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Ngc 3324 | Sternhaufen Ngc 3324

Di: Ava

NGC 3324 is an open cluster in the southern constellation Carina, located northwest of the Carina Nebula (NGC 3372) at a distance of 7,560 ly (2,317 pc) from Earth. It is closely associated with the e

NGC 3324

용골자리 성운 (Carina Nebula) 또는 용골자리 에타 성운 (Eta Carinae Nebula), NGC 3372 는 용골자리 방향으로 지구로부터 약 8,500 광년 (2,600 pc) 거리에 밝고 어두운 성운들 이 대규모로 복잡하게 형성되어 있는 영역이다. 용골자리 성운은 우리 은하 의 용골자리-궁수자리 팔 에 위치해 있다. 용골자리 성운의

Ähnliche Suchvorgänge für Ngc 3324

This new view shows a stellar nursery called NGC 3324. It was taken using the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. The intense ultraviolet radiation from several of NGC 3324’s hot young stars causes the gas cloud to glow with rich colours and has carved out a cavity in the surrounding gas and dust. NGC 3324的觀測將揭開恆星形成的過程。 電離氣體和熱塵埃往外吹時，推擠 星雲中其他的氣體和塵埃，若遇到任何不穩定的物質，增加的壓力將觸發物質塌縮並形成新的恆星。

NGC 3324 is an open cluster in the constellation of Carina. It is associated with the emission nebula IC 2599, also known as Gum 31 and the Gabriela Mistral nebula. The open cluster is 9’100 Ly from earth. Link to interactive sky chart.

NGC 3324，又稱 加夫列拉·米斯特拉爾星雲 （英語： Gabriela Mistral Nebula），是一個位於 船底座 的 疏散星團，位於 船底座星雲 的西北角，與

Explanation: This bright cosmic cloud was sculpted by stellar winds and radiation from the hot young stars of open cluster NGC 3324. With dust clouds in silhouette against its glowing atomic gas, the pocket-shaped star-forming region actually spans about 35 light-years.

NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. The Carina Nebula is home to the Keyhole Nebula and the active, unstable supergiant star called Eta Carinae.

  • Un Volto di Poetessa nella Carena
  • Webb Reveals Cosmic Cliffs, Glittering Landscape of Star Birth
  • Combined NIRCam and MIRI Image of the “Cosmic Cliffs” in Carina
  • A NASA bemutatta a James Webb űrteleszkóppal készült

ジェームズ・ウェッブ望遠鏡が捉えたタランチュラ星雲の画像を公開何千もの若い星を発見 JWSTは観測初日から、深宇宙の華麗な姿を撮り続けている カリーナ星雲の星形成領域「NGC 3324」。 NASA, ESA, CSA, STScI

NASA Scientific Visualization Studio

Mgławica NGC 3324 to gromada jasnych gwiazd, zanurzonych w obłoku materii gazowej rozświetlonej przez niektóre z nich. Zdjęcie wykonał Teleskop Kosmiczny Hubbla. NGC 3324是位于船底座的发射星云，由天文学家詹姆士·丹露帕于1826年发现。该星云内存在被称为“宇宙悬崖“的恒星形成活跃区，位于巨大气态腔边缘区域

NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. These observations of NGC 3324 will shed light on the process of star formation. Star birth propagates over time, triggered by the expansion of the eroding cavity. As the bright, ionised rim moves into the nebula, it slowly pushes into the gas and dust. NGC 3324 – mgławica emisyjna znajdująca się w konstelacji Kila w odległości około 7500 lat świetlnych. Została odkryta 1 maja 1826 roku przez Jamesa

這張船底座星雲（Carina Nebula）的影像，看起來像是點綴著閃耀星光的山脈和峽谷。 NASA的韋伯太空望遠鏡以紅外光拍攝到附近的NGC 3324恆星形成區域邊緣，讓我們首度看到先前未曾見過的恆星誕生區域。

Den smukke stjernetåge NGC 3324 ligger ca. 7.500 lysår fra Jorden i det sydlige stjernebillede Carina (Kølen). Tågen ligger i den nordlige udkant af det kaotiske område omkring den såkaldte Carina-tåge, der er en af Mælkevejens store stjernefabrikker. NGC 3324 er selv et fødested for nye stjerner, hvilket bl.a. ses af tågens markante rødlige glød. Det er tågens skyer NGC 3324 the emission/reflection nebula is at the center of the image and is on the northern outskirts of the chaotic environment of the Carina Nebula in the constellation of Carina, and is about 10 000 light-years distance. Stellar winds and intense radiation from the young stars have blown open a hollow in the surrounding gas and dust.

NGC 3324 v Lodním kýlu Uznání a copyright: Martin Pugh Toto jasné kosmické mračno opracovaly hvězdné větry a radiace horkých mladých hvězd z otevřené hvězdokupy NGC 3324. Silueta prachových mračen proti zářícímu atomárnímu plynu v kapsovité hvězdotvorné oblasti měří asi 35 světelných let. NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina.

