Out of This Whirl: the Whirlpool Galaxy (M51) and Companion Galaxy

Stsci_2005-12a_1024

stsci_2005-12a April 25th, 2005

Credit: NASA, ESA, S. Beckwith (STScI), and The Hubble Heritage Team (STScI/AURA)

The graceful, winding arms of the majestic spiral galaxy M51 (NGC 5194) appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust. This sharpest-ever image of the Whirlpool Galaxy, taken in January 2005 with the Advanced Camera for Surveys aboard NASA's Hubble Space Telescope, illustrates a spiral galaxy's grand design, from its curving spiral arms, where young stars reside, to its yellowish central core, a home of older stars. The galaxy is nicknamed the Whirlpool because of its swirling structure. The Whirlpool's most striking feature is its two curving arms, a hallmark of so-called grand-design spiral galaxies. Many spiral galaxies possess numerous, loosely shaped arms which make their spiral structure less pronounced. These arms serve an important purpose in spiral galaxies. They are star-formation factories, compressing hydrogen gas and creating clusters of new stars. In the Whirlpool, the assembly line begins with the dark clouds of gas on the inner edge, then moves to bright pink star-forming regions, and ends with the brilliant blue star clusters along the outer edge. Some astronomers believe that the Whirlpool's arms are so prominent because of the effects of a close encounter with NGC 5195, the small, yellowish galaxy at the outermost tip of one of the Whirlpool's arms. At first glance, the compact galaxy appears to be tugging on the arm. Hubble's clear view, however, shows that NGC 5195 is passing behind the Whirlpool. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years. As NGC 5195 drifts by, its gravitational muscle pumps up waves within the Whirlpool's pancake-shaped disk. The waves are like ripples in a pond generated when a rock is thrown in the water. When the waves pass through orbiting gas clouds within the disk, they squeeze the gaseous material along each arm's inner edge. The dark dusty material looks like gathering storm clouds. These dense clouds collapse, creating a wake of star birth, as seen in the bright pink star-forming regions. The largest stars eventually sweep away the dusty cocoons with a torrent of radiation, hurricane-like stellar winds, and shock waves from supernova blasts. Bright blue star clusters emerge from the mayhem, illuminating the Whirlpool's arms like city streetlights. The Whirlpool is one of astronomy's galactic darlings. Located 31 million light-years away in the constellation Canes Venatici (the Hunting Dogs), the Whirlpool's beautiful face-on view and closeness to Earth allow astronomers to study a classic spiral galaxy's structure and star-forming processes.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2005/news-2005-12

Curator: STScI, Baltimore, MD, USA

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

Image Details Image Details

Image Type
Observation
Object Name
Whirlpool Galaxy M51 NGC 5194/5
Subject - Local Universe
Galaxy > Type > Interacting
Galaxy > Grouping > Multiple
Galaxy > Type > Spiral

Distance Details Distance

Universescale2
31,000,000 light years
Stsci_2005-12a_128
 

Position Details Position Details

Position (ICRS)
RA = 13h 30m 1.3s
DEC = 47° 9’ 39.1”
Orientation
North is 91.8° CW
Field of View
9.5 x 6.6 arcminutes
Constellation
Canes Venatici

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
Red Hubble (ACS) Optical (Halpha [N II]) 658.0 nm
Red Hubble (ACS) Optical (I) 814.0 nm
November 4 - 7, 2004
Spectrum_base
Blue
Green
Red
Red
Stsci_2005-12a_1280
×
ID
2005-12a
Subject Category
C.5.1.7   C.5.5.2   C.5.1.1  
Subject Name
Whirlpool Galaxy, M51, NGC 5194/5
Credits
NASA, ESA, S. Beckwith (STScI), and The Hubble Heritage Team (STScI/AURA)
Release Date
2005-04-25T00:00:00
Lightyears
31,000,000
Redshift
31,000,000
Reference Url
https://hubblesite.org/contents/news-releases/2005/news-2005-12
Type
Observation
Image Quality
Good
Distance Notes
About 31 million light-years (9.6 Megaparsecs)
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
ACS, ACS, ACS, ACS
Color Assignment
Blue, Green, Red, Red
Band
Optical, Optical, Optical, Optical
Bandpass
B, V, Halpha [N II], I
Central Wavelength
435, 555, 658, 814
Start Time
2005-01-12T00:00:00, 2005-01-12T00:00:00, 2005-01-12T00:00:00, 2005-01-12T00:00:00
Integration Time
Dataset ID
Notes
N
Coordinate Frame
ICRS
Equinox
2000.0
Reference Value
202.50528309027, 47.16085095311
Reference Dimension
11477.00, 7965.00
Reference Pixel
2034.39341592733, 5929.20465741795
Scale
-0.00001385903, 0.00001385903
Rotation
-91.80774312061
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 801.43 450.45 2516.28 3272.98 872.33 1209.91 2404.27 1750.20 692.73 1328.74 2772.38 1516.84 1474.55 650.54 1174.13 2833.21 820.77 1679.04 2528.84 810.19 Center Pixel Coordinates: 5738.50 202.46854342544 3982.50 47.21291460221
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-p0512a-f-11477x7965.tif
Resource URL
https://mast.stsci.edu/api/latest/Download/file?uri=mast:OPO/product/STSCI-H-p0512a-f-11477x7965.tif
Related Resources
http://hubblesite.org/newscenter/archive/releases/2005/12
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
31,000,000 light years

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