The Mice (NGC 4676): Colliding Galaxies With Tails of Stars and Gas

Stsci_2002-11d_1024

stsci_2002-11d April 30th, 2002

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

The Advanced Camera for Surveys (ACS), the newest camera on NASA's Hubble Space Telescope, has captured a spectacular pair of galaxies engaged in a celestial dance of cat and mouse or, in this case, mouse and mouse. Located 300 million light-years away in the constellation Coma Berenices, the colliding galaxies have been nicknamed "The Mice" because of the long tails of stars and gas emanating from each galaxy. Otherwise known as NGC 4676, the pair will eventually merge into a single giant galaxy. The image shows the most detail and the most stars that have ever been seen in these galaxies. In the galaxy at left, the bright blue patch is resolved into a vigorous cascade of clusters and associations of young, hot blue stars, whose formation has been triggered by the tidal forces of the gravitational interaction. Streams of material can also be seen flowing between the two galaxies. The clumps of young stars in the long, straight tidal tail [upper right] are separated by fainter regions of material. These dim regions suggest that the clumps of stars have formed from the gravitational collapse of the gas and dust that once occupied those areas. Some of the clumps have luminous masses comparable to dwarf galaxies that orbit in the halo of our own Milky Way Galaxy. Computer simulations by astronomers Josh Barnes (University of Hawaii) and John Hibbard (National Radio Astronomy Observatory, Charlottesville, Va.) show that we are seeing two nearly identical spiral galaxies approximately 160 million years after their closest encounter. The long, straight arm is actually curved, but appears straight because we see it edge-on. The simulations also show that the pair will eventually merge, forming a large, nearly spherical galaxy (known as an elliptical galaxy). The stars, gas, and luminous clumps of stars in the tidal tails will either fall back into the merged galaxies or orbit in the halo of the newly formed elliptical galaxy. The Mice presage what may happen to our

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
NGC 4676 The Mice
Subject - Local Universe
Galaxy > Type > Interacting

Distance Details Distance

Universescale3
300,000,000 light years
Stsci_2002-11d_128
 

Position Details Position Details

Position (ICRS)
RA = 12h 46m 11.0s
DEC = 30° 43’ 40.9”
Orientation
North is 69.0° CW
Field of View
3.3 x 1.6 arcminutes
Constellation
Coma Berenices

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue Hubble (ACS) Optical (g) 475.0 nm
Green Hubble (ACS) Optical (V) 606.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
Spectrum_base
Blue
Green
Red
Stsci_2002-11d_1280
×
ID
2002-11d
Subject Category
C.5.1.7  
Subject Name
NGC 4676, The Mice
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
300,000,000
Redshift
300,000,000
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
g, V, I
Central Wavelength
475, 606, 814
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
191.54574077445, 30.72802792414
Reference Dimension
3973.00, 1865.00
Reference Pixel
1992.24701938759, 1173.17012164001
Scale
-0.00001395873, 0.00001395873
Rotation
-69.03016988784
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 1381.88 1559.50 1749.49 668.98 1387.91 1544.14 1782.12 668.98 1305.95 1833.95 1176.14 724.53 1336.47 1893.26 1087.94 821.59 1567.27 1857.06 1322.78 1224.94 1617.44 1693.72 1665.52 1203.01 Center Pixel Coordinates: 1986.50 191.54213961949 932.50 30.72675671099
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-p0211d-f-3973x1865.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0211d-f-3973x1865.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
300,000,000 light years

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