M 100

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Wikipedia Description:

Messier 100 (also known as NGC 4321 or the Mirror Galaxy) is a grand design intermediate spiral galaxy in the southern part of the mildly northern Coma Berenices.[5] It is one of the brightest and largest galaxies in the Virgo Cluster and is approximately 55 million light-years[3] from our galaxy, about 166,000 light-years in diameter. It was discovered by Pierre Méchain in 1781[a] and 29 days later seen again and entered by Charles Messier in his catalogue “of nebulae and star clusters”.[6][7] It was one of the first spiral galaxies to be discovered,[7] and was listed as one of fourteen spiral nebulae by Lord William Parsons of Rosse in 1850. NGC 4323 and NGC 4328 are satellite galaxies of M100; the former is connected with it by a bridge of luminous matter.[8][9]

Wikipedia: M100

Acquisition Details:

TelescopeTakahashi TOA-130
OpticsTakahashi TOA-645 Flattener
FilterNone
CameraASI2600MC Pro OSC
Integration Time6.25 Hours
Subframes125 x 180 Seconds
DateMarch 8, 2025
LocationCarlsbad, California