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Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud -...

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Littl
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Largest available format 3231 × 2696 px 4 MB
Dimension [pixels] Dimension in 300dpi [mm] File size [MB] Online Purchase
Large 3231 × 2696 px 274 × 228 mm 3.5 MB
Medium 1024 × 855 px 87 × 72 mm 1.4 MB

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IMAGE number
PIX4613306
Image title
Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the right the Toucan cluster, at the top of the galaxy the NGC 362 cluster. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years, quite close enough for it to be resolved into individual stars on this colour picture made from plates taken on the UK Schmidt Telescope. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at the top of the picture is NGC 362. It is about 30,000 light years distant, twice as far away as 47 Tuc
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Image description

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Two globular clusters are visible in this image, on the right the Toucan cluster, at the top of the galaxy the NGC 362 cluster. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years, quite close enough for it to be resolved into individual stars on this colour picture made from plates taken on the UK Schmidt Telescope. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at the top of the picture is NGC 362. It is about 30,000 light years distant, twice as far away as 47 Tuc

Photo credit
Photo © Anglo-Australian Observatory/David Malin Images/Novapix / Bridgeman Images
Image keywords
astronomy / star / astronomy / galaxy / dwarf galaxy / aao / toucan / tucana / mail / star / star cluster / Novapix / star cluster / Globular cluster / astronomy / Globular cluster / South Hemisphere / southern hemisphere / small magellanic cloud / star formation / Star Training / nebula / nebula / galaxy / Irreguliere Galaxy / Irregular Galaxy / 47 Toucan / 47 tucanae / Ngc 104 / ngc 292 / ngc 362 / dwarf galaxy

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