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

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

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.

Credits

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

About The Object
Object Name Whirlpool Galaxy, M51, NGC 5194/5
Object Description Face-on Spiral Galaxy with Companion
R.A. Position 13h 29m 52.37s
Dec. Position 47° 11' 40.8"
Constellation Canes Venatici
Distance About 31 million light-years (9.6 Megaparsecs)
Dimensions 9.6 arcminutes (87,000 light-years or 27,000 parsecs) wide
About The Data
Data Description This image was created from HST data from proposal : S. Beckwith (STScI), R. Kennicutt Jr. (University of Arizona), and H. Bond, C. Christian, L. Frattare, F. Hamilton, Z. Levay, M. Mutchler, K. Noll, and T. Royle (The Hubble Heritage Team, STScI). NOTE: High level science products (combined and mosaiced fits files for each filter) are available at:
Instrument HST>ACS/WFC
Exposure Dates January 18-22, 2005, Exposure Time: 9.0 hours
Filters F435W (B), F555W (V), F658N (Halpha + [N II]), F814W (I)
About The Image
Color Info Blue: F435W (B) Green: F555W (V) Red: F658N (Halpha + [N II]) + F814W (I)
Compass Image Two galaxies sit side by side. The larger of the two galaxies is on the left side of image. At its center is a hazy yellow circular region from which two well-defined arms extend to form loose spirals around the middle. The arms consist of dark reddish-brown dust trails that are spotted with red stars and shrouded in a haze of blue stars. The smaller galaxy on the far-right side of the image is a hazy yellow sphere resembling the core of the first galaxy but with no spiral arms. It is about twice the size of the core in the first galaxy, but because it has no spiral arms it is much smaller. The view of this smaller galaxy is partially obstructed by the tip of one of the arms of the spiral galaxy, which appears to cover the top third of the smaller galaxy.
About The Object
Object Name A name or catalog number that astronomers use to identify an astronomical object.
Object Description The type of astronomical object.
R.A. Position Right ascension – analogous to longitude – is one component of an object's position.
Dec. Position Declination – analogous to latitude – is one component of an object's position.
Constellation One of 88 recognized regions of the celestial sphere in which the object appears.
Distance The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
Dimensions The physical size of the object or the apparent angle it subtends on the sky.
About The Data
Data Description
  • Proposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
  • Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
Instrument The science instrument used to produce the data.
Exposure Dates The date(s) that the telescope made its observations and the total exposure time.
Filters The camera filters that were used in the science observations.
About The Image
Image Credit The primary individuals and institutions responsible for the content.
Publication Date The date and time the release content became public.
Color Info A brief description of the methods used to convert telescope data into the color image being presented.
Orientation The rotation of the image on the sky with respect to the north pole of the celestial sphere.