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Collection:
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NASA Hubble Space Telescope Collection
Collection
NASA Hubble Space Telescope Collection
Collection
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Title:
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Gaseous Streamers Flutter in Stellar Breeze
Title
Gaseous Streamers Flutter in Stellar Breeze
Title
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Object Name:
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N44C
Object_Name
N44C
Object Name
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General Information:
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What is Hubble Heritage?
A monthly showcase of new and archival Hubble images. Go to the Heritage site.
Back to top [ #top ]
General_Information
What is Hubble Heritage?
A monthly showcase of new and archival Hubble images. Go to the Heritage site.
Back to top [ #top ]
General Information
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Acknowledgement:
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Acknowledgement
Acknowledgement
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Acknowledgement:
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* Acknowledgment:* D. Garnett (University of Arizona)
Acknowledgement
* Acknowledgment:* D. Garnett (University of Arizona)
Acknowledgement
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Fast Facts:
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Technical facts about this news release: About the Object Object Name: N44C Object Description: H II Region in the Large Magellanic Cloud Position (J2000): R.A. 05h 22m 07.91s Dec. -67° 59' 12.95" Constellation: Dorado Distance: About 50 kiloparsecs (160,000 light-years) Dimensions: The image is roughly 2.7 arcminutes (126 light-years or 38 parsecs) across. About the Data Instrument: WFPC2 Exposure Date(s): November 13, 1996 Exposure Time: 1.3 hours Principal Astronomers: D. Garnett (U. Arizona), Y.-H. Chu (U. Illinois), V. Galarza (Museum of Science and Industry, Chicago) About the Image Image Credit: NASA and The Hubble Heritage Team (STScI/AURA) Release Date: May 9, 2002 Filters: F502N ([O III]), F547M (Strömgren y), F656N (H-alpha), F675W (R) Orientation: Gaseous Streamers from Nebula N44C Flutter in Stellar Breeze [ http://imgsrc.hubbl…]
Fast_Facts
Technical facts about this news release: About the Object Object Name: N44C Object Description: H II Region in the Large Magellanic Cloud Position (J2000): R.A. 05h 22m 07.91s Dec. -67° 59' 12.95" Constellation: Dorado Distance: About 50 kiloparsecs (160,000 light-years) Dimensions: The image is roughly 2.7 arcminutes (126 light-years or 38 parsecs) across. About the Data Instrument: WFPC2 Exposure Date(s): November 13, 1996 Exposure Time: 1.3 hours Principal Astronomers: D. Garnett (U. Arizona), Y.-H. Chu (U. Illinois), V. Galarza (Museum of Science and Industry, Chicago) About the Image Image Credit: NASA and The Hubble Heritage Team (STScI/AURA) Release Date: May 9, 2002 Filters: F502N ([O III]), F547M (Strömgren y), F656N (H-alpha), F675W (R) Orientation: Gaseous Streamers from Nebula N44C Flutter in Stellar Breeze [ http://imgsrc.hubbl…] Fast Facts
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note:
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*Image Type:*: Astronomical
note
*Image Type:*: Astronomical
note
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note:
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*Release Date*:May 9, 2002 12:00 AM (EDT)
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*Release Date*:May 9, 2002 12:00 AM (EDT)
note
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note:
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*News Release Number:*: STScI-2002-12a
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*News Release Number:*: STScI-2002-12a
note
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note:
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*Title*:Gaseous Streamers Flutter in Stellar Breeze
note
*Title*:Gaseous Streamers Flutter in Stellar Breeze
note
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note:
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*Description*: Resembling the hair in Botticelli's famous portrait of the birth of Venus [ http://heritage.sts…], softly glowing filaments stream from a complex of hot young stars. This image of a nebula, known as N44C, comes from the archives of NASA's Hubble Space Telescope (HST). It was taken with the Wide Field Planetary Camera 2 in 1996 and is being presented by the Hubble Heritage Project. N44C is the designation for a region of glowing hydrogen gas surrounding an association of young stars in the Large Magellanic Cloud, a nearby, small companion galaxy to the Milky Way visible from the Southern Hemisphere. N44C is peculiar because the star mainly responsible for illuminating the nebula is unusually hot. The most massive stars, ranging from 10-50 times more massive than the Sun, have maximum temperatures of 54,000 to 90,000 degrees Fahrenheit (30,000 to 50,000 degrees Kelvin). The star illuminating N44C appears to be significantly hotter, with a temperature of about 135,000 degrees Fahrenheit (75,000 degrees Kelvin)! Ideas proposed to explain this unusually high temperature include the possibility of a neutron star or black hole that intermittently produces X-rays but is now "switched off." On the top right of this Hubble image is a network of nebulous filaments that inspired comparison to Botticelli. The filaments surround a Wolf-Rayet star, another kind of rare star characterized by an exceptionally vigorous "wind" of charged particles. The shock of the wind colliding with the surrounding gas causes the gas to glow. N44C is part of the larger N44 complex, which includes young, hot, massive stars, nebulae, and a "superbubble" blown out by multiple supernova explosions. Part of the superbubble is seen in red at the very bottom left of the HST image. The data were taken in November 1996 with Hubble's Wide Field Planetary Camera 2 by Donald Garnett (University of Arizona) and collaborators and stored in the Hubble archive. The image was composed by the Hubble Heritage Team (STScI/AURA).
