Home

NGC 1277

NGC 1277. في الفهرس العام الجديد NGC 1277 هي مجرة محدبة من القدر 14.7m. تقع على مسافة تقدر بحوالي 220 مليون سنة ضوئية 65.9 مليون فرسخ فلكي من النظام الشمسي في كوكبة حامل رأس الغول وتنتمي لعنقود مجرات حامل رأس الغول. اكتشفت في 4 ديسمبر 1875 من قبل لورانس بارسونز، إيرل روس الرابع NGC 1277 is a relatively small galaxy, only 10 percent the mass and size of the Milky Way, yet the black hole is about 4,000 times larger than the one lying at the core of our galaxy. For comparison, the mass of the Milky Way's central bulge is around 20 billion solar masses,. find me:https://soundcloud.com/p98_tthttps://www.facebook.com/p98.tt/https://www.instagram.com/p98_live/https://www.residentadvisor.net/dj/p98_liv

Ngc 1277 - ويكيبيدي

ngc 1277 هى مجره بتتبع كوكبه حامل راس الجول و اللى اكتشفها لاورينس پارسونس, 4ث ايرل اوف روس و الاكتشاف كان بتاريخ 4 ديسمبر 1875. معلومات المجره. الانزياح الأحمر: 0.0166~|~0.016618 . (((Connect with me - https://linktr.ee/Dillon398)) NGC 1277 ist eine linsenförmige Galaxie vom Hubble-Typ S0 im Sternbild Perseus am Nordsternhimmel mit einem supermassereichen Schwarzen Loch im Zentrum. Sie ist schätzungsweise 231 Millionen Lichtjahre von der Milchstraße entfernt, hat einen Durchmesser von etwa 55.000 Lj und ist Mitglied des Perseus-Haufens Abell 426 NGC 1277 è una galassia lenticolare che si trova prospetticamente nella costellazione di Perseo all'incirca a 220 milioni di anni luce dalla Via Lattea. Fa parte dell' Ammasso di Perseo (o Abell 426 ). È principalmente conosciuta per la possibile presenza di un buco nero supermassiccio al suo interno

NGC 1277: Supermassive Black Hole in Lenticular Galaxy

NGC 1277 (również PGC 12434) - galaktyka soczewkowata (S0-a), znajdująca się w gwiazdozbiorze Perseusza w odległości 220 milionów lat świetlnych. Galaktyka została odkryta 4 grudnia 1875 roku przez Lawrence'a Parsonsa. Należy do Gromady w Perseuszu. Charakterystyka fizyczn NGC 1277 é uma galáxia lenticular localizada na direcção da constelação de Perseus. Possui uma declinação de +41° 34' 27 e uma ascensão recta de 3 horas , 19 minutos e 51,4 segundos . NGC 1277 foi descoberta em 4 de Dezembro de 1875 por Lawrence Parsons ngc 1277は、ペルセウス座の方向に地球から2億2000万光年離れた位置にある小さなレンズ状銀河である 。 ngc 1277の中心部には、2012年になって太陽の170 ± 30億倍という超大質量ブラックホールが発見された 。質量は恒星の動きから推定された NGC 1277 - Lenticular Galaxy in Perseus. NGC 1277 is a Lenticular Galaxy in the Perseus constellation.NGC 1277 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere NGC 1277. The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature. Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system)

Astronomers puzzled over huge black hole in the middle of

Video: P98 - NGC 1277 - YouTub

NGC 1277 est une galaxie lenticulaire située dans la constellation de Persée à environ 231 millions d'années-lumière de la Voie lactée. Elle a été découverte par l'astronome irlandais Lawrence Parsons en 1875 [6]. Des mesures non basées sur le décalage vers le rouge (redshiftMpc (∼186 millions d'a.l.) [9], ce qui est à l'extérieur de NGC 1277 — компактная линзовидная галактика в созвездии Персей. Галактику открыл британский астроном Лоренс Парсонс. Звёздное население галактики очень старое, звездообразование в ней завершилось более 8 млрд лет назад. Находится на расстоянии 220 млн световых лет от Земли.

