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NGC 3293 (Gem Cluster)


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NGC 3293
Open Cluster (散開星団)
Gem Cluster (宝石星団)
OC I3r


別名 (Other names)
OCL 816, ESO 128-SC5

明るさ (Brightness)
4.7等級

距離 (Distance)
8,000光年 (8,000 light-years)

星座 (Constellation)
りゅうこつ座 (Car) (Carina)

NGC 3293 (Gem Cluster) is an open cluster located 8,000 light years from the Earth in the constellation Carina.

NGC 3293 (Gem Cluster) : Picture

NGC 3293 (Gem Cluster)
NGC 3293 (Gem Cluster)
(C) ESO
This beautiful star cluster, NGC 3293, is found 8,000 light-years from Earth in the constellation of Carina. This cluster was first spotted by the French astronomer Nicolas-Louis de Lacaille in 1751, during his stay in what is now South Africa, using a tiny telescope with an aperture of just 12 millimetres. It is one of the brightest clusters in the southern sky and can be easily seen with the naked eye on a dark clear night.

Star clusters like NGC 3293 contain stars that all formed at the same time, at the same distance from Earth and out of the same cloud of gas and dust, giving them the same chemical composition. As a result clusters like this are ideal objects for testing stellar evolution theory.

Most of the stars seen here are very young, and the cluster itself is less than 10 million years old. Just babies on cosmic scales if you consider that the Sun is 4.6 billion years old and still only middle-aged. An abundance of these bright, blue, youthful stars is common in open clusters like NGC 3293, and, for example, in the better known Kappa Crucis cluster, otherwise known as the Jewel Box or NGC 4755.

These open clusters each formed from a giant cloud of molecular gas and their stars are held together by their mutual gravitational attraction. But these forces are not enough to hold a cluster together against close encounters with other clusters and clouds of gas as the cluster’s own gas and dust dissipates. So, open clusters will only last a few hundred million years, unlike their big cousins, the globular clusters, which can survive for billions of years, and hold on to far more stars.

Despite some evidence suggesting that there is still some ongoing star formation in NGC 3293, it is thought that most, if not all, of the nearly fifty stars in this cluster were born in one single event. But even though these stars are all the same age, they do not all have the dazzling appearance of a star in its infancy; some of them look positively elderly, giving astronomers the chance to explore how and why stars evolve at different speeds.

Take the bright orange star at the bottom right of the cluster. This huge star, a red giant, would have been born as one of the biggest and most luminous of its litter, but bright stars burn out fast. As the star used up the fuel at its core its internal dynamics changed and it began to swell and cool, becoming the red giant we now observe. Red giants are reaching the end of their life cycle, but this red giant’s sister stars are still in what is known as the pre-main-sequence — the period before the long, stable, middle period in a star’s life. We see these stars in the prime of their life as hot, bright and white against the red and dusty background.

This image was taken with the Wide Field Imager (WFI) installed on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in northern Chile.

NGC 3293 (Gem Cluster)
NGC 3293 (Gem Cluster)
(C) Andre.lucas.melo

NGC 3293
The star cluster NGC 3293 in the constellation of Carina
(C) ESO, IAU and Sky & Telescope
This chart shows the location of the bright open star cluster NGC 3293 in the southern constellation of Carina. All the stars visible to the naked eye on a clear and dark night are marked, along with the positions of some nebulae and clusters. The location of NGC 3293 is marked with a red circle. This cluster is bright enough to be seen without optical aid in good conditions and is a spectacular sight in a moderate-sized telescope.

NGC 3293
NGC 3293: A Bright Young Open Cluster
(C) David Malin (AAO), AATB

NGC 3293 (Gem Cluster) NGC 3293 (Gem Cluster)
NGC 3293 (Gem Cluster)
(C) ESO
NGC 3293 (Gem Cluster)
(C) Andre.lucas.melo
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NGC 3293 (Gem Cluster) : Movie

Zooming in on the bright star cluster NGC 3293
This zoom video starts from a broad view of the Milky Way and takes the viewer on a journey to the bright star cluster NGC 3293 in the constellation of Carina. This spectacular object would have been just a cloud of gas and dust about ten million years ago, but as stars began to form it became the bright group we see here. Clusters like this are celestial laboratories that allow astronomers to learn more about how stars evolve.

A close-up look at the star cluster NGC 3293
This pan video gives a close-up view of a colourful image from the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. It shows a group of young stars huddled together against a backdrop of clouds of glowing gas and lanes of dust. This star cluster, known as NGC 3293, would have been just a cloud of gas and dust itself about ten million years ago, but as stars began to form it became the bright group we see here. Clusters like this are celestial laboratories that allow astronomers to learn more about how stars evolve.
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