Elephant Trunk Nebula (IC 1396)

IC 1396
IC 1396: Elephant Trunk Nebula and Garnet Star in Cepheus; SMC Pentax 67 300 mm f/4.0 ED Green Star @ f/4.0; Canon EOS Ra; 10 Micron GM 2000 QCI Ultraportable; 36x5 min @ 800 ASA; Muri b. Bern, 515 m AMSL; © 10.-11. 8. 2021 Manuel Jung [45]
IC 1396
IC 1396: Elephant Trunk Nebula; Celestron RASA 11" f/2.22; ZWO ASI6200 Pro; Tentlingen; © 2020 Peter Kocher [33]
IC 1396
IC 1396: Elephant Trunk Nebula; Astrooptik Keller Cassegrain 400mm f/3, SBIG STL-11000M; Filter L + R + G + B + SII + Hα + OIII, total 12h; Observatory Oberes Schlierental, Obwalden; © 6.-11. 10. 2010 Eduard von Bergen [30]
IC 1396
IC 1396: Elephant Trunk with globule in IC 1396; 500 mm Cassegrain f=3625 mm f/7.2; SBIG STL11K; 120+3*40 min; Bernese Highlands; © 2011 Radek Chromik [32]

History

The galactic nebula IC 1396 was discovered photographically in August 1893 by the astronomer Edward Barnard. [196] The Canadian astronomer Sidney van den Bergh discovered a reflection nebula on the photo plates of the "Palomar Sky Survey" in the elephant trunk near the star BD + 57 ° 2309 (HD 239710), which he recorded as vdB 142 in his 1966 catalog of reflection nebulae. He noted: Type I-II (star partly inside, partly outside the nebula), moderate brightness, color blue, very strong absorption, radius 0.3 '(red) to 0.6' (blue). [255]

Physical Properties

IC 1396 is a large H-II region with an angular diameter of about 3°, which is home to areas of active star formation, so-called globules. The most noticeable globule is the Elephant Trunk Nebula (also often referred to as IC 1396A). This is illuminated by the trapezoid-like, variable O-type multiple star system HD 206267 located 4.5 pc away (see Fig. 3). According to Gaia DR2 measurements, this star is 945+90-73 pc from Earth. The main structure of IC 1396A measures approximately 5.4 arcminutes (about 1.4 pc) in diameter. Behind it, more dark globules and ionized, glowing gas extend over half a degree. This structure is only a small part of the large, bubble-shaped nebula around the star cluster Trumpler 37 or Collinder 439, which typically contains many variables for a young star cluster. [360, 361]

Revised+Historic NGC/IC Version 22/9, © 2022 Dr. Wolfgang Steinicke [277]
Name RA Dec Type Dim MD Dreyer Description Identification, Remarks
IC 1396 21 38 54.0 +57 29 20 EN 170 × 140 0.800 Neb part of M. Way LBN 451/452; SG 1.19
IC 1396 A 21 35 30.0 +57 23 00 EN 14 × 2 Neb part of M. Way LBN 452
IC 1396 B 21 34 30.0 +57 28 00 EN 12 × 4 Neb part of M. Way LBN 451

Dark Nebulae

Data from Simbad [145]
Name Type RA
(J2000.0)
Dec
(J2000.0)
Rvel
[km/s]
z Size
[']
Identifiers
Barnard 160 DNe 21h 38m 12s +56° 14' 00" 31 × 31 Barnard 160; LDN 1088; TGU H585; TGU H585 P1; [DB2002b] G98.34+2.88
Barnard 161 DNe 21h 40m 24s +57° 49' 00" 4.5 0.000015 Barnard 161
Barnard 162 DNe 21h 41m 12s +56° 19' 00" Barnard 162
Barnard 163 DNe 21h 42m 15s +56° 43' 44" 4.6 0.000015 Barnard 163; LDN 1106
Barnard 365 DNe 21h 34m 54s +56° 43' 00" Barnard 365
Barnard 367 DNe 21h 44m 36s +57° 12' 00" 5 × 5 Barnard 367; LDN 1113; [DB2002b] G99.65+3.02

Finder Chart

The galactic nebula IC 1396 is located in the constellation Cepheus, which is best visible from May to December.

Finder Chart Elephant Trunk Nebula (IC 1396)
Elephant Trunk Nebula (IC 1396) in constellation Cepheus. Charts created using SkySafari 6 Pro and STScI Digitized Sky Survey. Limiting magnitudes: Constellation chart ~6.5 mag, DSS2 close-ups ~20 mag. [149, 160]

Objects Within a Radius of 10°

References