NGC 1277 (također poznat kao MCG 7-7-64 i PGC 12434) je spiralna galaksija koja je udaljena oko 233 miliona sg od Zemlje i nalazi se u sazviježđu Perzej.Najveći prečnik je 0,80 (54 hiljade sg) a najmanji 0,3 uglovnih minuta (20 hiljada sg). Prvo otkriće je napravio Lawrence, 4.Earl of Rosse Parsons 4. decembra 1875. godine في الفهرس العام الجديد NGC 1277 هى مجرة محدبة من القدر 14.7m. [1 NGC 1277 bývá nazývána jako pozůstatek raného vesmíru, protože se její hvězdy tvořily během 100 miliónů let dlouhého období před více než dvanácti miliardami let, když byl vesmír starý pouze 2 miliardy let

Ngc 1277 (مجره) - ويكيبيدي

  1. ngc 1277 Викиҗыентыкта NGC 1277 — Томанлыклар һәм йолдыз тупланмалары яңа гомуми каталогында теркәлгән галактика
  2. NGC 1277是在天球上位於英仙座的透鏡狀星系。該星系是英仙座星系團的成員星系，距離銀河系約7300萬秒差距 或2.2億光年。該星系的視星等14.7。1875年12月4日，天文學家 勞倫斯·帕森思，第四代羅斯伯爵 （ 英语 ： Lawrence Parsons, 4th Earl of Rosse ） 發現NGC 1277
  3. Media in category NGC 1277 The following 8 files are in this category, out of 8 total. NGC 1273 SDSS.jpg. NGC 1274 SDSS.jpg. NGC 1277 SDSS.jpg. NGC 1277 viewed by Hubble.jpg. NGC 1278 SDSS.jpg. NGC1277 - SDSS DR14.jpg 800 × 800; 62 KB. NGC1277 NGC1278 - HST - Potw1812a.tiff
  4. Навигацин тӀегӀо Лахарна тӀегӀо. NGC 1277. Каталоган код. NGC 1277, PGC 12434, 2MASX J03195148+4134242, MCG+07-07-064, Z 540-104, Z 0316.6+4123, UZC J031951.6+413425, LEDA 12434, [BM99] 274. Юьхь йиллинарг я кхоллархо
  5. NGC 1277, yew cısmê asmêniyo. No cısım Katalogê Neweyê Pêroyi de ca gêno. 4 Kanun 1875 de terefê Lawrence Parsonsi ra keşıf biyo. Bıvênên. Asmên; Galaksi; Pulsar; Nebula; Lista cısmanê NGC; Gırey teberi. Heqa NGC 1277 sitay NASA/IPAC Extragalactic Database sero bıvênê (be İngılızki

NGC 1277是在天球上位于英仙座的透镜状星系。该星系是英仙座星系团的成员星系，距离银河系约7300万秒差距或2.2亿光年。该星系的视星等14.7。1875年12月4日，天文学家劳伦斯·帕森思，第四代罗斯伯爵发现NGC 1277 NGC 1277 là một thiên hà hình hạt đậu trong chòm sao Anh Tiên.Nó là một thành viên của cụm Perseus và nằm khoảng 73Mpc (Mega parsec) hay 220 triệu năm ánh sáng từ Ngân Hà.Nó có cấp sao biểu kiến là khoảng 14,7. Nó được phát hiện vào ngày 4 tháng 12 năm 1875 bởi Lawrence Parsons, Bá tước thứ tư của Rosse ngc 1278 في الفهرس العام الجديد، هي مجرة، تقع في كوكبة حامل رأس الغول. اكتشفت في 14 فبراير 1863 بواسطة ويليام هيرشل . مراجع [ عدل NGC 1277, Yeni Genel Katalog'da yer alan bir merceksi galaksidir.Gökyüzünde Kahraman takımyıldızı yönünde yaklaşık olarak 218,52 MIy (67 Mpc) uzaklıkta bulunur.İngiliz astronom Lawrence Parsons tarafından 1875 yılında 182,88 cm (72 inç) çaplı aynalı tip bir teleskopla keşfedilmiştir.. 28 Kasım 2012 tarihinde Almanya'daki Max Planck Enstitüsü'ne bağlı gökbilimciler.

