Tag: LMC

Large Magellanic Cloud (LMC), Small Magellanic Cloud (SMC), and the dust around

The Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) are two irregular dwarf galaxies that orbit the Milky Way. They are among the closest galaxies to us and are visible from the Southern Hemisphere.

  • Large Magellanic Cloud (LMC): Located about 160,000 light-years away, the LMC is the fourth-largest galaxy in the Local Group. It contains the Tarantula Nebula, one of the most active star-forming regions in the nearby universe.
  • Small Magellanic Cloud (SMC): Positioned around 200,000 light-years from Earth, the SMC is smaller and more irregular than the LMC. It has a rich mix of young and old stars and is known for its interaction with both the LMC and the Milky Way, causing bursts of star formation.

Both galaxies are important for studying cosmic evolution and are key targets for astronomers exploring star formation and galactic interactions.

TelescopeSigma 40mm @F1.4
Aperture28 mm
Focal length40 mm
MountiOptron HEM15
AutoguidingZWO ASI485MC, QHY Mini Guide Scope
CameraZWO 6200MC @0°C
Filtersnone
Exposure84x180s, Gain 100, bin 1×1,
Date2024-10-02

NGC 2060 Tarantula Nebula

Our galaxy Milky Way is surrounded by two dwarf galaxies. Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC). SMC I captured recently by the relatively short focal length of 250 mm. LMC is much larger, so it wouldn’t fit into the field of view of my 94 mm refractor. However, LMC is full of very interesting objects, just like the Tarantula Nebula. I used the HaLRGB technique to make the nebulosity pop.

TelescopeSharpstar 94EDPH
Aperture94 mm
Focal length414 mm
MountRainbow Astro RST 135
AutoguidingZWO 174MM, QHY Mini Guide Scope
CameraZWO 2600MM @-10°C
CorrectorF4.4 Quad Reducer
FiltersAntlia HaLRGB
Exposure16x180s HaL, 10x180s RGB, Gain 100, bin 1x1,
Date2022-05-31