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New Image Reveals Young Stars In Trapezium Cluster

Orion the Hunter, perhaps the best known constellation in the sky, is well placed in the evening at this time of the year for observers in both the northern and southern hemispheres.

For astronomers, Orion is one of the most important constellations, as it contains one of the nearest and most active stellar nurseries in the Milky Way, the galaxy in which we live.

Here tens of thousands of new stars have formed within the past ten million years or so -- a very short span of time in astronomical terms.

(For comparison, our own Sun is now 4,600 million years old and has not yet reached half-age. Reduced to a human time-scale, star formation in Orion would have been going on for just one month as compared to the Sun's 40 years.)

Just below Orion's belt, the hilt of his sword holds a great jewel in the sky, the beautiful Orion Nebula. Bright enough to be seen with the naked eye, a small telescope or even binoculars, the nebula is a few tens of light-years' wide complex of gas and dust illuminated by several massive and hot stars at its core, the famous Trapezium stars.

But the heart of this nebula also conceals a secret from the casual observer. There are in fact about one thousand very young stars about one million years old within the so-called Trapezium Cluster, crowded into a space smaller than the distance between the Sun and its nearest neighbor stars.

The cluster is very hard to observe in visible light, but is clearly seen in a new spectacular image of this area obtained by Mark McCaughrean (Astrophysical Institute, Potsdam, Germany) and his collaborators with the infrared multi-mode ISAAC instrument on the ESO Very Large Telescope (VLT) at Paranal (Chile).

That image can be seen at this European Southern Observatory URL.

Reader A.A. Schaller submitted a commentary on this story, posted on January 18 for the edition of January 19.

Dear Mr. Radler,

Your recent report on the spectacular ESO infrared image of the central region of the Orion Nebula implies that the cluster of 1000 stars imaged by infrared are within the Trapezium cluster. This is not so. For decades, radio and infrared observations have indicated non-optical sources in a region BEHIND the optically-opaque 'wall' of the nebula situated immediately to the north of the Trapezium. These observations and the most recent ones have shown that the infrared cluster has its own independent concentration of stars and confirms that this cluster is not associated with the Trapezium cluster other than through relatively close line-of-sight proximity. The new ESO images clearly show that the infrared cluster is located beyond the Trapezium region, within or behind the dust wall which renders that cluster invisible in optical wavelengths. The conclusion is that the Orion Nebula Complex is producing a 'double cluster' of stars, eventually similar in appearance to the famous double cluster NGC 869/NGC 884 in Perseus. 

Sincerely,

A. A. Schaller

18-Jan-2001

 

 

 

 

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