NGC 1277 Blackhole Sounds - YouTub

  1. NGC 1277 es una galaxia lenticular localizada en la constelación de Perseo.Está situada a aproximadamente 220 millones de años luz de distancia de la Vía Láctea, y es mejor conocida por contener un agujero negro supermasivo.. NGC 1277 fue dada a conocer inicialmente después de las observaciones realizadas en Irlanda por parte de Lawrence Parsons el 4 de diciembre de 1875
  2. NGC 1277 by The Soviet Space Dog Project, released 25 August 2019 1. Relic of the Early Universe An album about deep space exploration, i.e. it has absolutely no beats at all. So, stop worrying about Earthly things, put on some headphones and drift away to that far distant galaxy for half an hour
  3. The NGC 1277 black hole provides new information in the quest to understand the relationship between galaxies and their central black holes. Over a couple of decades, astronomers observed that there is a relationship between the mass of a galactic black hole and the mass of the bulge of stars around it
  4. NGC 1277: A Massive Compact Relic Galaxy in the Nearby Universe. As early as 10 Gyr ago, galaxies with more than 10 11 M ⊙ of stars already existed. While most of these massive galaxies must have subsequently transformed through on-going star formation and mergers with other galaxies, a small fraction (lsim0.1%) may have survived untouched.
  5. NGC 2000.0: NGC 1277: HYPERLEDA-I: PGC 12434 → Request more catalogs and designations from VizieR.
  6. NGC 1277 Location. The NGC 1277's location is 03 19 51.488 (R.A.) and +41 34 24.26 (Dec.). The Right Ascension is the angular distance of an object along the celestial equator from the March Equinox. As rough guide, the location is located in the constellation of Pisces. If the number is negative, it is west of the March Equinox

NGC 1277 is a small, flattened lenticular galaxy of roughly 25,000 light-years across, located about 220 million light-years away in the constellation of Perseus, while speeding away from us at approximately 5066 kilometers per second. It is a member of the Perseus Cluster of Galaxies NGC 1277 is moving so fast through the cluster, at 2 million miles per hour, that it cannot merge with other galaxies to collect stars or pull in gas to fuel star formation. In addition, near the galaxy cluster center, intergalactic gas is so hot it cannot cool to condense and form stars NGC 1277 is located at a distance of around 250 million light-years, toward the constellation Perseus. This Hubble image shows lenticular galaxy NGC1277 Astronomers measured the mass of the object at the center of NGC 1277 to be around 17 billion times the mass of the Sun, which is over four thousand times more massive than the 4 million solar. NGC 1277 is embedded in the Perseus galaxy cluster, some 220 million light-years away. Early this year, NASA released a report suggesting that the 20 million mph (32 million km/h) winds associated with the presence of similarly massive black holes may prevent the formation of new stars. This seems to correspond with the lack of star formation.

The unusual black hole has been detected in a lenticular galaxy known as NGC 1277 with the Hobby-Eberly Telescope (HET) at the McDonald observatory in Texas. The lenticular galaxy NGC 1277 lies. The black hole in NGC 4889 is estimated to have a mass of 21 billion suns, according to The New York Times. Gebhardt, who worked on the NGC 4889 study, said that the estimate for the black hole in that galaxy is between 6 billion and 25 billion solar masses. The range for NGC 1277 is 14 billion to 20 billion solar masses, he said

NGC 1277 has recently received a lot of attention due to the claim by van den Bosch et al. that this object has an extraordinary large supermassive black hole (SMBH). Interestingly, NGC 1277 is massive ( M = 1.2 ± 0.4 × 10 11 M ☉ ) and compact ( R e = 1.2 kpc), two of the three properties we require for a massive galaxy to be a relic NGC 1277 är en linsformad spiralgalax i stjärnbilden Perseus, belägen omkring 220 miljoner ljusår bort.. Den 28 november 2012 upptäckte astronomer vid Max Planck-institutet för astronomi ett supermassivt svart hål i galaxens mitt, vilket är ett av universums största hittills upptäckta, med en massa motsvarande 17 miljarder Solmassor. [1] Hålet har en massa som är 14 procent av hela. NGC 1277 has previously been proposed to host an overmassive black hole (BH) compared to the galaxy bulge luminosity (mass), based on stellar-kinematic measurements. The CO (1-0) emission, observed with the IRAM Plateau de Bure Interferometer (PdBI) using both, a more compact (2.9-arcsec resolution) and a more extended (1-arcsec resolution.

