NGC 2298 is a globular cluster in the southern constellation of Puppis. Discovered by James Dunlop on May 30, 1826, it is probably a former member of the disputed Canis Major Dwarf galaxy.

NGC 2298 是在南天星座 船尾座 的一個球狀星團。 它於1826年5月30日被 詹姆士·敦洛普 發現，它之前可能是有爭議的 大犬座矮星系 的成員 [2]。

NGC 2298 是在南天星座 船尾座 的一個球狀星團。 它於1826年5月30日被 詹姆士·敦洛普 發現，它之前可能是有爭議的 大犬座矮星系 的成員 [2]。

2024年2月14日 · This new NASA Hubble Space Telescope view shows the globular cluster NGC 2298, a sparkling collection of thousands of stars held together by their mutual gravitational attraction. Globular clusters are typically home to older populations of stars, and they mostly reside in the dusty outskirts of galaxies.

2024年2月14日 · This new NASA Hubble Space Telescope view shows the globular cluster NGC 2298, a sparkling collection of thousands of stars held together by their mutual gravitational attraction. Globular clusters are typically home to older populations of stars, and they mostly reside in the dusty outskirts of galaxies.

NGC 2298 is a Globular Cluster in the Puppis constellation. NGC 2298 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 8.89, NGC 2298 is visible with the help of a binocular with a 60-70mm aperture or a small telescope.

NGC 2298 is a Globular Cluster located in the constellation of Puppis in the southern hemisphere. NGC 2298 is called NGC 2298 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to …

Discovered on May 30, 1826, by James Dunlop, NGC 2298 is a loner, some 40,000 light years from Earth. It orbits the Milky Way along a very broad, elliptical path that carries it as close as 6,500 light years from the galactic core and as far as …

2021年12月20日 · We present the far-UV (FUV) photometry of images acquired with UVIT on AstroSat to probe the horizontal branch (HB) population of the Galactic globular cluster NGC 2298.

Globular cluster NGC 2298 was discovered by James Dunlop on May 30, 1826 and cataloged as Dunlop 578. This cluster is probably a former member of the Canis Major Dwarf galaxy discovered in 2003.