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What Feeds the Beast in a Galaxy Cluster?
Ssc2015 03b

Credit: NASA/ESA/STScI/JPL-Caltech/McGill

Observation • September 10th, 2015 • ssc2015-03b

ssc2015-03b

A massive cluster of galaxies, called SpARCS1049+56, can be seen in this multi-wavelength view from NASA's Hubble and Spitzer space telescopes. At the middle of the picture is the largest, central member of the family of galaxies (upper right red dot of central pair). Unlike other central galaxies in clusters, this one is bursting with the birth of new stars.

Scientists say this star birth was triggered by a collision between a smaller galaxy and the giant, central galaxy. The smaller galaxy's wispy, shredded parts, called a tidal tail, can be seen coming out below the larger galaxy. Throughout this region are features called "beads on a string," which are areas where gas has clumped to form new stars.

This type of "feeding" mechanism for galaxy clusters -- where gas from the merging of galaxies is converted to new stars -- is rare.

The Hubble data in this image show infrared light with a wavelength of 1 micron in blue, and 1.6 microns in green. The Spitzer data show infrared light of 3.6 microns in red.

About the Object

Name
SpARCS1049+56
Type
Galaxy > Grouping > Cluster
Galaxy > Type > Interacting
Distance
9,800,000 Light Years
Redshift
1.7

Color Mapping

Band Wavelength Telescope
Infrared 1.1 µm Hubble WFC3
Infrared 1.6 µm Hubble WFC3
Infrared 3.6 µm Spitzer IRAC

Astrometrics

Position (J2000)
RA =10h 49m 22.7s
Dec = 56° 40' 31.4"
Field of View
0.8 x 0.8 arcminutes
Orientation
North is up