Explanation: A smaller companion seems wrapped in the spiral arms of enigmatic galaxy NGC 1097. This amazingly deep image of the peculiar spiral system, also known as Arp 77, actually combines data from two telescopes, one in the northern and one in the southern hemisphere of planet Earth. The faint details revealed include hints of a mysterious jet emerging toward the top of the view. Seen to be about 42,000 light-years from the larger galaxy's center, the companion galaxy is gravitationally interacting with the spiral and will ultimately merge with it. NGC 1097's center also harbors a massive black hole. NGC 1097 is located about 45 million light-years away in the chemical constellation Fornax.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Seyfert galaxy - active galaxy - spiral arms - aktivnaya galaktika - Seifertovskaya galaktika - Spiral'nye vetvi galaktik Publikacii so slovami: Seyfert galaxy - active galaxy - spiral arms - aktivnaya galaktika - Seifertovskaya galaktika - Spiral'nye vetvi galaktik
Sm. takzhe: Velikolepnaya spiral'naya galaktika NGC 5643 Obolochki i dzhety galaktiki Centavr A M106: spiral'naya galaktika so strannym yadrom Tri galaktiki v Drakone Aktivnaya galaktika NGC 1275 V rukavah NGC 1097 Centavr A Vse publikacii na tu zhe temu >>