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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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Forming a Planetary Gap
Title
Forming a Planetary Gap
Title
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Description:
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Astronomers are using NASA's Spitzer Space Telescope to probe the structures of circumstellar discs, the dusty discs that surround young stars, to look for the earliest signs of the formation of planetary systems. Examining young stars in the constellation of Taurus known to have such discs, Spitzer's ultra-sensitive infrared spectrograph instrument has detected the clearest evidence to date that an inner gap has formed in the disc surrounding the star CoKu Tau 4. Such a gap could indicate the presence of a new planet that has formed from the missing material.
This animation illustrates one possible scenario for the formation of an inner gap. Initially we see the circumstellar disc around a young star, made of the dust, ices and gases from which planets might form. As we move in to view the inner disc, an unstable ripple forms in the inner part of the disc. The force of gravity acts upon this ripple, allowing the material to rapidly condense into a new planet. The innermost portions of the disc that did not condense onto the planet rapidly spiral in and accrete onto the star, adding a little more to its final mass.
Description
Astronomers are using NASA's Spitzer Space Telescope to probe the structures of circumstellar discs, the dusty discs that surround young stars, to look for the earliest signs of the formation of planetary systems. Examining young stars in the constellation of Taurus known to have such discs, Spitzer's ultra-sensitive infrared spectrograph instrument has detected the clearest evidence to date that an inner gap has formed in the disc surrounding the star CoKu Tau 4. Such a gap could indicate the presence of a new planet that has formed from the missing material.
This animation illustrates one possible scenario for the formation of an inner gap. Initially we see the circumstellar disc around a young star, made of the dust, ices and gases from which planets might form. As we move in to view the inner disc, an unstable ripple forms in the inner part of the disc. The force of gravity acts upon this ripple, allowing the material to rapidly condense into a new planet. The innermost portions of the disc that did not condense onto the planet rapidly spiral in and accrete onto the star, adding a little more to its final mass.
Description
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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/JPL-Caltech/R. Hurt (SSC-Caltech)
Release_Credit
NASA/JPL-Caltech/R. Hurt (SSC-Caltech)
Release Credit
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Object type:
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Circumstellar disk
Object_type
Circumstellar disk
Object type
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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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Taurus
facet_what
Taurus
facet_what
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facet_what:
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Infrared Spectrograph (IRS)
facet_what
Infrared Spectrograph (IRS)
facet_what
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facet_what:
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Advanced Communication Technology Satellite (ACTS)
facet_what
Advanced Communication Technology Satellite (ACTS)
facet_what
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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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Stennis Space Center (SSC)
facet_where
Stennis Space Center (SSC)
facet_where
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Image #:
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ssc2004-08v3
Image_#
ssc2004-08v3
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-ssc2004-08 v3
UID
SPD-SPITZ-ssc2004-08 v3
UID
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