Ionized Carbon Atoms in Orion

Nhsc_nhsc2016-003a_1024

nhsc_nhsc2016-003a October 12th, 2016

Credit: ESA/NASA/JPL-Caltech

The dusty side of the Sword of Orion is illuminated in this striking infrared image from the European Space Agency's Hershel Space Observatory.

This immense nebula is the closest large region of star formation, situated about 1,500 light years away in the constellation of Orion. The parts that are easily observed in visible light, known alternatively as the Orion Nebula or Messier 42, correspond to the light blue regions. This is the glow from the warmest dust, illuminated by clusters of hot stars that have only recently been born in this chaotic region.

The red spine of material running from corner to corner reveals colder, denser filaments of dust and gas that are scattered throughout the Orion nebula. In visible light this would be a dark, opaque feature, hiding the reservoir of material from which stars have recently formed and will continue to form in the future.

Herschel data from the PACS instrument observations, at wavelengths of 100 and 160 microns, is displayed in blue and green, respectively, while SPIRE 250-micron data is shown in red.

Within the inset image, the emission from ionized carbon atoms (C+), overlaid in yellow, was isolated and mapped out from spectrographic data obtained by the HIFI instrument.

Herschel is a European Space Agency mission, with science instruments provided by consortia of European institutes and with important participation by NASA. While the observatory stopped making science observations in April 2013, after running out of liquid coolant as expected, scientists continue to analyze its data. NASA's Herschel Project Office is based at JPL. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of IPAC, supports the U.S. astronomical community. Caltech manages JPL for NASA.

Provider: Herschel Space Observatory

Image Source: https://www.herschel.caltech.edu/image/nhsc2016-003a

Curator: NASA Herschel Science Center, Pasadena, CA, USA

Image Use Policy: http://www.herschel.caltech.edu/index.php?SiteSection=ImageUsePolicy

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Image Details Image Details

Image Type
Collage
Object Name
Orion Nebula Messier 42 M42
Subject - Milky Way
Nebula > Type > Star Formation
Nebula > Appearance > Emission

Distance Details Distance

Universescale1
1,344 light years
Nhsc_nhsc2016-003a_128
 

Position Details Position Details

Position (ICRS)
RA = 5h 34m 18.1s
DEC = -5° 43’ 24.9”
Orientation
North is up
Constellation
Orion

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Herschel (PACS) Infrared 100.0 µm
Green Herschel (PACS) Infrared 160.0 µm
Red Herschel (SPIRE) Infrared 250.0 µm
Yellow Herschel (HIFI) Infrared (C+ line) 157.8 µm
Spectrum_ir1
Blue
Green
Red
Yellow
Nhsc_nhsc2016-003a_1280
×
ID
nhsc2016-003a
Subject Category
B.4.1.2   B.4.2.1  
Subject Name
Orion Nebula, Messier 42, M42
Credits
ESA/NASA/JPL-Caltech
Release Date
2016-10-12
Lightyears
1,344
Redshift
1,344
Reference Url
https://www.herschel.caltech.edu/image/nhsc2016-003a
Type
Collage
Image Quality
Good
Distance Notes
Facility
Herschel, Herschel, Herschel, Herschel
Instrument
PACS, PACS, SPIRE, HIFI
Color Assignment
Blue, Green, Red, Yellow
Band
Infrared, Infrared, Infrared, Infrared
Bandpass
-, -, -, C+ line
Central Wavelength
100000, 160000, 250000, 157790
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
83.5753408, -5.7235745
Reference Dimension
Reference Pixel
Scale
Rotation
0.01
Coordinate System Projection:
TAN
Quality
Position
FITS Header
Notes
Creator (Curator)
NASA Herschel Science Center
URL
http://www.herschel.caltech.edu/
Name
Email
Telephone
Address
1200 E. California Blvd.
City
Pasadena
State/Province
CA
Publisher
NASA Herschel Science Center
Publisher ID
nhsc
Resource ID
Metadata Date
2018-06-21T00:05:35Z
Metadata Version
1.1
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Detailed color mapping information coming soon...

×
Universescalefull
1,344 light years

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