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Collection:
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NASA Great Images in Nasa Collection
Collection
NASA Great Images in Nasa Collection
Collection
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Title:
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Peering into the Heart of the Crab Nebula
Title
Peering into the Heart of the Crab Nebula
Title
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Full Description:
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In the year 1054 A.D., Chinese astronomers were startled by the appearance of a new star, so bright that it was visible in broad daylight for several weeks. Today, the Crab Nebula is visible at the site of the "Guest Star." Located about 6,500 light-years from Earth, the Crab Nebula is the remnant of a star that began its life with about 10 times the mass of our own Sun. Its life ended on July 4, 1054 when it exploded as a supernova. In this image, NASA's Hubble Space Telescope has zoomed in on the center of the Crab to reveal its structure with unprecedented detail. The Crab Nebula data were obtained by Hubble's Wide Field and Planetary Camera 2 in 1995. Images taken with five different color filters have been combined to construct this new false-color picture. Resembling an abstract painting by Jackson Pollack, the image shows ragged shards of gas that are expanding away from the explosion site at over 3 million miles per hour. The core of the star has survived the explosion as a pulsar, visible in the Hubble image as the lower of the two moderately bright stars to the upper left of center. The pulsar is a neutron star that spins on its axis 30 times a second. It heats its surroundings, creating the ghostly diffuse bluish-green glowing gas cloud in its vicinity, including a blue arc just to its right. The colorful network of filaments is the material from the outer layers of the star that was expelled during the explosion. The picture is somewhat deceptive in that the filaments appear to be close to the pulsar. In reality, the yellowish green filaments toward the bottom of the image are closer to us, and approaching at some 300 miles per second. The orange and pink filaments toward the top of the picture include material behind the pulsar, rushing away from us at similar speeds. The various colors in the picture arise from different chemical elements in the expanding gas, including hydrogen (orange), nitrogen (red), sulfur (pink), and oxygen (green). The shades of color represent variations in the temperature and density of the gas, as well as changes in the elemental composition. Kris Davidson (U. Minn.) led the research team of William P. Blair (JHU), Robert A. Fesen (Dartmouth), Alan Uomoto (JHU), Gordon M. MacAlpine (U. Mich.), and Richard B.C. Henry (U. Okla.) in the collection of the HST data. The Hubble Heritage Team created the color image from black and white data processed by Dr. Blair.
Full_Description
In the year 1054 A.D., Chinese astronomers were startled by the appearance of a new star, so bright that it was visible in broad daylight for several weeks. Today, the Crab Nebula is visible at the site of the "Guest Star." Located about 6,500 light-years from Earth, the Crab Nebula is the remnant of a star that began its life with about 10 times the mass of our own Sun. Its life ended on July 4, 1054 when it exploded as a supernova. In this image, NASA's Hubble Space Telescope has zoomed in on the center of the Crab to reveal its structure with unprecedented detail. The Crab Nebula data were obtained by Hubble's Wide Field and Planetary Camera 2 in 1995. Images taken with five different color filters have been combined to construct this new false-color picture. Resembling an abstract painting by Jackson Pollack, the image shows ragged shards of gas that are expanding away from the explosion site at over 3 million miles per hour. The core of the star has survived the explosion as a pulsar, visible in the Hubble image as the lower of the two moderately bright stars to the upper left of center. The pulsar is a neutron star that spins on its axis 30 times a second. It heats its surroundings, creating the ghostly diffuse bluish-green glowing gas cloud in its vicinity, including a blue arc just to its right. The colorful network of filaments is the material from the outer layers of the star that was expelled during the explosion. The picture is somewhat deceptive in that the filaments appear to be close to the pulsar. In reality, the yellowish green filaments toward the bottom of the image are closer to us, and approaching at some 300 miles per second. The orange and pink filaments toward the top of the picture include material behind the pulsar, rushing away from us at similar speeds. The various colors in the picture arise from different chemical elements in the expanding gas, including hydrogen (orange), nitrogen (red), sulfur (pink), and oxygen (green). The shades of color represent variations in the temperature and density of the gas, as well as changes in the elemental composition. Kris Davidson (U. Minn.) led the research team of William P. Blair (JHU), Robert A. Fesen (Dartmouth), Alan Uomoto (JHU), Gordon M. MacAlpine (U. Mich.), and Richard B.C. Henry (U. Okla.) in the collection of the HST data. The Hubble Heritage Team created the color image from black and white data processed by Dr. Blair.
Full Description
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Date:
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06/01/2000
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NASA Center:
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Hubble Space Telescope Center
NASA_Center
Hubble Space Telescope Center
NASA Center
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Subject Category:
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Deep Space Studies
Subject_Category
Deep Space Studies
Subject Category
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Subject Category:
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Hubble
Subject_Category
Hubble
Subject Category
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Keywords:
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Space
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Keywords:
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Field
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Keywords:
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Camera
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Keywords:
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Telescope
Keywords
Telescope
Keywords
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Keywords:
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Wide
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Keywords:
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Planetary
Keywords
Planetary
Keywords
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Keywords:
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Hubble
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Keywords:
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HST
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Keywords:
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Nebula
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Keywords:
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WFPC
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Keywords:
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Crab
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Audience:
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General Public
Audience
General Public
Audience
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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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Earth
facet_what
Earth
facet_what
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facet_what:
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Sun
facet_what
Sun
facet_what
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facet_what:
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Aura
facet_what
Aura
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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Jackson
facet_where
Jackson
facet_where
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facet_when:
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1995
facet_when
1995
facet_when
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facet_when:
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July 4, 1054
facet_when
July 4, 1054
facet_when
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facet_when:
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06-01-2000
facet_when
06-01-2000
facet_when
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facet_when_year:
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1995
facet_when_year
1995
facet_when_year
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facet_when_year:
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2000
facet_when_year
2000
facet_when_year
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facet_when_year:
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1054
facet_when_year
1054
facet_when_year
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Image #:
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PR00-15
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original_url:
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original_url
original_url
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UID:
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SPD-GRIN-GPN-2000-00 0895
UID
SPD-GRIN-GPN-2000-00 0895
UID
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Center:
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HSTI
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Center Number:
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PR00-15
Center_Number
PR00-15
Center Number
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GRIN DataBase Number:
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GPN-2000-000895
GRIN_DataBase_Number
GPN-2000-000895
GRIN DataBase Number
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Creator-Photographer:
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NASA, The Hubble Heritage Team, STScI, AURA ODPeering into the Heart
Creator-Photographer
NASA, The Hubble Heritage Team, STScI, AURA ODPeering into the Heart
Creator-Photographer
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Original Source:
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DIGITAL
Original_Source
DIGITAL
Original Source
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