Posted on 06/19/2002 9:24:16 PM PDT by petuniasevan
Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
Explanation: Big and beautiful spiral galaxy M81, in the northern constellation Ursa Major, is one of the brightest galaxies visible in the skies of planet Earth. This superbly detailed view reveals its bright nucleus, grand spiral arms and sweeping cosmic dust lanes with a scale comparable to the Milky Way. Hinting at a disorderly past, a remarkable dust lane runs straight through the disk, below and right of the galactic center, contrary to M81's other prominent spiral features. The errant dust lane may be the lingering result of a close encounter between M81 and its smaller companion galaxy, M82. Scrutiny of variable stars in M81 (aka NGC 3031) has yielded one of the best determined distances for an external galaxy -- 11.8 million light-years.
120 minute b/w detail scan.
10 minute red filter scan.
10 minute green filter scan.
20 minute blue filter scan.
By a technique known as "luminance layering" the photographer combined the images using Photoshop.
This gives the image detail, depth, and authentic hues.
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Winking star surrounded by embryonic solar system
Astronomers have found a young star with a dust cloud around it which may one day form a solar system like our own.
The cloud eclipses the star making it wink. It's the first time scientists have had a chance to study a structure like it.
It may help them understand how our own star and planet evolved.
Their view is so good they can see annual and even monthly changes.
The structure is thought to be just three million years old and 2,400 light years from the Earth.
Scientists led by William Herbst and Catrina Hamilton, of Wesleyan University in Connecticut, carried out the study into KH 15D.
The star is in the constellation of Monoceros and inhabits a nebulous region of space close to the famous Cone Nebula.
Observations made in the late 1990s tipped them off that this structure was different to others. Herbst said: "Basically, the star winked at us."
That is because it fades out every 48.3 days and stays faint for about 18 days. Material orbiting the star blocks its light out on this regular basis.
There are many examples of eclipsing binary stars but the length of the eclipse is unique in the case of KH 15D because only a collection of smaller objects surrounding the star can explain it.
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