Media Information

 
 
 
Collection:
NASA Spitzer Space Telescope Collection
Title:
Spitzer Discovers Hidden Ring
Description:
This animation transitions from a visible light image of the planetary nebula called NGC 246 to Spitzer's new infrared view. The movie highlights Spitzer's ability to see the invisible; as the movie dissolves to the Spitzer image, a giant ring (red) emerges. This clumpy ring consists of material that was expelled from the aging star at the center of the nebula.

Planetary nebulas are clouds of gas and dust that surround dying stars. When a star like our own Sun begins to run out of fuel, its core shrinks and heats up, boiling off the star's outer layers. Leftover material shoots outward, expanding in shells around the star. This ejected material is then bombarded with ultraviolet light from the central star's fiery surface, producing huge, glowing clouds -- planetary nebulas -- that look like giant jellyfish in space.

In the Spitzer image, the expelled gases appear green, and the ring of expelled material appears red. Astronomers believe the ring is likely made of hydrogen molecules that were ejected from the star in the form of atoms, then cooled to make hydrogen pairs. The new data will help explain how planetary nebulas take shape, and how they nourish future generations of stars.

The Spitzer image composite was taken on Dec. 6, 2003, by Spitzer's infrared array camera, and is composed of images obtained at four wavelengths: 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red).

The visible light image is from the Advanced Observing Program of the National Optical Astronomy Observatory. Visible-light image credit: Jeff Cremer/Adam Block/NOAO/AURA/NSF
Release Date:
2004/08/09
Press Release:
Dying Star Goes Out With a Ring [ http://www.spitzer.…]
Release Credit:
NASA/JPL-Caltech/R. Hurt (SSC-Caltech)
Image Credit:
NASA/JPL-Caltech/J. Hora (Harvard-Smithsonian CfA)
Object name:
NGC 246
Object type:
Planetary nebula
Position (J2000):
*RA: *00h47m4.52s *Dec: *-11d52m19.00s
Distance:
1,800 light-years or 550 parsecs
Constellation:
Cetus
Wavelength:
3.6 (blue), 4.5 (green), 5.8 (orange), 8.0 (red) microns
Image scale:
5.2x5.2 arcmin
Observers:
Joseph Hora - Principal Investigator (Harvard-Smithsonian Center for Astrophysics)
Lori Allen (Harvard-Smithsonian Center for Astrophysics)
Lynne Deutsch (Harvard-Smithsonian Center for Astrophysics)
Giovanni Fazio (Harvard-Smithsonian Center for Astrophysics)
William Latter (Spitzer Science Center)
Massimo Marengo (Harvard-Smithsonian Center for Astrophysics)
Judith Pipher (University of Rochester)
Instrument:
IRAC
Exposure Date:
06 Dec 2003
Exposure Time:
214 sec
Orientation:
North is 58.5 deg CW from up
Magnitude:
11.78
facet_what:
Spitzer Space Telescope
facet_what:
Visible Light
facet_what:
Sun
facet_what:
Aura
facet_what:
Cetus
facet_what:
Infrared Array Camera (IRAC)
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_where:
Stennis Space Center (SSC)
facet_when:
06 Dec 2003
facet_when_year:
2003
Image #:
ssc2004-13v1
original url:
UID:
SPD-SPITZ-ssc2004-13 v1

Spitzer Discovers Hidden Ring