- Galaxies NGC 3169 and 3166 are 70 million light-years from Earth
- They’re close enough together to be warped by each other’s gravity
THE GALAXIES IN THIS COSMIC PAIRING, captured by the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile, display some curious features, demonstrating that each member of the duo is close enough to feel the distorting gravitational influence of the other.
The gravitational tug-of-war has warped the spiral shape of one galaxy, NGC 3169 (on the left), and fragmented the dust lanes in its companion, NGC 3166.
Meanwhile, a third, smaller galaxy to the lower right, NGC 3165, has a front-row seat to the gravitational twisting and pulling of its bigger neighbours.
This galactic grouping—located about 70 million light-years away in the direction of the constellation Sextans (The Sextant)—was discovered by the English astronomer William Herschel in 1783.
Modern astronomers have gauged the distance between NGC 3169 (left) and NGC 3166 (right) as a mere 50,000 light-years. That’s only about half the width of our Milky Way galaxy.
In such tight quarters, gravity can start to play havoc with galactic structure.
Spiral galaxies like NGC 3169 and NGC 3166 tend to have orderly swirls of stars and dust pinwheeling about their glowing centres. Close encounters with other big galaxies can jumble this configuration, often serving as a prelude to the merging of the galaxies into one larger galaxy.
So far, the interactions of NGC 3169 and NGC 3166 have just lent a bit of character. NGC 3169’s arms, shining bright with big, young, blue stars, have been teased apart, and lots of luminous gas has been drawn out from the main body.
In NGC 3166’s case, the dust lanes that also usually outline spiral arms are in disarray. The lack of blue colour indicates that NGC 3166 is not forming many new stars.
Spotting a supernova
NGC 3169 has another distinction—the faint yellow dot beaming through a veil of dark dust just to the left of and close to the galaxy’s centre. This flash is the leftover of a supernova detected in 2003 and known accordingly as SN 2003cg. (Note that this supernova does not still shine today—the image was taken back in 2003.)
A supernova of this variety, classified as a Type Ia, is thought to occur when a dense, hot star called a white dwarf—a remnant of medium-sized stars like our Sun—gravitationally sucks gas away from a nearby companion star.
This added fuel will eventually cause the whole star to explode in a runaway nuclear fusion reaction.
The new image presented here of a remarkable galactic dynamic duo is based on data selected by Igor Chekalin for ESO’s Hidden Treasures 2010 astrophotography competition. Chekalin won the first overall prize and this image received the second highest ranking of the nearly 100 contest entries.
Adapted from information issued by ESO / Igor Chekalin.
Get SpaceInfo.com.au daily updates by RSS or email! Click the RSS Feed link at the top right-hand corner of this page, and then save the RSS Feed page to your bookmarks. Or, enter your email address (privacy assured) and we’ll send you daily updates. Or follow us on Twitter, @spaceinfo_oz
Like this story? Please share or recommend it…