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Collection:
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NASA Spitzer Space Telescope Collection
Collection
NASA Spitzer Space Telescope Collection
Collection
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Title:
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Spitzer and Hubble Team Up To Find 'Big Baby' Galaxies in the Newborn Universe
Title
Spitzer and Hubble Team Up To Find 'Big Baby' Galaxies in the Newborn Universe
Title
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Description:
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This image demonstrates how data from two of NASA's Great Observatories, the Spitzer and Hubble Space Telescopes, are used to identify one of the most distant galaxies ever seen. This galaxy is unusually massive for its youthful age of 800 million years. (After the Big Bang, the Milky Way by comparison, is approximately 13 billion years old.) [Left] - The galaxy, named HUDF-JD2, was pinpointed among approximately 10,000 others in a small area of sky called the Hubble Ultra Deep Field. This is the deepest images of the universe ever made at optical and near-infrared wavelengths. [Upper Right] - A blow-up of one small area of the Hubble Ultra Deep Field is used to identify where the distant galaxy is located (inside green circle). This indicates that the galaxy's visible light has been absorbed by traveling billions of light-years through intervening hydrogen. [Center Right] - The galaxy was detected using Hubble's near infrared camera and multi-object spectrometer. But at near-infrared wavelengths it is very faint and red. [Bottom Right] - The Spitzer infrared array camera, easily detects the galaxy at longer infrared wavelengths. The instrument is sensitive to the light from older, redder stars which should make up most of the mass in a galaxy. The brightness of the infrared galaxy suggests that it is quite massive.
Description
This image demonstrates how data from two of NASA's Great Observatories, the Spitzer and Hubble Space Telescopes, are used to identify one of the most distant galaxies ever seen. This galaxy is unusually massive for its youthful age of 800 million years. (After the Big Bang, the Milky Way by comparison, is approximately 13 billion years old.) [Left] - The galaxy, named HUDF-JD2, was pinpointed among approximately 10,000 others in a small area of sky called the Hubble Ultra Deep Field. This is the deepest images of the universe ever made at optical and near-infrared wavelengths. [Upper Right] - A blow-up of one small area of the Hubble Ultra Deep Field is used to identify where the distant galaxy is located (inside green circle). This indicates that the galaxy's visible light has been absorbed by traveling billions of light-years through intervening hydrogen. [Center Right] - The galaxy was detected using Hubble's near infrared camera and multi-object spectrometer. But at near-infrared wavelengths it is very faint and red. [Bottom Right] - The Spitzer infrared array camera, easily detects the galaxy at longer infrared wavelengths. The instrument is sensitive to the light from older, redder stars which should make up most of the mass in a galaxy. The brightness of the infrared galaxy suggests that it is quite massive.
Description
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Release Date:
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2005/09/27
Release_Date
2005/09/27
Release Date
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Release Date:
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27 September 2005
Release_Date
27 September 2005
Release Date
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Press Release:
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Press_Release
Press Release
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Release Credit:
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NASA, ESA/JPL-Caltech/B. Mobasher (STScI/ESA)
Release_Credit
NASA, ESA/JPL-Caltech/B. Mobasher (STScI/ESA)
Release Credit
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Image Credit:
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NASA, ESA/JPL-Caltech/B. Mobasher (STScI/ESA)
Image_Credit
NASA, ESA/JPL-Caltech/B. Mobasher (STScI/ESA)
Image Credit
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Object name:
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HUDF-JD2
Object_name
HUDF-JD2
Object name
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Object name:
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UDF033238.74-274839. 9
Object_name
UDF033238.74-274839. 9
Object name
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Object type:
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High-Redshift Galaxy in the Hubble Ultra Deep Field
Object_type
High-Redshift Galaxy in the Hubble Ultra Deep Field
Object type
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Position (J2000):
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*RA: *03h32m28.74s *Dec: *-27d48m39.90s
Position_(J2000)
*RA: *03h32m28.74s *Dec: *-27d48m39.90s
Position (J2000)
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Distance:
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redshift of z=6.5
Distance
redshift of z=6.5
Distance
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Constellation:
