Media Information

 
 
 
Collection:
NASA Spitzer Space Telescope Collection
Title:
Coronet: A Star-Formation Neighbor
Description:
While perhaps not quite as well known as its star-formation cousin Orion, the Corona Australis region (containing, at its heart, the Coronet cluster) is one of the nearest and most active regions of ongoing star formation. At only about 420 light-years away, the Coronet is over three times closer than the Orion nebula is to Earth. The Coronet contains a loose cluster of a few dozen young stars with a wide range of masses and at various stages of evolution, giving astronomers an opportunity to observe embryonic stars simultaneously in several wavelengths.

This composite image shows the Coronet in X-rays from Chandra (purple) and infrared from Spitzer (orange, green, and cyan). The Spitzer image shows young stars plus diffuse emission from dust. Due to the host of young stars in different life stages in the Coronet, astronomers can use these data to pinpoint details of how the youngest stars evolve.
Release Date:
2007/09/13
Release Credit:
NASA/CXC/JPL-Caltech /CfA
Image Credit:
NASA/JPL-Caltech/L. Allen (CfA) and the IRAC GTO team
Image Credit:
NASA/CXC/J. Forbrich(CfA)
Object name:
Coronet Cluster
Object type:
star cluster
Position (J2000):
*RA: *19h01m45.00s *Dec: *-36d58m9.00s
Distance:
424 light-years
Constellation:
Corona Australis
Wavelength:
4.5 microns (cyan), 8.0 microns (green), and 24 microns (orange)
Wavelength:
X-ray (purple)
Image scale:
16.8 x 16.8 arcmin
Instrument:
IRAC MIPS
Instrument:
Chandra
Exposure Date:
5 pointings between 08/08/2005 - 08/13/2005
Exposure Time:
43.5 hours
facet_what:
Earth
facet_what:
Orion
facet_what:
MIPS
facet_what:
Opportunity
facet_what:
Infrared Array Camera (IRAC)
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_when:
08-08-2005
facet_when:
08-13-2005
facet_when_year:
2005
Image #:
sig07-017
original url:
UID:
SPD-SPITZ-sig07-017

Coronet: A Star-Formation Neighbor