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291:يُحتملُ ظهور لولبيَّة صغيرة ضمن الأذرع اللولبيَّة لمجرَّة UGC 1810 في أعلى اليمين. يُلاحظُ كيف أنَّ الذراع اللولبي الأكثر تطرُّفًا يُغيَّر هيئته أثناء عُبوره في المجرَّة الثالثة، فيتحوَّل من المصقول السويّ ذي النجوم العتيقة (مُحمرَّة اللون) على إحدى الجهات إلى المُلتف ذي النجوم قاتمة الزُرقة على الطرف الآخر. يُمكنُ التكهّن بالمُباعدة الطبيعيَّة بين العُقد المُكوِّنة للنجوم الزرقاء بناءً على عدم استقرار كميَّة الغاز المحفوظة ضمن الذراع، كما يظهر أنَّها تتطابق مع ما يظهر في الأذرع اللولبيَّة الخاصَّة بمجرَّاتٍ أُخرى.
288:تُظهرُ سلسلة من الأنماط الحلزونيَّة في المجرَّة الكُبرى دليلًا على حصول تفاعل. يبدو الذراع الأكبر الخارجي بشكلٍ حلقيّ جُزئيًّا، وهي ظاهرة تبدو للناظر عندما تتداخل المجرَّات المُتفاعلة مع بعضها البعض. هذا يُفيدُ باحتماليَّة غوص المجرَّة القرينة الأصغر عميقًا، خارج المركز، وعبر مجرَّة UGC 1810. المجمعة الداخليَّة من الأذرع اللولبيَّة مُشوَّهة ومُنعطفة خارج السطح المجرّي حيثُ يظهر أحد الأذرع خارج الكُتلة المركزيَّة ثُمَّ يعود ليلتف من الجهة الأُخرى. ولا يزال العُلماء يتسائلون عن كيفيَّة اتصال هذين النمطين اللولبيين.
294:المجرَّةُ الأكبر الواقعة ضمن زوج UGC 1810 - UGC 1813 تتمتَّعُ بكُتلةٍ تفوقُ كُتلة المجرَّات الأصغر بحوالي خمس مرَّات. في الأزواج اللامُتساوية مثل هذه، يُنتجُ العبور السريع لمجرَّةٍ قرينة البُنية المُتباينة أو اللامُتماثلة في اللولبيَّة الرئيسيَّة. أيضًا في مثل هكذا أحداث، يبدأُ الانفجار النجمي نمطيًّا في المجرَّات الصُغرى قبل تلك الكُبرى. يُمكنُ لهذه التأثيرات أن تكون بسبب استهلاك المجرَّات الصُغرى لكميَّةٍ أقل من الغاز الموجود في مركزها، الذي تتولَّد منه النجوم الجديدة.
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The larger galaxy in the UGC 1810 - UGC 1813 pair has a mass that is about five times that of the smaller galaxy. In unequal pairs such as this, the relatively rapid passage of a companion galaxy produces the lopsided or asymmetric structure in the main spiral. Also in such encounters, the starburst
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A possible mini-spiral may be visible in the spiral arms of UGC 1810 to the upper right. It is noticeable how the outermost spiral arm changes character as it passes this third galaxy, from smooth with lots of old stars (reddish in color) on one side to clumpy and extremely blue on the other. The
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A series of uncommon spiral patterns in the large galaxy is a tell-tale sign of interaction. The large, outer arm appears partially as a ring, a feature seen when interacting galaxies actually pass through one another. This suggests that the smaller companion actually dived deep, but off-center,
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279:، المعروفة باسم UGC 1810، تتمتَّعُ بقرصٍ يخضع لعمليَّة مدٍّ وجزرٍ من الانحراف فيتشوَّه شكله ليُصبح أشبه بالوردة بسبب جاذبيَّة المجرَّة القرينة أسفله، المعروفة باسم UGC 1813. تظهرُ رُقعة من الدُرَّات الزرقاء عبر أعلى الصورة، وهي عبارة عن مجموعة من الأضواء المُنبعثة من عناقيد
334:, known as UGC 1810, has a disk that is tidally distorted into a rose-like shape by the gravitational tidal pull of the companion galaxy below it, known as UGC 1813. A swath of blue jewels across the top is the combined light from clusters of intensely bright and hot young
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activity typically begins in the minor galaxies earlier than in the major galaxies. These effects could be due to the fact that the smaller galaxies have consumed less of the gas present in their nucleus, from which new stars are born.
745:. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material.
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through UGC 1810. The inner set of spiral arms is highly warped out of the plane with one of the arms going behind the bulge and coming back out the other side. How these two spiral patterns connect is still not precisely known.
314:هذه الصورة الخاصَّة بهابل هي عبارة عن مجموعةِ من البيانات الممزوجة والمأخوذة بواسطة مُرشحات موجودة على الكاميرا سالفة الذِكر تسمحُ بعبور مجالٍ واسع من الموجات الإشعاعيَّة تُغطي الأجزاء الفوق بنفسجيَّة، والزرقاء، والحمراء للطيف.
