Cone Nebula (NGC 2264): Star-Forming Pillar of Gas and Dust

Stsci_2002-11b_1024

stsci_2002-11b April 30th, 2002

Credit: NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA

Resembling a nightmarish beast rearing its head from a crimson sea, this monstrous object is actually an innocuous pillar of gas and dust. Called the Cone Nebula (NGC 2264) - so named because, in ground-based images, it has a conical shape - this giant pillar resides in a turbulent star-forming region. This picture, taken by the newly installed Advanced Camera for Surveys (ACS) aboard NASA's Hubble Space Telescope, shows the upper 2.5 light-years of the nebula, a height that equals 23 million roundtrips to the Moon. The entire nebula is 7 light-years long. The Cone Nebula resides 2,500 light-years away in the constellation Monoceros. Radiation from hot, young stars [located beyond the top of the image] has slowly eroded the nebula over millions of years. Ultraviolet light heats the edges of the dark cloud, releasing gas into the relatively empty region of surrounding space. There, additional ultraviolet radiation causes the hydrogen gas to glow, which produces the red halo of light seen around the pillar. A similar process occurs on a much smaller scale to gas surrounding a single star, forming the bow-shaped arc seen near the upper left side of the Cone. This arc, seen previously with the Hubble telescope, is 65 times larger than the diameter of our solar system. The blue-white light from surrounding stars is reflected by dust. Background stars can be seen peeking through the evaporating tendrils of gas, while the turbulent base is pockmarked with stars reddened by dust. Over time, only the densest regions of the Cone will be left. Inside these regions, stars and planets may form. The Cone Nebula is a cousin of the M16 pillars, which the Hubble telescope imaged in 1995. Monstrous pillars of cold gas, like the Cone and M16, are common in large regions of star birth. Astronomers believe that these pillars are incubators for developing stars. ACS made this observation on April 2, 2002. The color image is constructed from three separate images taken in blue, ne

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2002/news-2002-11

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

Image Details Image Details

Image Type
Observation
Object Name
Cone Nebula NGC 2264
Subject - Milky Way
Nebula > Appearance > Emission

Distance Details Distance

Universescale1
2,500 light years
Stsci_2002-11b_128
 

Position Details Position Details

Position (ICRS)
RA = 6h 41m 12.4s
DEC = 9° 25’ 14.8”
Orientation
North is 4.6° CW
Field of View
3.1 x 3.1 arcminutes
Constellation
Monoceros

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Green Hubble (ACS) Optical (V) 568.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
Spectrum_base
Blue
Green
Red
Stsci_2002-11b_1280
×
ID
2002-11b
Subject Category
B.4.2.1  
Subject Name
Cone Nebula, NGC 2264
Credits
NASA, H. Ford (JHU), G. Illingworth (UCSC/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA
Release Date
2002-04-30T00:00:00
Lightyears
2,500
Redshift
2,500
Reference Url
https://hubblesite.org/contents/news-releases/2002/news-2002-11
Type
Observation
Image Quality
Good
Distance Notes
Distance in Lightyears
Facility
Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS
Color Assignment
Blue, Green, Red
Band
Optical, Optical, Optical
Bandpass
B, V, I
Central Wavelength
435, 568, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
100.30178073936, 9.42078513506
Reference Dimension
3690.00, 3743.00
Reference Pixel
1991.21361802203, 1777.08984495195
Scale
-0.00001389298, 0.00001389298
Rotation
-4.60855936335
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center FITS X FITS Y EPO X EPO Y 792.25 564.31 1325.58 757.03 1370.46 706.08 2461.28 1129.99 719.98 1131.39 1088.53 1879.71 1054.03 1533.43 1693.68 2729.22 Center Pixel Coordinates: 1845.00 100.30393006568 1871.50 9.42195227599
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p0211b-f-3690x3743.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0211b-f-3690x3743.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2002/11
Metadata Date
2022-07-06T00:00:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

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Universescalefull
2,500 light years

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