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Sharpless 63 This is the high latitude molecular cloud MBM 159, which is located at a distance of about 220 pc and may form part of the Aquila rift.Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge Apo TEC140 (140/f7.2) - FLI Proline 16803 - L (450m) R (90m) G (90m) B (150m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
Sharpless 2-1 and Vdb 99 Wisps of dust fill the space between the stars. This dust is usually invisible, subtly acting to dim the light of more distant stars. Sometimes this dust is thick and prominent as dark patches on otherwise bright emission nebulae. Other times this dust may show itself by reflecting the light of bright, nearby stars. Because bright stars tend to be blue, and because dust reflects blue light more easily than red, the resulting reflection nebula usually appears blue. Pictured above is the reflection nebula Sharpless 2-1 in the constellation of Scorpius (text adapted from APOD). This is a mosaic of 2 panels.Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge Apo TEC140 (140/f7.2) - FLI Proline 16803 - Ha (300m) L (250m) R (140m) G (110m) B (120m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
Sharpless 63

This is the high latitude molecular cloud MBM 159, which is located at a distance of about 220 pc and may form part of the Aquila rift.

Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge

Apo TEC140 (140/f7.2) - FLI Proline 16803 - L (450m) R (90m) G (90m) B (150m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
Sharpless 63

This is the high latitude molecular cloud MBM 159, which is located at a distance of about 220 pc and may form part of the Aquila rift.

Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge

Apo TEC140 (140/f7.2) - FLI Proline 16803 - L (450m) R (90m) G (90m) B (150m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia" href="javascript:openLB(2221993788,'',XLarge,'',768,768);"> Sharpless 63 This is the high latitude molecular cloud MBM 159, which is located at a distance of about 220 pc and may form part of the Aquila rift.Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge Apo TEC140 (140/f7.2) - FLI Proline 16803 - L (450m) R (90m) G (90m) B (150m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
Sharpless 63

This is the high latitude molecular cloud MBM 159, which is located at a distance of about 220 pc and may form part of the Aquila rift.

Mouse over the image to display all resolutions available. Click "share" button on top to get direct links to download the images up to XXXL size. Click "buy" button to purchase high quality prints of this imge

Apo TEC140 (140/f7.2) - FLI Proline 16803 - L (450m) R (90m) G (90m) B (150m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
See photo in original gallery.
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