Putting into perspective just how big the black hole of

NGC 1277 ye una galaxa espiral alcontrada na constelación de Perséu. Ta asitiada a aprosimao 220 millones d'años lluz de distancia de la Vía Lláctea, y ye meyor conocida por contener un furacu prietu supermasivu.. NGC 1277 foi dada a conocer primeramente dempués de les observaciones realizaes n'Irlanda per parte de Lawrence Parsons el 4 d'avientu de 1875 Listen to music from NGC_1277's library (51,982 tracks played). NGC_1277's top artists: Steve Roach, Benighted in Sodom, Mathias Grassow. Get your own music profile at Last.fm, the world's largest social music platform

NGC-1277- 0 points 1 point 2 points 2 months ago * Taken with a Sony a6000 I'm still learning all the settings and need to purchase a lens that has a lower aperture (currently this is 4.5f). permalin NGC 1277. The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature. Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). Link by name to the catalogue in VizieR

We all know how large VY Canis Majoris is, but adding

Here we report observations of the stellar kinematics of NGC 1277, which is a compact, lenticular galaxy with a mass of 1.2 × 10 11 solar masses. From the data, we determine that the mass of the central black hole is 1.7 × 10 10 solar masses, or 59 per cent of its bulge mass The filaments persist in NGC 1275 even though the turmoil of galactic collisions should destroy them. First, active galaxy NGC 1275 is the central, dominant member of the large and relatively nearby Perseus Cluster of Galaxies. Wild-looking at visible wavelengths, the active galaxy is also a prodigious source of x-rays and radio emission

NGC 1277 - Wikipedia, wolna encyklopedi

NGC 1277 also has a black hole at its center that's absurdly large for such a small galaxy. It's possible that although the galaxy's black hole grew in size, NGC 1277 didn't have the gases. NGC 1278 is an elliptical galaxy located about 230 million light-years away in the constellation Perseus. NGC 1278 was discovered by astronomer Heinrich d'Arrest on February 14, 1863. It was then rediscovered by astronomer Guillaume Bigourdan on October 22, 1884 and was later listed as IC 1907. NGC 1278 is a member of the Perseus Cluster and is a low-luminosity AGN (LLAGN)

NGC 1277是在天球上位于英仙座的透镜状星系。 该星系是英仙座星系团的成员星系，距离银河系约7300万秒差距 或2.2亿光年。 该星系的视星等14.7。1875年12月4日，天文学家 劳伦斯·帕森思，第四代罗斯伯爵 （ 英语 ： Lawrence Parsons, 4th Earl of Rosse ） 发现NGC 1277。. NGC 1277因为其恒星是在约120亿年前以每1亿. The massive relic galaxy NGC 1277 has few blue globular clusters, indicating that it has undergone little mass accretion and is a candidate 'red nugget' in the nearby Universe. Globular. 13,7. Prividne dimenzije (V) 1.0'x0.4'. Stvarne osobine objekta. Ostalo. Druge oznake. MCG +07-07-064, CGCG 540.104, PGC 12434. NGC 1277 je lećasta galaksija u zviježđu Perzej. Otkrio ju je Lawrence Parsons 4. prosinca 1875 NGC 1277是在天球上位於英仙座的透鏡狀星系。該星系是英仙座星系團的成員星系，距離銀河系約7300萬秒差距[2]或2.2億光年。該星系的視星等14.7。1875年12月4日，天文學家勞倫斯·帕森思，第四代羅斯伯爵（英語：Lawrence Parsons, 4th Earl of Rosse）發現NGC 1277 NGC 1277 was a Red Hypergiant that was angery because he will be a supernova right now. He now became a supernova, and will become a Black Hole right now. He now is a Black Hole, and is sad because he did NOT become a Metagiant star. Community content is available under CC-BY-SA unless otherwise noted. Let's Go Luna

