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]

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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.

This object is a barred spiral galaxy located 110 million light years away in the constellation of Camelopardalis at a declination of +75 degrees. The galaxy spans 6 arc-minutes in our apparent view, which corresponds to a diameter of 125,000 light years. The structure of this galaxy is beautiful and fascinating.

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 是鹿豹座的一个星系。

NGC 1530 is a barred spiral galaxy in Camelopardalis and lies at a distance of 116 million light years. It is one of the most studied galaxies by the professionals. It is a double-barred galaxy - do...

NGC 1530 is a Barred Spiral Galaxy in the Camelopardalis constellation. NGC 1530 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere.

2006年12月22日 · The barred galaxy NGC 1530 has been observed in a large number of wavebands, including spectral lines in H1, Hα and CO, giving a nearly complete velocity field across the whole nuclear and bar region.