NGC 1569 is a dwarf irregular galaxy in Camelopardalis. The galaxy is relatively nearby and consequently, the Hubble Space Telescope can easily resolve the stars within the galaxy. [3] The distance to the galaxy was previously believed to be only 2.4 Mpc (7.8 Mly). [4]

2016年7月1日 · This NASA/ESA Hubble Space Telescope image reveals the iridescent interior of one of the most active galaxies in our local neighborhood — NGC 1569, a small galaxy located about eleven million light-years away in the constellation of Camelopardalis (The Giraffe).

2008年11月20日 · NGC 1569 is pumping out stars at a rate that is 100 times faster than the rate observed in our Milky Way Galaxy. This frenzied pace has been almost continuous for the past 100 million years. The core's centrepiece is a grouping of three giant star clusters, each containing more than a million stars.

2024年2月16日 · NGC 1569 is pumping out stars at a rate that is 100 times faster than the rate observed in our Milky Way Galaxy and has been almost continuously for the past 100 million years. The core's centerpiece is a grouping of three giant star clusters, each containing more than a …

Two massive star clusters - youthful counterparts to globular star clusters in our own spiral Milky Way galaxy - are seen left of center in the gorgeous Hubble Space Telescope image. The above picture spans about 8,000 light-years across NGC 1569.

2023年7月25日 · This NASA/ESA Hubble Space Telescope image reveals the iridescent interior of one of the most active galaxies in our local neighborhood — NGC 1569, a small galaxy located about eleven million light-years away in the constellation of Camelopardalis (The Giraffe).

2011年7月15日 · NGC 1569 is a dwarf irregular galaxy found in the Camelopardalis constellation. It is one of the best known starburst galaxies in the sky. It was first discovered by William Herschel on November 4, 1788. NGC 1569 has an apparent visual magnitude of 11.9 lies at a distance of 11 million light years.

NGC 1569 is a dwarf irregular galaxy in Camelopardalis. This faint galaxy is well studied by professional astronomers, who are interested in the history of star formation in the galaxy.

NGC 1569 is an irregular dwarf galaxy with a very high star birth activity, 100 times faster than observed in our own Milky Way Galaxy, and lasted almost continuous for the past 100 million years.

Classified as a starburst galaxy, NGC 1569 is smaller than the Small Magellanic Cloud that hovers near the Milky Way, but it makes up for its diminutive stature with its intense stellar productivity.