Explanation: M78 isn't really hiding in planet Earth's night sky. About 1,600 light-years away and nestled in the nebula rich constellation Orion, the large, bright, reflection nebula is well-known to telescopic skygazers. But this gorgeous image of M78 was selected as the winner of the Hidden Treasures 2010 astrophotography competition. Held by the European Southern Observatory (ESO), the competition challenged amateur astronomers to process data from ESO's astronomical archive in search of hidden cosmic gems. The winning entry shows off amazing details within bluish M78 (center) embraced in dark, dusty clouds, along with a smaller reflection nebula in the region, NGC 2071 (top). Yellowish and even more compact, the recently discovered, variable McNeil's Nebula is prominent in the scene below and right of center. Based on data from ESO's WFI camera and 2.2 meter telescope at La Silla, Chile, this image spans just over 0.5 degrees on the sky. That corresponds to 15 light-years at the estimated distance of M78.
How can space be so dusty and look so nice?? THAT doesn't work at my house! So whats the hidden treasures? If we can see them, they're not hidden, no matter what the name of the competition is.
Re: APOD: Hidden Treasures of M78 (2011 Jan 27)
Posted: Thu Jan 27, 2011 7:25 am
by Ann
That's a great image, very beautiful and wonderfully well-resolved.
Ann
Re: APOD: Hidden Treasures of M78 (2011 Jan 27)
Posted: Thu Jan 27, 2011 11:21 am
by Boomer12k
Looks like a painting including brush strokes. Awesome!
Re: APOD: Hidden Treasures of M78 (2011 Jan 27)
Posted: Thu Jan 27, 2011 12:07 pm
by neufer
beyond wrote:
How can space be so dusty and look so nice?? THAT doesn't work at my house!
How come the diffraction patterns around the bright stars to the left and right aren't concentric? They seem displaced along axes which radiate from the center of the shot. Is this an indicator ("coma") of really fast optics, or something else?
Re: APOD: Hidden Treasures of M78 (2011 Jan 27)
Posted: Thu Jan 27, 2011 2:01 pm
by orin stepanek
Today's APOD is a worthy background for my computer.
Hidden: Previously unrevealed information in prior attempts to process the same raw data. In this case, the stunning amount of detail in the dust and clouds indicates the person who did the image processing worked extra hard to bring it out, while still keeping the image looking fairly natural.
A beautiful result to be sure. Nice work!
And since M78 is invisible to the naked eye (even the brightest stars in the image are only about magnitude 10), one could say it's hidden from view in reality as well. Only with significant optical and/or electronic instruments can we see a view like this.
* Home Planet: "The Land Of Light," Nebula M78
* Height: 40 meters
* Weight: 35,000 tons (Earth gravitation)
* Age: 20,000 Earth years old
* Flight Speed: Mach 5
* Jump Ceiling: 800 meters
* Running Speed: 450 kilometers per hour
* Swimming Speed: 200 knots
* Physical Strength: Can lift a 100,000-ton tanker.
* Human Form: Shin Hayata (host)
* Transformation Item: Beta Capsule
* Occupations: Teacher at Space University;
Chief of Space Garrison Milky Way Office.
<<Ultraman (ウルトラマン, Urutoraman?), a character featured in tokusatsu (special effects) television programs in Japan, is the first and best-known of the "Ultra-Crusaders." The show was produced by Tokyo Broadcasting System and Tsuburaya Productions, and was broadcast on Tokyo Broadcasting System (TBS) from July 17, 1966 to April 9, 1967, with a total of 39 episodes (40, counting the pre-premiere special that aired on July 10, 1966). A major pop culture phenomenon in Japan, the show has spawned dozens of imitators as well as numerous sequels and remakes, which continued to be popular as of early January of 2011.
The series takes place in the early 1990s. Sinister aliens and giant monsters constantly threaten civilization during this period. The only Earth organization equipped to handle these disasters is the Science Special Search Party, or SSSP, a special worldwide police force equipped with high-tech weapons and vehicles, as well as extensive scientific and engineering facilities; this organization is called the Science Patrol, or the United Nations Scientific Investigation Agency. The branch of the Science Patrol that is focused on in the series is located in Tokyo, Japan. Led by Captain "Cap" Muramatsu, the Science Patrol is always ready to protect the Earth from rampaging monsters, but sometimes it finds itself outclassed. When the situation becomes desperate, Hayata, the Patrol's most capable member, holds the key to salvation in the form of the "beta capsule," which, when activated, allows him to transform secretly into the super-humanoid-powered giant from space, who becomes known to the people of Earth as Ultraman.>>
The nebula Messier 78 takes centre stage in this image taken with the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile, while the stars powering the bright display take a backseat. The brilliant starlight ricochets off dust particles in the nebula, illuminating it with scattered blue light. Igor Chekalin was the overall winner of ESO’s Hidden Treasures 2010 astrophotography competition with his image of this stunning object.
Messier 78 is a fine example of a reflection nebula. The ultraviolet radiation from the stars that illuminate it is not intense enough to ionise the gas to make it glow — its dust particles simply reflect the starlight that falls on them. Despite this, Messier 78 can easily be observed with a small telescope, being one of the brightest reflection nebulae in the sky. It lies about 1350 light-years away in the constellation of Orion (The Hunter) and can be found northeast of the easternmost star of Orion’s belt.
This new image of Messier 78 from the MPG/ESO 2.2-metre telescope at the La Silla Observatory is based on data selected by Igor Chekalin in his winning entry to the Hidden Treasures competition*.
The pale blue tint seen in the nebula in this picture is an accurate representation of its dominant colour. Blue hues are commonly seen in reflection nebulae because of the way the starlight is scattered by the tiny dust particles that they contain: the shorter wavelength of blue light is scattered more efficiently than the longer wavelength red light.
This image contains many other striking features apart from the glowing nebula. A thick band of obscuring dust stretches across the image from the upper left to the lower right, blocking the light from background stars. In the bottom right corner, many curious pink structures are also visible, which are created by jets of material being ejected from stars that have recently formed and are still buried deep in dust clouds.
Two bright stars, HD 38563A and HD 38563B, are the main powerhouses behind Messier 78. However, the nebula is home to many more stars, including a collection of about 45 low mass, young stars (less than 10 million years old) in which the cores are still too cool for hydrogen fusion to start, known as T Tauri stars. Studying T Tauri stars is important for understanding the early stages of star formation and how planetary systems are created.
Remarkably, this complex of nebulae has also changed significantly in the last ten years. In February 2004 the experienced amateur observer Jay McNeil took an image of this region with a 75 mm telescope and was surprised to see a bright nebula — the prominent fan shaped feature near the bottom of this picture — where nothing was seen on most earlier images. This object is now known as McNeil’s Nebula and it appears to be a highly variable reflection nebula around a young star.
This colour picture was created from many monochrome exposures taken through blue, yellow/green and red filters, supplemented by exposures through an H-alpha filter that shows light from glowing hydrogen gas. The total exposure times were 9, 9, 17.5 and 15.5 minutes per filter, respectively.
* Igor Chekalin from Russia uncovered the raw data for this image of Messier 78 in ESO’s archives in the competition Hidden Treasures (eso1102). He processed the raw data with great skill, claiming first prize in the contest for his final image. ESO’s team of in-house image processing experts then independently processed the raw data at full resolution to produce the image shown here.
Click to play embedded YouTube video.
Zooming into Messier 78
Credit: ESO/Igor Chekalin/S. Brunier/Chris Johnson
Music: John Dyson (from Moonwind)