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Fornax
Constellation
Fornax
Constellation
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Wavelength:
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3.6, 4.5, 5.8, and 8.0 microns
Wavelength
3.6, 4.5, 5.8, and 8.0 microns
Wavelength
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Wavelength:
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ACS Filters: F435W (B), F606W (V), F775W (i), F850LP (z); NICMOS Filters: F110W (J110) and F160W (H160)
Wavelength
ACS Filters: F435W (B), F606W (V), F775W (i), F850LP (z); NICMOS Filters: F110W (J110) and F160W (H160)
Wavelength
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Observers:
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B. Mobasher (STScI/ESA); M. Dickinson (NOAO) H.C. Ferguson(STScI) M. Giavalisco (STScI) T. Wiklind (STScI/ESA) D. Stark (Caltech) R.S. Ellis (Caltech) M. Fall (STScI) N.A. Grogin (JHU) L. Moustakas (STScI) N. Panagia (STScI/ESA) M. Sosey, M. Stiavelli (STScI) E. Bergeron (STScI) S. Casertano (STScI) P. Ingram (Gemini Obs.) A. Koekemoer (STScI) I. Labbe (Carnegie Obs.) M. Livio (STScI) B. Rogers (Gemini Obs.) C. Scarlata (Inst. For Astronomy, Zurich, Switzerland) J. Venet (ESO) A. Renzini (ESO) P. Rosati (ESO) H. Kuntschner (STECF/ESO) M. Kummel (STECF/ESO) J.R. Walsh (STECF/ESO) H. Yan (SSC, Caltech) M. Dickinson (NOAO) D Stern (JPL) P.R.M. Eisenhardt (JPL) R.-R. Chary (SSC, Caltech) C.J. Conselice (Caltech) C. Papovich (Steward) W.T. Reach (SSC, Caltech) N. Grogin (STScI) L.A. Moustakas (JPL) M. Ouchi (STScI)
Observers
B. Mobasher (STScI/ESA); M. Dickinson (NOAO) H.C. Ferguson(STScI) M. Giavalisco (STScI) T. Wiklind (STScI/ESA) D. Stark (Caltech) R.S. Ellis (Caltech) M. Fall (STScI) N.A. Grogin (JHU) L. Moustakas (STScI) N. Panagia (STScI/ESA) M. Sosey, M. Stiavelli (STScI) E. Bergeron (STScI) S. Casertano (STScI) P. Ingram (Gemini Obs.) A. Koekemoer (STScI) I. Labbe (Carnegie Obs.) M. Livio (STScI) B. Rogers (Gemini Obs.) C. Scarlata (Inst. For Astronomy, Zurich, Switzerland) J. Venet (ESO) A. Renzini (ESO) P. Rosati (ESO) H. Kuntschner (STECF/ESO) M. Kummel (STECF/ESO) J.R. Walsh (STECF/ESO) H. Yan (SSC, Caltech) M. Dickinson (NOAO) D Stern (JPL) P.R.M. Eisenhardt (JPL) R.-R. Chary (SSC, Caltech) C.J. Conselice (Caltech) C. Papovich (Steward) W.T. Reach (SSC, Caltech) N. Grogin (STScI) L.A. Moustakas (JPL) M. Ouchi (STScI)
Observers
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Instrument:
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IRAC
Instrument
IRAC
Instrument
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Instrument:
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Hubble ACS & NICMOS
Instrument
Hubble ACS & NICMOS
Instrument
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Exposure Date:
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February 2004
Exposure_Date
February 2004
Exposure Date
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Exposure Date:
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ACS: September 24, 2003 - January 16, 2004; NICMOS: September 3, 2003 - November 27, 2003
Exposure_Date
ACS: September 24, 2003 - January 16, 2004; NICMOS: September 3, 2003 - November 27, 2003
Exposure Date
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Exposure Time:
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5 days
Exposure_Time
5 days
Exposure Time
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Exposure Time:
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ACS: 11.3 days NICMOS: 4.5 days
Exposure_Time
ACS: 11.3 days NICMOS: 4.5 days
Exposure Time
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Related links:
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Related_links
Related links
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note:
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*Hubble Ultra Deep Field* Screen-Resolution (450x450): JPEG [ http://ipac.jpl.nas
ssc2005-19b1_small.j pg ] High-Resolution (3100x3100): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/R. Windhorst (ASU) and H. Yan (SSC, Caltech)
note
*Hubble Ultra Deep Field* Screen-Resolution (450x450): JPEG [ http://ipac.jpl.nas
ssc2005-19b1_small.j pg ] High-Resolution (3100x3100): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/R. Windhorst (ASU) and H. Yan (SSC, Caltech)
note
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note:
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*Hubble visible-light view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a2_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/B. Mobasher (STScI/ESA)
note
*Hubble visible-light view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a2_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/B. Mobasher (STScI/ESA)
note
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note:
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*Hubble near-infrared view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a3_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/B. Mobasher (STScI/ESA)
note
*Hubble near-infrared view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a3_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA, ESA/B. Mobasher (STScI/ESA)
note
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note:
