The Large Magellanic Cloud (LMC)

1.1 Stefan Westphal

The Large Magellanic Cloud (LMC) is a nearby galaxy, and a satellite of the Milky Way. At a distance of slightly less than 50 kiloparsecs (≈163,000 light-years), the LMC is the third closest galaxy to the Milky Way, with the Sagittarius Dwarf Spheroidal (~ 16 kiloparsecs) and the putative Canis Major Dwarf Galaxy (~ 12.9 kiloparsecs, though its status as a galaxy is under dispute) lying closer to the center of the Milky Way. It has a mass equivalent to approximately 10 billion times the mass of the Sun (1010 solar masses), making it roughly 1/100 as massive as the Milky Way, and a diameter of about 14,000 light-years (~ 4.3 kpc).The LMC is the fourth largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).

Imaging telescopes or lenses: Canon EF 135mm f/2.0 L
Imaging cameras: Canon EOS 600Da
Mounts: Vixen GPD2
Guiding telescopes or lenses: TS Optics 60mm Helical Sucher
Guiding cameras: M-Gen Guiding Kamera
Software: Fitswork4,  Adobe Photoshop CS 6, Deep Sky Stacker 3.3.3 Beta 51 DSS DeepSkyStacker
Accessories: Lacerta MGEN2
Resolution: 2662×1849
Dates: July 26, 2014
Frames: 16×300″ ISO800
Integration: 1.3 hours
Darks: ~3
Avg. Moon age: 28.68 days
Avg. Moon phase: 0.82%
Locations: Astrofarm Kiripotib / Namibia, Dordabis, Namibia
Author: Stefan Westphal