Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Cone Nebula
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Description== The diffuse Cone Nebula, so named because of its apparent shape, lies in the southern part of [[NGC 2264]], the northern part being the magnitude-3.9 [[Christmas Tree Cluster]]. It is in the northern part of [[Monoceros (constellation)|Monoceros]], just north of the midpoint of a line from [[Procyon]] to [[Betelgeuse]]. The cone's shape comes from a dark [[absorption nebula]] consisting of cold molecular hydrogen and dust in front of a faint [[emission nebula]] containing hydrogen ionized by [[S Monocerotis]], the brightest star of NGC 2264. The faint nebula is approximately seven light-years long (with an apparent length of 10 [[arcminute]]s), and is 2,700 light-years from Earth. The nebula is part of a much larger star-forming complex—the [[Hubble Space Telescope]] was used to capture images of forming stars in 1997.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)