Media Information

 
 
 
Collection:
NASA Spitzer Space Telescope Collection
Title:
Older Galaxy Pair Has Surprisingly Youthful Glow
Description:
A pair of interacting galaxies might be experiencing the galactic equivalent of a mid-life crisis. For some reason, the pair, called Arp 82, didn't make their stars early on as is typical of most galaxies. Instead, they got a second wind later in life -- about 2 billion years ago -- and started pumping out waves of new stars as if they were young again. Arp 82 is an interacting pair of galaxies with a strong bridge and a long tail. NGC 2535 is the big galaxy and NGC 2536 is its smaller companion. The disk of the main galaxy looks like an eye, with a bright "pupil" in the center and oval-shaped "eyelids." Dramatic "beads on a string" features are visible as chains of evenly spaced star-formation complexes along the eyelids. These are presumably the result of large-scale gaseous shocks from a grazing encounter. The colors of this galaxy indicate that the observed stars are young to intermediate in age, around 2 million to 2 billion years old, much less than the age of the universe (13.7 billion years). The puzzle is: why didn't Arp 82 form many stars earlier, like most galaxies of that mass range? Scientifically, it is an oddball and provides a relatively nearby lab for studying the age of intermediate-mass galaxies. This picture is a composite captured by Spitzer's infrared array camera with light at wavelength 8 microns shown in red, NASA's Galaxy Evolution Explorer combined 1530 and 2310 Angstroms shown in blue, and the Southeastern Association for Research in Astronomy Observatory light at 6940 Angstroms shown in green.
Release Date:
2007/01/10
Release Credit:
NASA/JPL-Caltech/M. Hancock (E. Tenn. State Univ.)
Image Credit:
NASA/JPL-Caltech/M. Hancock (East Tennessee State University)
Object name:
Arp 82
Object type:
Interacting Galaxie
Position (J2000):
*RA: *08h11m13.50s *Dec: *25d12m25.00s
Wavelength:
8.0 microns (red, continuum subtracted)
Wavelength:
1530 and 2310 Angstroms (blue); R Band 6940 Angstroms (green)
Observers:
M. Hancock (East Tennessee State University) B. J. Smith (East Tennessee State University) C. Struck (Iowa State University) M. L. Giroux (East Tennessee State University) P. N. Appleton (Spitzer Science Center) V. Charmandaris (University of Crete) W. T. Reach (Spitzer Science Center)
Instrument:
IRAC
Instrument:
GALEX (Near- and Far-UV Detectors) and SARA (optical)
Exposure Date:
2004-11-01
Exposure Date:
GALEX: 2005-02-13; SARA: 2005-01-03
Exposure Time:
6x12 seconds in each filter
Exposure Time:
GALEX FUV 1684 seconds, NUV 3019 seconds; SARA H-alpha 16x600 seconds, R 5x500 seconds
facet_what:
GALEX
facet_what:
Explorer
facet_what:
Galaxy Evolution Explorer
facet_what:
SARA
facet_what:
Infrared Array Camera (IRAC)
facet_where:
Tennessee
facet_where:
Iowa
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
Image #:
sig07-002
original url:
http://sscws1.ipac.…
UID:
SPD-SPITZ-sig07-002
Image ID:
168524
Resolution Size:
4
Format:
JPEG
Media Type:
Image
File Name:
sig07-002_mac.jpg
Width:
975
Height:
700

Older Galaxy Pair Has Surprisingly Youthful Glow