NGC 4848 is a barred spiral galaxy in the constellation Coma Berenices. It is circa 340 million light-years from Earth, which, given its apparent dimensions, means that NGC 4848 is about 170,000 light years across.

2020年7月24日 · In this image, taken with the NASA/ESA Hubble Space Telescope, the stunning silvery-blue spiral arms of the galaxy NGC 4848 are observed in immense detail. Not only do we see the inner section of the spiral arms containing hundreds of thousands of young, bright, blue stars, but Hubble has also captured the extremely faint, wispy tails of the ...

2020年7月20日 · Astronomers classify NGC 4848 as an active barred spiral galaxy. “A notable feature of most spiral galaxies is the multitude of arching spiral arms that seemingly spin out …

NGC 4848 is an Active Galactic Nuclei/Nucleus located in the constellation of Coma Berenices in the northern hemisphere. NGC 4848's distance from Earth is 339,936,484.65 light years. NGC 4848 is called NGC 4848 in the New General Catalogue (NGC).

2020年7月20日 · In this image, taken with the NASA/ESA Hubble Space Telescope, the stunning silvery-blue spiral arms of the galaxy NGC 4848 are observed in immense detail. Not only do we see the inner section of the spiral arms containing hundreds of thousands of young, bright, blue stars, but Hubble has also captured the extremely faint wispy tails of the ...

2020年7月26日 · In this image, taken with the NASA/ESA Hubble Space Telescope, the stunning silvery-blue spiral arms of the galaxy NGC 4848 are observed in immense detail.

圖中螺旋星系 NGC 4848 位於 后髮座（Coma Berenices） 中。 這顆毛茸茸的棒旋星系最早是由德國天文學家羅雷爾·路德威·德亞瑞司特（德語：Heinrich Louis d'Arrest）在 1865 年發現的。

NGC 4848 is a barred spiral galaxy in the constellation Coma Berenices. It is circa 340 million light-years from Earth, which, given its apparent dimensions, means that NGC 4848 is about 170,000 light years across.

The astronomical object called NGC 4848 is a Active Galaxy Nucleus

Of these, 3 central subclusters around thegalaxies NGC 4889, NGC 4874, and NGC 4839 have been singled out. We haveused the objective statistical criterion applied by Vennik and Anosovain studies of close groups of galaxies to evaluate each member includedin a …