Happy Sweet Sixteen, Hubble Telescope! - Starburst Galaxy M82

Stsci_2006-14a_1024

stsci_2006-14a April 24th, 2006

Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA) Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)

To celebrate the Hubble Space Telescope's 16 years of success, the two space agencies involved in the project, NASA and the European Space Agency (ESA), are releasing this image of the magnificent starburst galaxy, Messier 82 (M82). This mosaic image is the sharpest wide-angle view ever obtained of M82. The galaxy is remarkable for its bright blue disk, webs of shredded clouds, and fiery-looking plumes of glowing hydrogen blasting out of its central regions. Throughout the galaxy's center, young stars are being born 10 times faster than they are inside our entire Milky Way Galaxy. The resulting huge concentration of young stars carved into the gas and dust at the galaxy's center. The fierce galactic superwind generated from these stars compresses enough gas to make millions of more stars. In M82, young stars are crammed into tiny but massive star clusters. These, in turn, congregate by the dozens to make the bright patches, or "starburst clumps," in the central parts of M82. The clusters in the clumps can only be distinguished in the sharp Hubble images. Most of the pale, white objects sprinkled around the body of M82 that look like fuzzy stars are actually individual star clusters about 20 light-years across and contain up to a million stars. The rapid rate of star formation in this galaxy eventually will be self-limiting. When star formation becomes too vigorous, it will consume or destroy the material needed to make more stars. The starburst then will subside, probably in a few tens of millions of years. Located 12 million light-years away, M82 appears high in the northern spring sky in the direction of the constellation Ursa Major, the Great Bear. It is also called the "Cigar Galaxy" because of the elliptical shape produced by the oblique tilt of its starry disk relative to our line of sight. The observation was made in March 2006, with the Advanced Camera for Surveys' Wide Field Channel. Astronomers assembled this six-image composite mosaic by combining exposures taken with four colored filters that capture starlight from visible and infrared wavelengths as well as the light from the glowing hydrogen filaments. Hubble was launched on April 24, 1990, aboard the space shuttle Discovery.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2006/news-2006-14

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
M82 NGC 3034
Subject - Local Universe
Galaxy > Activity > AGN
Galaxy > Type > Irregular

Distance Details Distance

Universescale2
12,000,000 light years
Stsci_2006-14a_128
 

Position Details Position Details

Position (ICRS)
RA = 9h 55m 17.3s
DEC = 69° 39’ 30.0”
Orientation
North is 50.2° CCW
Field of View
7.9 x 6.2 arcminutes
Constellation
Ursa Major

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (B) 435.0 nm
Green Hubble (ACS) Optical (V) 555.0 nm
Orange Hubble (ACS) Optical (Halpha) 658.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
March 27-29, 2006
Spectrum_base
Blue
Green
Orange
Red
Stsci_2006-14a_1280
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ID
2006-14a
Subject Category
C.5.3.2   C.5.1.6  
Subject Name
M82, NGC 3034
Credits
NASA, ESA, and The Hubble Heritage Team (STScI/AURA) Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI), and P. Puxley (National Science Foundation)
Release Date
2006-04-24T00:00:00
Lightyears
12,000,000
Redshift
12,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2006/news-2006-14
Type
Observation
Image Quality
Good
Distance Notes
12 million light-years (3.7 Megaparsecs)
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS, ACS
Color Assignment
Blue, Green, Orange, Red
Band
Optical, Optical, Optical, Optical
Bandpass
B, V, Halpha, I
Central Wavelength
435, 555, 658, 814
Start Time
2006-03-27T00:00:00, 2006-03-27T00:00:00, 2006-03-27T00:00:00, 2006-03-27T00:00:00
Integration Time
Dataset ID
Notes
M
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
148.82217492048, 69.65833998784
Reference Dimension
9500.00, 7400.00
Reference Pixel
8531.34769581406, 5657.83493428196
Scale
-0.00001392731, 0.00001392731
Rotation
50.22269665954
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 562.16 1850.84 7902.93 3626.11 1142.60 2281.16 9305.38 3288.60 989.84 854.98 6920.68 1697.58 1734.77 1002.17 8098.71 746.15 Center Pixel Coordinates: 4750.00 148.97963636155 3700.00 69.68117025277
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-p0614a-f-9500x7400.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0614a-f-9500x7400.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2006/14
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
12,000,000 light years

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