NGC 1277 - Wikipédia, a enciclopédia livr

NGC 1277의 성장이 멈춘 명확한 원인은 은하 주변에 밀집되어 있는 오래된 구상 성단에 있다. 이 은하계는 지구에서 2억 4천만광년 떨어진 곳에 위치한 1,000개 이상의 은하로 이루어진 페르세우스 은하단의 중심 근처에 살고 있다. NGC1277은 시속 320만km로 은하단을. NGC 1277, Yeni Baş Kataloqda qeydə alınmış qalaktikadır. Göy üzündə Persey bürcü istiqamətində yerləşir. S0-a tipli qalaktikadır. İngilis astronomu Lawrence Parsons tərəfindən 1875-ci ildə 182.88 sm (72 düymə) ölçülü reflektor vasitəsilə ildə kəşf edilmişdir This diagram shows how the diamater of the 17-billion-solar-mass black hole in the heart of galaxy NGC 1277 compares with the orbit of Neptune around the Sun. The black hole is eleven times wider than Neptune's orbit. Shown here in two dimensions, the edge of the black hole is actually a sphere. This boundary is called the event horizon, the point from beyond which, onc NGC 1277 је лентикуларна галаксија у сазвежђу Персеј која се налази на NGC листи објеката дубоког неба.. Деклинација објекта је + 41° 34' 27 а ректасцензија 3h 19m 51,4s. Привидна величина (магнитуда) објекта NGC 1277 износи 13,8 а.

NGC 1277 - Lenticular Galaxy in Perseus TheSkyLive

  1. uta) Rektascenzija Deklinacija (astronomija) Tip; NGC 1281: 0,06 3 sat. 20 m 6,3 s +41° 37' 47'' eliptična galaksija () : NGC 1277
  2. Medien in der Kategorie NGC 1277 Folgende 8 Dateien sind in dieser Kategorie, von 8 insgesamt
  3. ngc 1277 — леќеста галаксија во соѕвездието Персеј, заведена во Новиот општ каталог на објекти на длабокото небо.. Објектот бил предмет и на други истражувања, па освен како ngc 1277 се споменува и како mcg 7-7-64, cgcg 540-104
  4. ngc 1277 — галактика типу s0-a у сузір'ї Персей.. Відкривачем цього об'єкта є Лоренс Парсонс, четвертий ерл Росс, який уперше спостерігав за об'єктом 4 грудня 1875.. Цей об'єкт міститься в оригінальній редакції Нового.
  5. NGC 1277 Persey yulduz turkumidagi S0-a tipli galaktikadir. Somon Yoʻlidan taqriban 220 million yorugʻlik yili uzoqlikda joylashgan.. Ushbu obyektni Lawrence Parsons 1875-yilda kashf etgan.. Ushbu obyekt Yangi umumiy katalog asl nashrida mavjud.. Qora tuynuk. 2012-yil 28-noyabrida Olmoniyaning Max Planck Astronomiya Instituti astronomlari NGC 1277 galaktikasi markazida oʻta massiv qora.

A diferencia de la cercana galaxia NGC 1277, que tiene una población de cúmulos dominantes de metal rico o rojo, NGC 1278 tiene una rica población de cúmulos de ambos azules de metales ricos y pobres. [6] Ver también. Lista de objetos NGC (1001-2000) NGC 1275; NGC 1277; Referencia NGC 1278 = IC 1907 ist eine elliptische Galaxie vom Hubble-Typ E2 im Sternbild Perseus am Nordsternhimmel.Sie ist schätzungsweise 277 Mio. Lichtjahre von der Milchstraße entfernt, hat einen Durchmesser von etwa 115.000 Lj und ist Mitglied des Perseus-Haufens Abell 426.. In derselben Himmelsregion liegen die Galaxien NGC 1274, NGC 1275, NGC 1277, NGC 1281 NGC 1277 je galaxia v súhvezdí Perzeus, ktorú objavil írsky astronóm Lawrence Parsons 4. decembra 1875. Jej zdanlivá hviezdna veľkos.

NASA finds 'Lost Galaxy' shining out of Virgo's bosom

NGC 1277 - unistra.f

In the case of the NGC 1277 disk galaxy, the astronomers arrived at around 17 billion solar masses. Researchers don't know what the current record holder might be, estimates range from 6 and 37 billion solar masses, so if the true value is at the lower end, NGC 1277 will hold the record A ground-based view of NGC 1277. It is the small, flattened galaxy at center, just to the upper right of a large round galaxy. This diagram shows the size of the NGC 1277 black hole, with the orbits of Neptune and Earth around the Sun at the same scale The galaxy NGC 1277 (center) is embedded in the nearby Perseus galaxy cluster. All the ellipticals and round yellow galaxies in the picture are located in this cluster. NGC 1277 is a relatively compact galaxy compared to the galaxies around it. The Perseus cluster is 250 million light years from us. Credit: David W. Hogg, Michael Blanton, and the SDSS Collaboratio Hubble Image of the Week - Lenticular Galaxy NGC 1277. This idyllic scene, packed with glowing galaxies, has something truly remarkable at its core: an untouched relic of the ancient Universe. This relic can be seen in the large galaxy at the center of the frame, a lenticular galaxy named NGC 1277. This galaxy is a member of the famous. NGC 1277 and the other Perseus core UMBH, NGC 1270, have not, however, been able to gather more stars or gas owing to their rapid orbital motion in the cluster core. View. Show abstract

