An elegant galaxy in an unusual light
NGC 1365 in infrared light helps astronomers understand the complex flow of material within the galaxy and how it affects the reservoirs of gas from which new stars can form.
September 23, 2010
Provided by ESO, Garching, Germany
September 23, 2010
HAWK-I infrared image of the spectacular barred spiral galaxy NGC 1365.
Photo by ESO
A new image taken with the powerful HAWK-I camera on the European Southern Observatory's (ESO) Very Large Telescope at Paranal Observatory in Chile shows the beautiful barred spiral galaxy NGC 1365 in infrared light. NGC 1365 is a member of the Fornax cluster of galaxies and lies about 60 million light-years from Earth.
NGC 1365 is one of the best-known and most studied barred spiral galaxies and is sometimes nicknamed the Great Barred Spiral Galaxy because of its strikingly perfect form, with the straight bar and two prominent outer spiral arms. Closer to the center there is also a second spiral structure, and the whole galaxy is laced with delicate dust lanes.
This galaxy is an excellent laboratory for astronomers to study how spiral galaxies form and evolve. The new infrared images from HAWK-I are less affected by the dust that obscures parts of the galaxy than images in visible light, and they clearly reveal the glow from vast numbers of stars in both the bar and the spiral arms. The data were acquired to help astronomers understand the complex flow of material within the galaxy and how it affects the reservoirs of gas from which new stars can form. The huge bar disturbs the shape of the gravitational field of the galaxy, and this leads to regions where gas is compressed and star formation is triggered. Many huge, young star clusters trace out the main spiral arms, and each contains hundreds or thousands of bright young stars that are less than 10 million years old. The galaxy is too remote for single stars to be seen in this image, and most of the tiny clumps visible in the picture are really star clusters. Over the whole galaxy, stars are forming at a rate of about 3 times the mass of our Sun per year.
While the bar of the galaxy consists mainly of older stars long past their prime, many new stars are born in stellar nurseries of gas and dust in the inner spiral close to the nucleus. The bar also funnels gas and dust gravitationally into the center of the galaxy where astronomers have found evidence for the presence of a supermassive black hole, well hidden among myriad intensely bright new stars.
NGC 1365, including its two huge outer spiral arms, spreads around 200,000 light-years. Different parts of the galaxy take different times to make a full rotation around the core of the galaxy, with the outer parts of the bar completing one circuit in about 350 million years. NGC 1365 and other galaxies of its type have come to more prominence in recent years with new observations, indicating that the Milky Way could also be a barred spiral galaxy. Such galaxies are quite common — two thirds of spiral galaxies are barred according to recent estimates — and studying others can help astronomers understand our own galactic home.