Eskimo Nebula (NGC 2392)
A planetary nebula in the constellation
Gemini that looks like a face
peering out of the fur-lined hood of parka. It was discovered by William
Herschel in 1787. The parka is really
a disk of material embellished with a ring of comet-shaped objects, with
their tails streaming away from the central star. The Eskimo's face is formed
from a bubble of material being blown into space by the central star's intense
wind of high-speed material. The nebula is composed of two elliptically
shaped lobes of matter streaming above and below the dying star.
Scientists believe that a ring of dense material around the star's equator,
ejected during its red giant phase, created the nebula's shape. This dense
waist of material is plodding along at 115,000 km/h, preventing high-velocity
stellar winds from pushing matter along
the equator. Instead, the 1.5-million-km/h winds are sweeping the material
above and below the star, creating the elongated bubbles. The bubbles are
not smooth like balloons but have filaments of denser matter. Each bubble
is about 1 light-year long and about half a light-year wide. One possible
explanation is that these objects formed from a collision of slow- and fast-moving
gases.
| visual magnitude |
nebula: 8.5, central star: 11 |
| angular size |
0.8' × 0.7' |
| age |
about 10,000 years |
| distance |
~3,000 light-years (920 pc) |
| position |
R.A. 07h 29m 10.8s;
Dec. 20° 55' 42.5 " |
| other designations |
Clown Face Nebula, HIP 36369,
BD+21 1609, PN G197.8+17.3 |
Related category
• NEBULAE
AND STAR CLUSTERS
Also on this site: Encyclopedia
of Alternative Energy & Sustainable Living
Encyclopedia
of History
BACK TO TOP
|