Click on the image for full resolution (9.3 MB)
VV 340, also known as Arp 302 or UGC 9618, provides a textbook example of colliding galaxies seen in the early stages of their interaction. The edge-on galaxy, near the top of the image, is VV 340 North and the face-on galaxy, at the bottom of the image, is VV 340 South. Millions of years later these two spirals will merge - much like the Milky Way and Andromeda will likely do billions of years from now. Data from NASA's Chandra X-ray Observatory (purple) are shown here along with optical data from the Hubble Space Telescope (red, green, blue). VV 340 is located about 450 million light years from Earth. Because it is bright in infrared light, VV 340 is classified as a Luminous Infrared Galaxy (LIRG). These observations are part of the Great Observatories All-Sky LIRG Survey (GOALS) combining data from Chandra, Hubble, NASA's Spitzer Space Telescope and Galaxy Evolution Explorer (GALEX), as well as ground-based telescopes. The survey includes over 200 LIRGs in the local universe. A chief motivation of this study is to understand why LIRGs emit so much infrared radiation. These galaxies generate energy that is tens to hundreds of times larger than that emitted by a typical galaxy. An actively growing supermassive black hole or an intense burst of star formation is often invoked as the most likely source of the energy.
The full resolution image weighs 9.3 MB, so please be patient when downloading!
X-ray: NASA/CXC/IfA/D.Sanders et al
Optical: NASA/STScI/NRAO/A.Evans et al
Image enhancement: Jean-Baptiste Faure