Celestial hemisphere:  Southern  ·  Constellation: Dorado (Dor)  ·  Contains:  30 Dor Cluster  ·  NGC 1809  ·  NGC 1858  ·  NGC 1901  ·  NGC 1910  ·  NGC 1918  ·  NGC 1983  ·  NGC 2001  ·  NGC 2015  ·  NGC 2031  ·  NGC 2033  ·  NGC 2042  ·  NGC 2044  ·  NGC 2052  ·  NGC 2069  ·  NGC 2070  ·  NGC 2074  ·  NGC 2081  ·  Tarantula Nebula
Getting plate-solving status, please wait...
The Large Magellanic Cloud in HARGB, Ian Parr
The Large Magellanic Cloud in HARGB
Powered byPixInsight

The Large Magellanic Cloud in HARGB

Getting plate-solving status, please wait...
The Large Magellanic Cloud in HARGB, Ian Parr
The Large Magellanic Cloud in HARGB
Powered byPixInsight

The Large Magellanic Cloud in HARGB

Equipment

Loading...

Acquisition details

Loading...

Description

The Large Magellanic Cloud (LMC) is a spiral satellite galaxy of the Milky Way. At a distance of around 163,000 light-years, the LMC is the second or third closest galaxy to the Milky Way and is about 32,200 light-years across.  It straddles the constellations Dorado and Mensa with an apparent length of about 10 degrees to the naked eye, 20 times the Moon's diameter.
It is quite a treat visually as well as through binoculars and telescopes both large and small.

The Tarantula Nebula (NGC 2070) top left is a large HII region in the south-east corner  of Large Magellanic Cloud (LMC) and is the  most active starburst region known in the Local Group of galaxies. It is simply stunning particulary large scopes with or without filters and OIII works a treat.

Quite low for me last night but as it traversed the root top if managed just over 4 hours before the clouds kindly let me get some sleep.

Comments

Sky plot

Sky plot

Histogram

The Large Magellanic Cloud in HARGB, Ian Parr