NGC 1277 — Wikipédi

  1. NGC 1277 - линзовидная галактика, удаленная на 220 миллионов лет. Проживает в Персее, а по видимой величине достигает 14.7. В центре скрывается огромная черная дыра. Примечательна тем, что по.
  2. Apart from NGC 1277, NGC 4486B 9 and Henize 2-10 17 are known to lie significantly above the relations, and at least three galaxies are known to lie significantly below the relations 10,18,19. We.
  3. Enter a coin's NGC certification number (circled in the image) and grade to confirm its description and grade in NGC's database and, if available, view the images of the coin taken by NGC. For coins that have a grade of 1 to 70, enter the certification number, select the numeric grade in the dropdown menu and click Go
  4. dfyh1993的博客. 12-08. 1万+. Java Package. isAnnotationPresent()方法 用法实例教程。. 方法 返回true，如果指定类型的注释存在于此元素上,否则返回false。. 这种 方法 的设计主要是为了方便访问标记注释 描述 java.lang.Package. isAnnotationPresent( Class annotation Class) 方法 返回true.
  5. NGC 1277 glows red, proof that it's development was stunted during the early stages of its evolution. Photo by NASA/ESA/M. Beasley/Instituto de Astrofísica de Canarias. March 13 (UPI) -- New.
  6. A A. NGC 1277, considered a relic galaxy that has gone unchanged for the past 10 billion years, was discovered by Earth-bound astronomers using NASA's Hubble Space Telescope, according to a statement from the space agency. Details of NGC 1277 were published in Monday's edition of science journal Nature, where researchers said the galaxy once.
  7. NGC 1277 belongs to a cluster of galaxies in the constellation Perseus and is a type common in clusters: The galaxy is a so-called lenticular galaxy, a cross between a spiral and an elliptical galaxy. Like a spiral galaxy, NGC 1277 has a disk of stars, but like an elliptical galaxy, it no longer gives birth to any more
Over-massive black hole in compact galaxy NGC1277 on Vimeo

Ngc 1277 — Википеди

Abstract: The nearby lenticular galaxy NGC 1277 is thought to host one of the largest black holes known, however the black hole mass measurement is based on low spatial resolution spectroscopy. In this paper, we present Gemini Near-infrared Integral Field Spectrometer observations assisted by adaptive optics. We map out the galaxy's stellar kinematics within ~440 pc of the nucleus with an. NGC 1277. Idi na navigaciju Idi na pretragu. NGC 1277. galaksija. Otkriće: Položaj Epoha J2000.0: Zviježđe: Perzej Rektascenzija: 03 h 19 m 51.4 s: Deklinacija +41° 34′ 25″ Izgled na našem nebu: Prividna magnituda: 13,7 Prividne dimenzije (V) 1.0'x0.4' Stvarne osobine objekta. Sorpresa: nella galassia NGC 1277 un buco nero con una massa di 17 miliardi di soli. Un gruppo di astronomi guidato da Remco van den Bosch, del Max Planck Institute for Astronomy (MPIA) ha scoperto un buco nero che potrebbe scuotere le fondamenta degli attuali modelli sull'evoluzione delle galassie. La sua massa è di 17 miliardi di soli.

