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EPL6889683
EPL6954169
EPL6889684
Peter Langer
UIG1568616
Peter Langer
UIG1568616
Peter Langer
UIG1568617
Peter Langer
UIG1568617
Peter Langer
UIG1568618
Peter Langer
UIG1568618
EPL6852416
![Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spiral galaxies at the bottom] bear the telltale marks of close interactions with each other, or perhaps with an interloper galaxy not pictured here. Their distorted shapes suggest that gravitational forces have reshaped them. The halos around the galaxies indicate that stars have been ripped away. The galaxy at bottom, center, has a 35,000 light - year - long tail of stars flowing from it. The tail may have been pulled from the galaxy about 500 million years ago. Although part of the group, the nearly edge - on spiral galaxy at top, center, remains relatively undisturbed, except for the slight warp in its disk. Most of its stars have remained within its galactic boundaries. Unlike most other galaxy interactions observed with the Hubble telescope, this group shows no evidence of the characteristic blue regions of young star clusters, which generally arise during galaxy interactions. The lack of star - forming clusters suggests that there is something different about Seyfert's Sextet compared wi](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.59686540.7055475/4565516.jpg?old-wm)
David Henley
PFH1183220
David Henley
PFH1183220
David Henley
PFH1183222
David Henley
PFH1183222
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