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*Spitzer infrared view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a4_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA/JPL-Caltech/B. Mobasher (STScI/ESA)
note
*Spitzer infrared view* Screen-Resolution (450x313): JPEG [ http://ipac.jpl.nas
ssc2005-19a4_small.j pg ] High-Resolution (948x660): JPEG | Mac TIFF | PC TIFF Credit: NASA/JPL-Caltech/B. Mobasher (STScI/ESA)
note
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facet_what:
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Spitzer Space Telescope
facet_what
Spitzer Space Telescope
facet_what
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facet_what:
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Visible Light
facet_what
Visible Light
facet_what
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facet_what:
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Spectrometer
facet_what
Spectrometer
facet_what
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facet_what:
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ESO
facet_what
ESO
facet_what
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facet_what:
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Gemini
facet_what
Gemini
facet_what
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facet_what:
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JD2
facet_what
JD2
facet_what
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facet_what:
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Multi-Object Spectrometer
facet_what
Multi-Object Spectrometer
facet_what
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facet_what:
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Fornax
facet_what
Fornax
facet_what
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facet_what:
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NICMOS
facet_what
NICMOS
facet_what
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facet_what:
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galaxies
facet_what
galaxies
facet_what
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facet_what:
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Infrared Array Camera (IRAC)
facet_what
Infrared Array Camera (IRAC)
facet_what
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facet_what:
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Hubble Space Telescope (HST)
facet_what
Hubble Space Telescope (HST)
facet_what
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facet_what:
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Near Infrared Camera and Multi-Object Spectrometer (NICMOS)
facet_what
Near Infrared Camera and Multi-Object Spectrometer (NICMOS)
facet_what
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facet_where:
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Switzerland
facet_where
Switzerland
facet_where
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facet_where:
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Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
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facet_where:
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Washington, D.C.
facet_where
Washington, D.C.
facet_where
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facet_where:
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Stennis Space Center (SSC)
facet_where
Stennis Space Center (SSC)
facet_where
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facet_when:
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February 2004
facet_when
February 2004
facet_when
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facet_when:
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September 24, 2003
facet_when
September 24, 2003
facet_when
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facet_when:
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January 16, 2004
facet_when
January 16, 2004
facet_when
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facet_when:
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September 3, 2003
facet_when
September 3, 2003
facet_when
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facet_when:
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November 27, 2003
facet_when
November 27, 2003
facet_when
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facet_when:
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27 September 2005
facet_when
27 September 2005
facet_when
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facet_when_year:
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2005
facet_when_year
2005
facet_when_year
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facet_when_year:
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2003
facet_when_year
2003
facet_when_year
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facet_when_year:
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2004
facet_when_year
2004
facet_when_year
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Image #:
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ssc2005-19b
Image_#
ssc2005-19b
Image #
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original url:
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original_url
original url
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UID:
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SPD-SPITZ-ssc2005-19 b
UID
SPD-SPITZ-ssc2005-19 b
UID
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