NGC 1530 is a barred spiral galaxy in the northern constellation of Camelopardalis. It was discovered by German astronomer W. Tempel in 1876. [7] Danish astronomer J. L. E. Dreyer in 1888 described it only as large and pretty bright. [8] NGC 1530 has an apparent visual magnitude of 12.3 [5] and an angular size of 4.6′ × 2.4′. [5]

ngc 1530 是鹿豹座的一個星系。 维基共享资源上的相關多媒體資源：ngc 1530. ned – ngc 1530; seds – ngc 1530; simbad – ngc 1530; vizier – ngc 1530

NGC 1530 is a barred spiral galaxy located approximately of 65 million light years distant. It is receding from the Milky Way with a velocity of 2,622 km/s.

NGC 1530, a barred spiral galaxy situated in the constellation Camelopardalis, captivates astronomers with its distinctive structure. The prominent bar running through its central region is accompanied by tightly wound spiral arms, hosting regions of active star formation.

NGC 1530, a barred spiral galaxy situated in the constellation Camelopardalis, captivates astronomers with its distinctive structure. The prominent bar running through its central region is accompanied by tightly wound spiral arms, hosting regions of active star formation.

2025年2月12日 · NGC 1530: The Hurricane Galaxy Celestial hemisphere: Northern · Constellation: Camelopardalis (Cam) · Contains: NGC 1530

ngc 1530 是鹿豹座的一个星系。 维基共享资源上的相关多媒体资源：ngc 1530. ned – ngc 1530; seds – ngc 1530; simbad – ngc 1530; vizier – ngc 1530

NGC 1530 is a mag 12 galaxy, classified as an SBb type barred spiral in Camelopardis. Based on CO emission analysis it has also been termed a nuclear ring galaxy. Despite being faint with respect to apparent magnitude, it is notable for being one of the largest barred spirals in the northern hemisphere with one of the strongest bars known.

NGC 1530 is a very strongly barred galaxy (Font et al. 2014). Something more it is double-barred galaxy. Double-barred galaxies account for almost one third of all barred galaxies, suggesting that secondary stellar bars, which are embedded in large-scale primary bars, are long-lived structures (Wozniak H., 2014).

NGC 1530, a barred spiral galaxy situated in the constellation Camelopardalis, captivates astronomers with its distinctive structure. The prominent bar running through its central region is accompanied by tightly wound spiral arms, hosting regions of active star formation.