note
*Description*: Resembling the hair in Botticelli's famous portrait of the birth of Venus [ http://heritage.sts…], softly glowing filaments stream from a complex of hot young stars. This image of a nebula, known as N44C, comes from the archives of NASA's Hubble Space Telescope (HST). It was taken with the Wide Field Planetary Camera 2 in 1996 and is being presented by the Hubble Heritage Project. N44C is the designation for a region of glowing hydrogen gas surrounding an association of young stars in the Large Magellanic Cloud, a nearby, small companion galaxy to the Milky Way visible from the Southern Hemisphere. N44C is peculiar because the star mainly responsible for illuminating the nebula is unusually hot. The most massive stars, ranging from 10-50 times more massive than the Sun, have maximum temperatures of 54,000 to 90,000 degrees Fahrenheit (30,000 to 50,000 degrees Kelvin). The star illuminating N44C appears to be significantly hotter, with a temperature of about 135,000 degrees Fahrenheit (75,000 degrees Kelvin)! Ideas proposed to explain this unusually high temperature include the possibility of a neutron star or black hole that intermittently produces X-rays but is now "switched off." On the top right of this Hubble image is a network of nebulous filaments that inspired comparison to Botticelli. The filaments surround a Wolf-Rayet star, another kind of rare star characterized by an exceptionally vigorous "wind" of charged particles. The shock of the wind colliding with the surrounding gas causes the gas to glow. N44C is part of the larger N44 complex, which includes young, hot, massive stars, nebulae, and a "superbubble" blown out by multiple supernova explosions. Part of the superbubble is seen in red at the very bottom left of the HST image. The data were taken in November 1996 with Hubble's Wide Field Planetary Camera 2 by Donald Garnett (University of Arizona) and collaborators and stored in the Hubble archive. The image was composed by the Hubble Heritage Team (STScI/AURA). note
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facet_what:
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Sun
facet_what
Sun
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facet_what:
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Camera 2
facet_what
Camera 2
facet_what
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facet_what:
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Venus
facet_what
Venus
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facet_what:
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COMPASS
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COMPASS
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facet_what:
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Aura
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Aura
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facet_what:
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Dorado
facet_what
Dorado
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_where:
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Large Magellanic Cloud
facet_where
Large Magellanic Cloud
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facet_where:
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Arizona
facet_where
Arizona
facet_where
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facet_where:
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Venus
facet_where
Venus
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facet_where:
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Illinois
facet_where
Illinois
facet_where
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facet_where:
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Chicago
facet_where
Chicago
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_when:
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1996
facet_when
1996
facet_when
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facet_when:
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November 13, 1996
facet_when
November 13, 1996
facet_when
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facet_when:
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May 9, 2002
facet_when
May 9, 2002
facet_when
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facet_when:
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November 1996
facet_when
November 1996
facet_when
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facet_when_year:
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2002
facet_when_year
2002
facet_when_year
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facet_when_year:
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1996
facet_when_year
1996
facet_when_year
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UID:
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SPD-HUBBLE-STScI-200 2-12a
UID
SPD-HUBBLE-STScI-200 2-12a
UID
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original url:
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original_url
original url
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Release Date:
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May 9, 2002 12:00 AM (EDT)
Release_Date
May 9, 2002 12:00 AM (EDT)
Release Date
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