104 بمجرة Sombrero نظرًا لتشابهها مع القبعة المكسيكية. تبد المجرة بهذا الشكل من خلال قرص رفيع يرى بإتجاه الحافة وعلى امتداد خط النظرتقريبًا ، والذي يظهر مضاءً بالانتفاخ السائد. يحتوي كل من القرص والانتفاخ على نجوم ، لكن النجوم الموجودة في الانتفاخ تميل إلى أن تكون أقدم ، بينما يحتوي القرص أيضًا على كميات كبيرة من الغبار والغاز مما يخلق الظلال.
تقع M 104 في كوكبة العذراء على بعد حوالي 50 سنة ضوئية. في حين أن بعض النقاط المرئية في الصورة هي نجوم في المقدمة ومجرات أخرى في الخلفية ، فإن الغالبية هي في الواقع مجموعات كروية ، وهي مجموعات كثيفة ضخمة من النجوم ، مرتبطة بمجرة سومبريرو.
Image credit: ESO / ب. بارثيل
Related glossary terms: Disk Galaxy , المجرة
Caption translation status: Approved by a reviewer
Caption translators: Somaya Saad
Caption reviewers: Ahmed Abulwfa

Italian
Image caption: M104, un galassia molto appariscente, è spesso chiamata galassia Sombrero per la sua somiglianza con il cappello messicano. Questo aspetto è creato dal sottile disco orientato quasi di taglio, che appare illuminato dal rigonfiamento centrale, dominante. Sia il disco che il rigonfiamento contengono stelle, ma le stelle nel rigonfiamento tendono a essere più vecchie, mentre il disco ospita anche grandi quantità di polvere e gas che creano ombre. M104 si trova nella costellazione della Vergine, a circa 50 anni luce di distanza dalla Terra. Anche se alcuni dei punti visibili nell'immagine sono stelle in primo piano e altri galassie di sfondo, la maggior parte sono in realtà ammassi globulari, cioè enormi e densi ammassi di stelle, associati alla Galassia Sombrero.
Image credit: ESO/P. Barthel
Related glossary terms: Galassia , Galassia a disco
Caption translation status: Approved by a reviewer
Caption translators: Giuliana Giobbi
Caption reviewers: Rosa Valiante, Rodolfo Canestrari, Anna Wolter

Simplified Chinese
Image caption: 由于这个著名的星系M104 与墨西哥帽子非常相似,因此经常被称为 "草帽星系"。它之所以看起来是这个样子,是由于我们观测的视角几乎平行于薄盘的平面,薄盘/星系盘 被星系的核球所照亮。星系盘和核球都含有恒星,但核球中的恒星往往比较老。星系盘中蕴含有大量的尘埃和气体,从而形成了阴影。M104 位于室女座,距离我们大约 50 光年。图中可见的小点有些是前景恒星,有些是背景星系,但实际上大部分都是球状星团,它们是与草帽星系相关的致密大质量恒星团。
Image credit: ESO/P.巴特尔
Related glossary terms: 盘状星系 , 银河系
Caption translation status: Approved by a reviewer
Caption translators: Lin Shijie
Caption reviewers: Jing Liang, Wang Yilin

Traditional Chinese
Image caption: 由於這個著名的星系M104 與墨西哥帽子非常相似,因此經常被稱為 "草帽星系"。之所以,看起來是這個樣子,是由於我們觀測的視角幾乎平行著薄圓盤的平面,圓盤被星系中的隆起(bulge)所照亮。星系盤和隆起都含有恆星,但隆起中的恆星往往比較老。星系盤中藏有大量的塵埃和氣體,從而形成了陰影。M104 位於室女座,距離我們大約 50 光年。圖中可見的小點有些是前景恆星,有些是背景星系,但實際上大部分都是球狀星團,它們是與草帽星系相關的緻密大質量恆星團。
Image credit: ESO/P.巴特爾
Related glossary terms: 盤狀星系 , 銀河系
Caption translation status: Approved by a reviewer
Caption translators: An automated transliteration from the simplified Chinese translation by - Lin Shijie