NGC 1783 (also known as ESO 85-SC29) is a globular cluster within the Dorado constellation and part of the Large Magellanic Cloud, a satellite dwarf galaxy of the Milky Way. At an aperture of 50 arcseconds, its apparent V-band magnitude is 10.39, [5] making it one of the brightest globular clusters in the LMC as viewed from Earth.

2015年8月28日 · First observed by John Herschel in 1835, NGC 1783 is nearly 160,000 light-years from Earth, and has a mass around 170,000 times that of the sun. Globular clusters are dense collections of stars held together by their own …

是 剑鱼座 的一個 星系。

2015年8月24日 · Shown here in a new image taken with the Advanced Camera for Surveys (ACS) on board the NASA/ESA Hubble Space Telescope, is the globular cluster NGC 1783. This is one of the biggest globular clusters in the Large Magellanic Cloud, a satellite galaxy of our own galaxy, the Milky Way, in the southern hemisphere constellation of Dorado.

2024年6月25日 · For NGC 1783, the age difference between the younger population and the main body is too large to be originated from native matters, contradicting the classical theoretical formation model of gravitationally bound binary clusters through the splitting of the parent cloud.

2013年3月12日 · NGC 1783 是 剑鱼座 的一個 星系。 维基共享资源 上的相關多媒體資源： NGC 1783

The presence of young stellar populations in the Large Magellanic Cloud cluster NGC 1783 has caught significant attention, with suggestions ranging from it being a genuine secondary stellar generation to a population of blue straggler stars or simply contamination from background stars.

NGC 1783是剑鱼座的一个星系。发现日期为1835年12月13日。

2015年8月31日 · This Hubble image shows globular cluster NGC 1783 in the Southern Hemisphere constellation of Dorado. NGC 1783 lies within the Large Magellanic Cloud, a satellite galaxy of our Milky Way, some 160,000 light-years from Earth.

2013年3月12日 · NGC 1783 是 剑鱼座 的一个 星系。 维基共享资源 上的相关多媒体资源： NGC 1783.