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The Tarantula in the Large Cloud, Brian Diettrich
The Tarantula in the Large Cloud
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The Tarantula in the Large Cloud

The Tarantula in the Large Cloud, Brian Diettrich
The Tarantula in the Large Cloud
Powered byPixInsight

The Tarantula in the Large Cloud

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Description

On November nights in New Zealand, the Large Magellanic Cloud circles the south celestial pole high in the southern sky.  Its brightest object, the Tarantula Nebula (30 Doradus), is visible with the eye as a fuzzy puff of light. A satellite galaxy, the LMC is the brightest galaxy in our skies, and on particularly dark nights it offers a rich view of many extra-galactic clusters and nebulae. The image shows the south-eastern LMC, focused around 30 Doradus but spotted with many open clusters, globular clusters, and nebulae all located within the LMC.

The wonderous Tarantula Nebula has invited many rich descriptions.  Writing from 1874, John Herschel described it as “one of the most singular and extraordinary objects which the heavens present” (Kanipe 2023:330). Stephen James O’Meara referred to it as “one of the most profound sights of the night sky”, and noted that from its centre “sprawl several crablike arms and legs, all extending in seemingly animated ways” (2002:474). Hartung wrote of “extensive clouds of luminous bluish haze contrasted with dark areas, and concentrated around a central star-like object in a series of well-defined hoops” (1995:283). The brightest object in the LMC, the Tarantula is also the largest H II region in the entire Local Group. Formerly called the Loop Nebula, the name Tarantula comes from photographs in the mid-twentieth century (Kanipe 2023:334) that showed its internal 'legs' of gas and dust.

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The Tarantula in the Large Cloud, Brian Diettrich