NGC 4383 是 室女座星系團 的成員，但位於 后髮座 的一個 螺旋星系。 愛德華·舍恩菲爾德 （英语：Eduard Schönfeld） 於1862年5月23日被發現了它 [2]。 它是星系團中最富氫的星系之一，擁有6千秒差距（20,000光年）的雙極外流，平均速度為每秒210公里。

NGC 4383 is a spiral galaxy located in the constellation Coma Berenices, within the Virgo Cluster. It was discovered on 23 May 1862 by Eduard Schönfeld. [2] It is one of the most H I-rich galaxies in the cluster, hosting a 6-kiloparsec (20,000 ly) bipolar outflow, travelling at an average velocity of 210 kilometres per second.

2025年3月18日 · NGC 4383 is about 60 million light-years away. It’s a member of the Virgo Cluster – a collection of hundreds of galaxies. Like our home galaxy, the Milky Way, NGC 4383 is a spiral. Bright “arms” of hot, young stars wrap around the galaxy’s heart. The galaxy is a hotbed of star formation – it’s giving birth to thousands of stars.

2024年4月22日 · Located around 62 million light-years from Earth, NGC 4383 is part of the Virgo Cluster and is undergoing a strange and turbulent evolution. This includes the galaxy spitting out an outflow of...

2024年4月22日 · A team of international researchers studied galaxy NGC 4383, in the nearby Virgo cluster, revealing a gas outflow so large that it would take 20,000 years for light to travel from one side to the...

2024年4月22日 · Researchers investigated the galaxy NGC 4383 in the neighboring Virgo cluster, discovering a massive gas outflow that light would take 20,000 years to get from one side to the other. This gas outflow is caused by highly intense stellar explosions in the galaxy’s central regions, which can emit massive amounts of hydrogen and heavier elements.

NGC 4383 is an Active Galactic Nuclei/Nucleus located in the constellation of Coma Berenices in the northern hemisphere. NGC 4383's distance from Earth is 62,008,850.53 light years.

Virgo HI Galaxy Survey - NGC 4383

2025年3月18日 · Coma Berenices is low in the eastern sky in early evening. It consists of a faint spray of sparkly stars, although you need dark skies to see them. Many galaxies lie within it, including NGC 4383, which is puffing out a chimney of gas that’s 20,000 light-years long.

NGC 4383 是 室女座星系团 的成员，但位于 后发座 的一个 螺旋星系。 爱德华·舍恩菲尔德 （英语：Eduard Schönfeld） 于1862年5月23日被发现了它 [2]。 它是星系团中最富氢的星系之一，拥有6千秒差距（20,000光年）的双极外流，平均速度为每秒210公里。