Spirograph Nebula (IC 418)
History
This planetary nebula was discovered on 26 March 1891 by Williamina Fleming, a Scottish-American astronomer. She worked for Edward Pickering to whom John L. E. Dreyer mistakenly credited the discovery in his «Index Catalogue» appeared in 1895. [314]
Physical Properties
IC 418 is a planetary nebula with a high-density ellipsoidal shell, which overall morphology looks simple. A detailed view of the Hubble Space Telescope has revealed an intricate cyclic pattern that has given the «Spirograph Nebula». Magnetic fields or variable stellar wind could be responsible for these patterns. The central star has a relatively low effective temperature of 39'000 K and is in an early evolutionary stage. The distance is measured to 1.3 ± 0.4 kpc. [541]
| Designations | PN G215.2-24.2: IC 418, PK 215-24.1, ARO 3, VV 22, VV' 32 |
| Right Ascension (J2000.0) | 05h 27m 28s |
| Declination (J2000.0) | -12° 41' 48" |
| Dimensions | 12." (optical) |
| Distance | 0.88 kpc |
| Radial Velocity | +61.0 km/s ± 2.0 km/s |
| Expansion Velocity | < 6.0 km/s (O-III), 12. km/s (N-II) |
| C-Star Designations | AG82 43, BD -12 1172, EM* CDS 500, GCRV 3288, HD 35914, PLX 1239, TD1 4662 |
| C-Star Magnitude | 10.00 mag (B filter), 10.17 mag (V filter) |
| C-Star Spectral Type | Of(H) |
| Discoverer | FLEMING 1891 |
Finder Chart
The 10 mag star ZZ Leporis with the planetary nebula IC 418 is located near the ears of the Hare (Lepus), south of Orion. Together with three other stars of about 7 mag it forms a conspicuous figure that can be seen in an eyepiece which gives approximately 1° true field of view. The best time to observe it is November to January.
Visual Observation
Description pending ...