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285:يُظهرُ الضوء المُنبعث من الطرف تقريبًا، علاماتٍ مُميَّزة تدُلُّ على وجود عنقودٍ نجميّ في وسطه، ولعلَّ ما يحثُّ هذا الضوء على الانبعاث هو التلاقي مع المجرَّة القرينة.
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The smaller, nearly edge-on companion shows distinct signs of intense star formation at its nucleus, perhaps triggered by the encounter with the companion galaxy.
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situées à environ 300 millions d'années-lumière de la Terre, dans la
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891:) and is considered one of the finest images. See its nomination
862:) and is considered one of the finest images. See its nomination
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326:image shows a group of interacting galaxies called
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737:because it was created by
638:telescópio espacial Hubble
563:costellazione di Andromeda
547:Telescopio spaziale Hubble
520:telescopio espacial Hubble
251:
246:
2440:File change date and time
2237:Portail:Astronomie/Images
1854:User:Gabrielchl/Main Page
1794:Bot: Image rotated by 90°
1676:
1402:This image is annotated:
1344:
1318:
1289:
1256:
1227:
1211:
1182:
1177:constellation d'Andromède
1154:
1145:constelación de Andrómeda
1126:
1115:, lying 300 million
1111:, a group of interacting
1098:
1073:
1054:, lying 300 million
1050:, a group of interacting
1031:on Wikimedia Commons for
872:
825:
808:
516:constelación de Andrómeda
412:constellation d'Andromède
16:
1959:Template:POTD/2014-03-01
1441:
1309:constelação de Andrômeda
1284:gwiazdozbiorze Andromedy
1262:Wykonana za pomocą
1024:
849:Picture of the Year 2016
634:constelação de Andrômeda
444:gwiazdozbiorze Andromedy
422:Wykonana za pomocą
159:members of the community
108:This is a file from the
41:
2461:04:50, 22 December 2010
1909:User talk:WindWalk55555
1823:
1793:
1763:
1733:
1352:заемоделувачки галаксии
1274:położonej 300 milionów
1223:Andromeda csillagképben
1173:galaxies en interaction
1121:constellation Andromeda
1060:constellation Andromeda
648:
575:заемоделувачки галаксии
536:Andromeda csillagképben
434:położonej 300 milionów
408:galaxies en interaction
112:. Information from its
1235:ruimtetelescoop Hubble
1188:Immagine, ripresa dal
1160:Image réalisée par le
1105:Hubble Space Telescope
1044:Hubble Space Telescope
858:on Wikimedia Commons (
815:
780:
594:ruimtetelescoop Hubble
545:Immagine, ripresa dal
395:Image réalisée par le
324:Hubble Space Telescope
115:description page there
46:Size of this preview:
2406:Horizontal resolution
1386:on Bengali Knowledge.
1324:Снимка, направена от
1295:Arp 273, um grupo de
813:
779:
763:European Space Agency
620:Arp 273, um grupo de
454:Снимка, направена от
380:تصویر گرفته شده توسط
277:المجرَّات الحلزونيَّة
2469:14:15, 18 April 2011
2443:18:15, 18 April 2011
2398:Number of components
2307:Կաղապար:Potd/2017-06
1884:User talk:Hadiyamind
1802:09:44, 24 April 2011
1772:14:00, 15 April 2017
1742:22:00, 20 April 2017
1249:in het sterrenbeeld
1237:gemaakte opname van
1198:galassie interagenti
731:This file is in the
608:in het sterrenbeeld
596:gemaakte opname van
555:galassie interagenti
330:. The larger of the
173:it using the proper
74:7,887 × 7,994 pixels
70:2,021 × 2,048 pixels
66:1,010 × 1,024 pixels
2414:Vertical resolution
2132:Шаблон:Potd/2017-06
2112:Şablon:Potd/2017-06
1712:15:23, 14 June 2017
1093:souhvězdí Andromedy
814:Picture of the year
493:souhvězdí Andromedy
368:Wide Field Camera 3
157:, which means that
52:Other resolutions:
2374:Compression scheme
2356:Bits per component
2217:الگو:نر/2016-03-21
2052:Халип:Potd/2017-06
2007:مقراب هابل الفضائي
1384:picture of the day
1264:teleskopu Hubble’a
1162:télescope spatial
1028:picture of the day
816:
781:
424:teleskopu Hubble’a
397:télescope spatial
237:Open in ZoomViewer
204:picture of the day
2493:Featured pictures
2481:
2480:
2382:Pixel composition
2321:more global usage
2297:Galaxiskeletkezés
1965:Global file usage
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908:Featured pictures
860:Featured pictures
789:
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784:
772:
718:
717:
696:
693:Reusing this file
382:تلسکوپ فضایی هابل
299:المرأة المُتسلسلة
269:مرصد هابل الفضائي
244:
243:
219:
218:
209:English Knowledge
189:
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130:
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110:Wikimedia Commons
32:Global file usage
2505:
2422:Data arrangement
2337:
2242:Angelus Silesius
1879:User:WhisperToMe
1814:
1789:SteinsplitterBot
1784:
1759:SteinsplitterBot
1754:
1724:
1686:
1626:17 December 2010
1456:
1452:Milky Way Galaxy
1448:
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1067:Other languages:
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961:featured picture
959: This is a
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940: This is a
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921: This is a
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902: This is a
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883: This is a
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