Interstellar dust clouds and bright nebulae abound in the fertile constellation of Orion. One of the brightest, M78, is just left of center in this colorful telescopic view, covering an area north of Orion's belt. At a distance of about 1,500 light-years, the bluish nebula itself is about 5 light-years across. Its blue tint is due to dust preferentially reflecting the blue light of hot, young stars in the region. Dark dust lanes and other nebulae can easily be traced through this gorgeous skyscape. The scene also includes the remarkable McNeil's Nebula -- a newly recognized nebula associated with the formation of a sun-like star, and the telltale reddish glow of many Herbig- Haro objects, energetic jets from stars in the process of formation (text adapted from APOD). Apo TEC140 (140/f7.2) - FLI Proline 16803 - Ha (420m) L (220m) R (220m) G (150m) B (280m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
South of the large star-forming region known as the Orion Nebula, lies bright blue reflection nebula NGC 1999. The nebula is marked with a dark inverted T-shape at the lower left in a broad cosmic vista that spans over 10 light-years. The dark shape is a dense gas and dust cloud, or Bok globule, seen in silhouette against the bright nebula, and likely a site of future star formation. At the edge of the Orion molecular cloud complex some 1,500 light-years distant, NGC 1999's illumination is provided by the embedded variable star V380 Orionis. The region abounds with energetic young stars producing jets and outflows that create luminous shock waves, including HH (Herbig-Haro) 1 and 2 just below and left of NGC 1999, and the apparent cascade of reddish arcs and bow shocks beginning at the upper right. The stellar jets and outflows push through the surrounding material at speeds of hundreds of kilometers per second (text adapted from APOD). Apo TEC140 (140/f7.2) - FLI Proline 16803 - Ha (330m) L (360m) R (120m) G (120m) B (120m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
At the "feet" of the SMC, east of the nebular group know as the "magnificent seven" is this amazing area rich of HII and O3 emissions. NGC456, NGC460 and NGC465 is the array of bright emission nebulae at right in the image above. The assortment of irregular shapes appear to be cut through with dark lanes, while the individual nebulae have a large brightness range amongst them. On the middle-left of the image is visible the blue spot of (Henize) N-89, than at its left lays NGC 602 (a young, bright open cluster) and the very faint but large ring of N-90. Radiation and shock waves from the stars have pushed away much of the lighter surrounding gas and dust that compose N90, and this in turn has triggered new star formation in the ridges (or "elephant trunks") of the nebula. Apo TEC140 (140/f7.2) - FLI Proline 16803 - Ha (360m) OIII(450m) L (180m) R (120m) G (120m) B (120m) - Warrumbungle Observatory, Coonabarabran, NSW, Australia
