Explanation: Many spiral galaxies have bars across their centers. Even our own Milky Way Galaxy is thought to have a bar, but perhaps not so prominent as the one in NGC 1365, shown above. The persistence and motion of the bar imply relatively massive spiral arms. The placements of bright young blue stars and dark dust lanes also indicate a strong rotating density wave of star formation. NGC 1365 is a member of the Fornax Cluster of Galaxies. Because NGC 1365 is relatively nearby, simultaneous measurements of its speed and distance are possible, which help astronomers estimate how fast our universe is expanding.

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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: NGC 1365 - barred spiral galaxy - galaktika, spiral'naya - spiral'naya galaktika s peremychkoi Publikacii so slovami: NGC 1365 - barred spiral galaxy - galaktika, spiral'naya - spiral'naya galaktika s peremychkoi
Sm. takzhe: Spiral'naya galaktika s peremychkoi NGC 1365 ot teleskopa "Dzheims Vebb" NGC 1365: velichestvennaya ostrovnaya vselennaya Skoplenie galaktik v Pechi M64: galaktika Podbityi Glaz M94: galaktika s dvoinym kol'com NGC 2442: galaktika v Letuchei Rybe Spiral'naya galaktika s peremychkoi NGC 1300 Vse publikacii na tu zhe temu >>