NGC 3324 the emission/reflection nebula is at the center of the image and is on the northern outskirts of the chaotic environment of the Carina Nebula in the constellation of Carina, and is about 10 000 light-years distance. Stellar winds and intense radiation from the young stars have blown open a hollow in the surrounding gas and dust. 지구에서 약 7,500광년 떨어진 우리은하 안에 위치해 있고 지구의 남반구에서 볼 수 있어요. 제임스웹 우주망원경이 찍은 사진은 용골자리 성운의 NGC 3324라는 부분이에요. 근적외선 카메라 (NIRCam)와 중적외선 기기 (MIRI)로 촬영했답니다.

幽靈般的船底座星雲

NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. The Cosmic Cliffs, a region at the edge of a gigantic, gaseous cavity within NGC 3324, has long intrigued astronomers as a hotbed for star formation.Many details of star formation in NGC 3324 remain hidden at visible-light wavelengths.

NGC 3324 es un cúmulo abierto en la constelación austral de Carina, ubicado al noroeste de la Nebulosa Carina (NGC 3372) a una distancia de 7600 años luz (2330 parsec) de la Tierra. [1][2][3] Está estrechamente asociada con la nebulosa de emisión IC 2599, también conocida como Gum 31. [4] A menudo se confunden las dos como un solo objeto, y juntas han sido

NGC 3324 es un cúmulo abierto en la constelación austral de Carina, ubicado al noroeste de la Nebulosa Carina (NGC 3372) a una distancia de 7600 años luz (2330 parsec) de la Tierra. 1 2 3 Está estrechamente asociada con la nebulosa de emisión IC 2599, también conocida como Gum 31. 4 A menudo se confunden las dos como un solo

Das obige Bild wurde auf den Seiten der ‚Astronomy Pictures of the Day‘ gefunden und soll den Keyhole Nebula im Innenbereich des großen Carina Nebels (NGC 3372) zeigen. Dieser wird bei den ‚Pictures of the Day‘ mit NGC 3324 gleichgesetzt. Diese Bezeichnung widerspricht allen Zuordnungen in den Katalogen.

NGC 3324 Az Éta-Carinae-csillagködhöz tartozó NGC 3324 csillagkeletkezési régió a Naprendszer egyik legaktívabb területe, amelyben ma is számos új csillag keletkezik. Neue Bilder des James Webb-Teleskopes: ein Einblick in den Carinanebel, er zeigt die relativ junge Region NGC 3324, in der sich Sterne

Discover when and where to find NGC3324 in the night sky. Learn about NGC3324 rise and set times, its path across the sky, and the best time for viewing.

Webb reveals “Cosmic Cliffs”

NGC 3324 ilk kez 1826’da James Dunlop tarafından kataloglanmıştır. Güney Yarımküreden gözlenebilen bulut, Karina takımyıldızındaki Karina Bulutsusunun (NGC 3372) kuzeybatı köşesinde yer alır. Karina Bulutsusunda, Anahtar Deliği Bulutsusu ve Eta Karina adlı aktif, kararsız üstdev yıldız da bulunmaktadır. ESA NGC 3324 هو عنقود مفتوح يقع في الجزء الشمالي الغربي من سديم القاعدة (Carina Nebula (NGC 3372، [4][5] أكتشف في عام 1826 من قبل جيمس دنلوب . [4]

NGC 3324 is a Star Cluster + Nebula in the Carina constellation. NGC 3324 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere.

這是一個驚人的畫面，恆星風通過一個遙遠的星雲的羽毛狀雲彩削減強烈的紫外線輻射創造了一個幽靈般的臉。從位於智利的拉西拉天文台的圖像揭示了船底座星雲的大質量恆星誕生地和大量恆星形成星座的區域NGC 3324——「星雲的臉」。 Il nome popolare di NGC 3324 è Nebulosa Gabriela Mistral, dalla poetessa cilena insignita del Nobel, per la somiglianza del bordo della parete di gas e polveri visibile sulla destra con un volto umano di profilo, con la sporgenza al centro corrispondente al naso. Located roughly 7,600 light-years away, NGC 3324 was first catalogued by James Dunlop in 1826. Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina.

The Gabriela Mistral Nebula, designated NGC 3324, is an emission nebula located in the Carina constellation, approximately 7,200 light-years from Earth. This region is a stellar nursery, where intense

Lizenz Diese Datei ist gemeinfrei, da sie von NASA und ESA erstellt wurde. Das Hubble-Material der NASA (und das Hubble-Material der ESA vor 2009) ist urheberrechtsfrei und kann ohne Gebühr als gemeinfrei verwendet werden, sofern nur die NASA, das STScI und/oder die ESA als Quelle des Materials angegeben werden. Diese Lizenz gilt nicht, wenn ESA-Material, das nach