IC 1396
Nebula in the constellation Cepheus
title: "IC 1396" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["dark-nebulae", "star-forming-regions", "cepheus-(constellation)", "ic-objects"] description: "Nebula in the constellation Cepheus" topic_path: "general/dark-nebulae" source: "https://en.wikipedia.org/wiki/IC_1396" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary Nebula in the constellation Cepheus ::
::data[format=table title="Infobox nebula"]
| Field | Value |
|---|---|
| name | IC 1396 |
| image | File:Elephant's Trunk nebula.jpg |
| type | emission |
| type2 | |
| epoch | |
| ra | |
| dec | |
| dist_ly | 2,400 |
| appdia | |
| constellation | Cepheus |
| :: |
NOTOC |name = IC 1396 |image = File:Elephant's Trunk nebula.jpg |caption = |credit = |type = emission |type2 = |epoch = |subtype = |class = |ra = |dec = |dist_ly = 2,400 |dist_pc = |dist_z = |appmag_v = |appdia = |size_v = |constellation = Cepheus |radius_ly = |radius_pc = |dimensions = |absmag_v = |notes = |names =
IC 1396 is a large emission nebulae, a region of ionized gas, located in the constellation Cepheus about 2,400 light years away from Earth.
IC 1396 is illuminated and ionized by a very bright, massive multiple star HD 206267 at its center, except for dense globules that can protect themselves from the star's harsh ultraviolet rays. This hierarchical triple star system has two members that form a spectroscopic binary that orbit each other with a period of 3.7 days, while a third member lies further away—it is unclear whether this third member is gravitationally bound to the pair. The system is emitting a stellar wind that reaches an exceptional velocity of 3,225 km/s, among the highest measured for stars of this type.{{citation | display-authors=1 | last1=Wojdowski | first1=P. S. | last2=Schulz | first2=N. S. | last3=Ishibashi | first3=K. | last4=Huenemoerder | first4=D. P. | title=The Hot Star Triplet HD 206267A | journal=High Resolution X-ray Spectroscopy with XMM-Newton and Chandra, Proceedings of the International Workshop Held at the Mullard Space Science Laboratory of University College London, Holmbury St Mary, Dorking, Surrey, UK, October 24–25, 2002 | date=December 2002 | page=49 | bibcode=2002hrxs.confE..49W
Jutting from the rim of the nebula is IC 1396A, commonly called the Elephant's Trunk Nebula, a dark, dense globule with a bright, sinuous rim being illuminated by HD 206267.
The red supergiant Mu Cephei is located at the edge of the nebula. It is well known for being one of the largest known stars.
References
Sources
References
- Matthews, HI. (1979). "High resolution radio observations of bright rims in IC 1396". Astronomy and Astrophysics.
- (2012). "The Elephant Trunk Nebula and the Trumpler 37 cluster: Contribution of triggered star formation to the total population of an H II region". Monthly Notices of the Royal Astronomical Society.
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