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Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo...

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is
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Largest available format 2631 × 2118 px 1 MB
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Large 2631 × 2118 px 223 × 179 mm 1.1 MB
Medium 1024 × 825 px 87 × 70 mm 1.3 MB

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IMAGE number
PIX4612972
Image title
Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 25 million years away - light from Earth. This galaxy interacts with a dwarf galaxy. Image obtained with a telescope of 35 cm, 12 hours of poses. NGC 6744 is a majestic spiral galaxy in the southern constellation of Pavo. It has great similarities to the Milky Way galaxy in both form and structure. It lies at a distance of approximately 25 million Light Years. At its northern tip NGC 6744 is interacting with a dwarf companion galaxy much in the same way the Milky Way interacts with the Large Magellanic Cloud. The northernmost spiral arm is most likely being stretched and its stars and gas stripped due to tidal pull from the dwarf companion. Likewise the stars of the companion will likely be engulfed and the companion will ultimately merge with NGC 6744 at a far off future time. Image taken with 14.5”” RCOS telescope, 12 Hours of exposure
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Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 25 million years away - light from Earth. This galaxy interacts with a dwarf galaxy. Image obtained with a telescope of 35 cm, 12 hours of poses. NGC 6744 is a majestic spiral galaxy in the southern constellation of Pavo. It has great similarities to the Milky Way galaxy in both form and structure. It lies at a distance of approximately 25 million Light Years. At its northern tip NGC 6744 is interacting with a dwarf companion galaxy much in the same way the Milky Way interacts with the Large Magellanic Cloud. The northernmost spiral arm is most likely being stretched and its stars and gas stripped due to tidal pull from the dwarf companion. Likewise the stars of the companion will likely be engulfed and the companion will ultimately merge with NGC 6744 at a far off future time. Image taken with 14.5”” RCOS telescope, 12 Hours of exposure

Photo credit
© R.Gendler/Novapix / Bridgeman Images
Image keywords
astronomy / 2008 / star / interaction / astronomy / galaxy / spiral galaxy / peacock / pavo / star / Novapix / astronomy / South Hemisphere / southern hemisphere / star formation / Star Training / Galaxy Spiral / interacting / NGC 6744 / NGC 6744

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