NGC 3717: 거의 옆으로 누워있는 나선 은하 (NGC 3717: A Nearly Sideways Spiral Galaxy)
어떤 나선 은하들은 옆으로 누워있다. 나선 은하에 있는 대부분의 밝은 별들은 원반의 중심 근처에 휘감겨 있고, 옆에서 보면
Explanation: Some spiral galaxies are seen nearly sideways. Most bright stars in spiral galaxies swirl around the center in a disk, and seen from the side, this disk can be appear quite thin. Some spiral galaxies appear even thinner than NGC 3717, which is actually seen tilted just a bit. Spiral galaxies form disks because the original gas collided with itself and cooled as it fell inward. Planets may orbit in disks for similar reasons. The featured image by the Hubble Space Telescope shows a light-colored central bulge composed of older stars beyond filaments of orbiting dark brown dust. NGC 3717 spans about 100,000 light years and lies about 60 million light years away toward the constellation of the Water Snake (Hydra).
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Phillip Newman Specific rights apply.
A Service of: ASD at NASA / GSFC & Michigan Tech. U.
Translated by: WouldYouLike