NGC 1277 NGC 1277 : La galaxie lenticulaire NGC 1277 : Données d'observation (Époque J2000.0) Constellation: Persée: Ascension droite (α) 03 h 19 m 51,5 s [1] Déclinaison (δ) 41° 34′ 25″ Magnitude apparente (V) 13,6 [2] 14,7 dans. ngc 1277. beni hala niye traş oluyoruz diye derin derin düşündüren kara deliktir. buyukluk kistasi belirtilmemistir. sıçarken bunu bile denk getiremeyecek adamlar vardır. ağızlarına sıçtıklarımının. boyu değil işlevi mühim olan kara deliktir. deliğin kütlesi mi olur lan diyerek kendisine çıkıştığım, aklımın. Den NGC 1277 ass eng lënsefërmeg Galaxis am Stärebild Perseus.Si ass ronn 220 Millioune Liichtjoer vun der Mëllechstrooss ewech. Den NGC 1277 gouf de 4.Dezember 1875 vum ireschen Astronom Lawrence Parsons entdeckt.. Den 28.November 2012 hu Physiker vum Max-Planck-Institut fir Astronomie entdeckt, datt dat Schwaarzt Lach am Zentrum vun der Galaxis eent vun de masseräichsten ass, dat bis. Ouça músicas na biblioteca de NGC_1277 com (52.136 faixas executadas). Principais artistas de NGC_1277: Steve Roach, Benighted in Sodom, Mathias Grassow. Crie seu próprio perfil musical na Last.fm, a maior plataforma social de músicas do mundo ngc 1277は「ペルセウス座銀河団」を構成する1000以上の銀河のひとつです。ngc 1277には天の川銀河の2倍の星々があるものの、そのサイズは直径約10.

Ngc 1277 - يونيونبيديا، الشبكة الدلالي

NGC 1277 (aliaj indikoj — PGC 12434, MCG 7-7-64, ZWG 540.104) estas galaksio en konstelacio Perseo. Ĉi tiu objekto estis jam en la originala versio de NGC-katalogo. Vidu ankaŭ. Messier-katalogo; NGC-katalog La galaxia NGC 1277 está compuesta solo por los cúmulos globulares rojos que se crearon con ella, y desde entonces se conserva inalterada. El autor del primer artículo sobre el tema en la revista Nature , Michael Beasley, explica que los cúmulos son piezas muy sensibles a la hora de formarse las galaxias NGC 1277 si trova a circa 220 milioni di anni-luce nella costellazione del Perseo e ha una massa e una dimensione pari al 10% rispetto alla Via Lattea. Nonostante le dimensioni ridotte della galassia, il buco nero si estende per ben 11 volte le dimensioni dell'orbita di Nettuno attorno al Sole NGC 1277 bývá nazývána jako pozůstatek raného vesmíru, protože se její hvězdy tvořily během 100 miliónů let dlouhého období před více než dvanácti miliardami let, když byl vesmír starý pouze 2 miliardy let. Po tomto výbuchu vznikání nových hvězd, tisíckrát rychlejšího než při vzniku Mléčné dráhy, tato. ngc 1277 (другие обозначения — mcg 7-7-64, zwg 540.104, pgc 12434) — компактная линзовидная галактика в созвездии Персей.Галактику открыл британский астроном Лоренс Парсонс. Звёздное население галактики очень старое.

Brève | Magnifique portrait d'une galaxie spirale où 5(NGC 4490), out of frame and now 24,000 light-years away

Az NGC 1275 5264 km/s sebességgel távolodik tőlünk, vöröseltolódása z=0.017559. Megfigyelési lehetőség. Kis távcsövekkel elég nehéz megfigyelni, mivel elég halvány (12,6 magnitúdós). Egy 20 centiméteres távcsővel, tiszta éjszakán halvány fényű, szemcsés, kicsiny fényfoltnak látható. Forráso NGC 1275 (również Perseusz A, PGC 12429 lub UGC 2669) - galaktyka soczewkowata (S0), znajdująca się w gwiazdozbiorze Perseusza w odległości 230 milionów lat świetlnych.Została odkryta 17 października 1786 roku przez Williama Herschela.Galaktyka ta rozciąga się na przestrzeni około 100 000 lat świetlnych NGC 1217-2 (također poznat kao ESO 300-10, MCG -7-7-2 i PGC 11642) je spiralna galaksija koja je udaljena oko 298 miliona sg od Zemlje i nalazi se u sazviježđu Hemijska peć.Najveći prečnik je 0,50 (43 hiljade sg) a najmanji 0,4 uglovnih minuta (35 hiljada sg) NGC 천체목록 [편집] 정식 명칭은 'New General Catalogue of Nebulae and Cluster of Stars'이다. 인류가 관측한 성단, 성운 및 은하를 체계적으로 정리하여 천구좌표계의 적경에 따라 번호를 부여한 일람으로 메시에 천체 목록 과 함께 천문분야에서 널리 사용되고 있다. 한국어.