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Tour of NGC 602
Quicktime MPEG With closed-captions (at YouTube)
The Small Magellanic Cloud — also known as the SMC — is one of the closest galaxies to the Milky Way. Because the SMC is so close and bright, it offers a chance to study phenomena that are difficult to examine in more distant galaxies. Chandra has been used to make the first detection of X-ray emission from young, low-mass stars outside our Milky Way galaxy. By "low-mass" we mean with masses similar to our Sun. The Chandra observations of these low-mass stars were made of the region known as the "Wing" of the SMC. In this composite image of the Wing the Chandra data is shown in purple, optical data from the Hubble Space Telescope is shown in red, green and blue and infrared data from the Spitzer Space Telescope is shown in red. The Wing differs from most areas in the Milky Way by having relatively few metals, that is elements heavier than hydrogen and helium. The Chandra results imply that the young, metal-poor stars in NGC 602a make X-rays just like stars with much higher metal content in our galaxy make X-rays.
[Runtime: 01:22]
Quicktime MPEG With closed-captions (at YouTube)
The Small Magellanic Cloud — also known as the SMC — is one of the closest galaxies to the Milky Way. Because the SMC is so close and bright, it offers a chance to study phenomena that are difficult to examine in more distant galaxies. Chandra has been used to make the first detection of X-ray emission from young, low-mass stars outside our Milky Way galaxy. By "low-mass" we mean with masses similar to our Sun. The Chandra observations of these low-mass stars were made of the region known as the "Wing" of the SMC. In this composite image of the Wing the Chandra data is shown in purple, optical data from the Hubble Space Telescope is shown in red, green and blue and infrared data from the Spitzer Space Telescope is shown in red. The Wing differs from most areas in the Milky Way by having relatively few metals, that is elements heavier than hydrogen and helium. The Chandra results imply that the young, metal-poor stars in NGC 602a make X-rays just like stars with much higher metal content in our galaxy make X-rays.
[Runtime: 01:22]
(Credit: NASA/CXC/A. Hobart)
The Galactic Empire
Quicktime MPEG With closed-captions (at YouTube)
Our galaxy, the Milky Way, is more than just a giant barred spiral containing hundreds of billions of stars. It's also the centre of a colossal empire and rules over about 20 smaller galaxies that orbit around it, similar to the way our Moon orbits the Earth. The shining stars and glowing arcs of gas in this picture reside in one of these subjects: a dwarf galaxy called the Small Magellanic Cloud.
If you live in the Southern Hemisphere or near the equator, you may have noticed two bright but blurry clouds in the dark night sky. The smaller of these clouds is the Small Magellanic Cloud, one of the Milky Way's so-called 'satellite galaxies'. It is a dwarf galaxy, meaning that it contains far fewer stars than galaxies similar to our own. While the Milky Way is made up of about 300 billion stars, the Small Magellanic Cloud has just a couple of billion.
On a cosmic scale, this galaxy is extremely close by. Moving at the fastest speed known in the Universe (the speed of light), it would take less than 200 thousand years to travel there from Earth.
Being so close to us, the Small Magellanic Cloud offers astronomers an opportunity to study phenomena that are difficult to examine in more distant galaxies. This picture shows an area of the galaxy called the 'Wing'. It contains three star clusters that astronomers have been studying recently to find out how young stars are born.
[Runtime: 02:00]
Quicktime MPEG With closed-captions (at YouTube)
Our galaxy, the Milky Way, is more than just a giant barred spiral containing hundreds of billions of stars. It's also the centre of a colossal empire and rules over about 20 smaller galaxies that orbit around it, similar to the way our Moon orbits the Earth. The shining stars and glowing arcs of gas in this picture reside in one of these subjects: a dwarf galaxy called the Small Magellanic Cloud.
If you live in the Southern Hemisphere or near the equator, you may have noticed two bright but blurry clouds in the dark night sky. The smaller of these clouds is the Small Magellanic Cloud, one of the Milky Way's so-called 'satellite galaxies'. It is a dwarf galaxy, meaning that it contains far fewer stars than galaxies similar to our own. While the Milky Way is made up of about 300 billion stars, the Small Magellanic Cloud has just a couple of billion.
On a cosmic scale, this galaxy is extremely close by. Moving at the fastest speed known in the Universe (the speed of light), it would take less than 200 thousand years to travel there from Earth.
Being so close to us, the Small Magellanic Cloud offers astronomers an opportunity to study phenomena that are difficult to examine in more distant galaxies. This picture shows an area of the galaxy called the 'Wing'. It contains three star clusters that astronomers have been studying recently to find out how young stars are born.
[Runtime: 02:00]
(Credit: NASA/CXC/April Jubett)
Return to NGC 602 (April 3, 2013)
Revised: July 10, 2023