What Happens When Galaxies Collide?
6:05
SPACE.comPaul Sutter
What Happens When Galaxies Collide?
Two galaxies, drawn together by forces that they can't see but they can feel. A mutual gravitational attraction. It's inevitable: Inch by inch, light-year by light-year, as the cosmic clock ticks on through the eons, the galaxies grow closer.
May 25, 2017
Interacting galaxy Formation
Panning across Interacting Galaxy System Arp-Madore 2105-332 | Hubble FriendsofNASA.org: This image features an interacting galaxy system known as Arp-Madore 2105-332, that lies about 200 million light-years from Earth in the constellation Microscopium. This system belongs to the Arp-Madore catalogue of peculiar galaxies. The wonderful quality of this image also reveals several further galaxies, not associated with this system but fortuitously positioned in such a way that they appear to be form
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Panning across Interacting Galaxy System Arp-Madore 2105-332 | Hubble FriendsofNASA.org: This image features an interacting galaxy system known as Arp-Madore 2105-332, that lies about 200 million light-years from Earth in the constellation Microscopium. This system belongs to the Arp-Madore catalogue of peculiar galaxies. The wonderful quality of this image also reveals several further galaxies, not associated with this system but fortuitously positioned in such a way that they appear to be form
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M51 – INTERACTING GALACTIC STRUCTURE M51, the Whirlpool Galaxy, is a grand-design spiral undergoing a close gravitational encounter with its companion NGC 5195. This interaction pulls out long tidal streams, compresses gas in the spiral arms, and ignites bursts of star formation that trace the galaxy’s sweeping blue structure. The distorted dust lanes and extended tidal debris record multiple past passages of the companion, each reshaping M51’s disk and amplifying its spiral density waves. The s
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M51 – INTERACTING GALACTIC STRUCTURE M51, the Whirlpool Galaxy, is a grand-design spiral undergoing a close gravitational encounter with its companion NGC 5195. This interaction pulls out long tidal streams, compresses gas in the spiral arms, and ignites bursts of star formation that trace the galaxy’s sweeping blue structure. The distorted dust lanes and extended tidal debris record multiple past passages of the companion, each reshaping M51’s disk and amplifying its spiral density waves. The s
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Galaxy Details and Mergers - NASA Science
Galaxy Details and Mergers - NASA Science
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