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Collection:
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NASA Planetary Photo Journal Collection
Collection
NASA Planetary Photo Journal Collection
Collection
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Title:
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Scene of Multiple Explosions
Title
Scene of Multiple Explosions
Title
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Original Caption Released with Image:
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This composite image shows Z Camelopardalis, or Z Cam, a double-star system featuring a collapsed, dead star, called a white dwarf, and a companion star, as well as a ghostly shell around the system. The massive shell provides evidence of lingering material ejected during and swept up by a powerful classical nova explosion that occurred probably a few thousand years ago.
The image combines data gathered from the far-ultraviolet and near-ultraviolet detectors on NASA's Galaxy Evolution Explorer on Jan. 25, 2004. The orbiting observatory first began imaging Z Cam in 2003.
Z Cam is the largest white object in the image, located near the center. Parts of the shell are seen as a lobe-like, wispy, yellowish feature below and to the right of Z Cam, and as two large, whitish, perpendicular lines on the left.
Z Cam was one of the first known recurrent dwarf nova, meaning it erupts in a series of small, "hiccup-like" blasts, unlike classical novae, which undergo a massive explosion. That's why the huge shell around Z Cam caught the eye of astronomer Dr. Mark Seibert of Carnegie Institution of Washington in Pasadena, Calif. - it could only be explained as the remnant of a full-blown classical nova explosion. This finding provides the first evidence that some binary systems undergo both types of explosions. Previously, a link between the two types of novae had been predicted, but there was no evidence to support the theory.
The faint bluish streak in the bottom right corner of the image is ultraviolet light reflected by dust that may or may not be related to Z Cam. Numerous foreground and background stars and galaxies are visible as yellow and white spots. The yellow objects are strong near-ultraviolet emitters; blue features have strong far-ultraviolet emission; and white objects have nearly equal amounts of near-ultraviolet and far-ultraviolet emission.
Original_Caption_Rel eased_with_Image
This composite image shows Z Camelopardalis, or Z Cam, a double-star system featuring a collapsed, dead star, called a white dwarf, and a companion star, as well as a ghostly shell around the system. The massive shell provides evidence of lingering material ejected during and swept up by a powerful classical nova explosion that occurred probably a few thousand years ago.
The image combines data gathered from the far-ultraviolet and near-ultraviolet detectors on NASA's Galaxy Evolution Explorer on Jan. 25, 2004. The orbiting observatory first began imaging Z Cam in 2003.
Z Cam is the largest white object in the image, located near the center. Parts of the shell are seen as a lobe-like, wispy, yellowish feature below and to the right of Z Cam, and as two large, whitish, perpendicular lines on the left.
Z Cam was one of the first known recurrent dwarf nova, meaning it erupts in a series of small, "hiccup-like" blasts, unlike classical novae, which undergo a massive explosion. That's why the huge shell around Z Cam caught the eye of astronomer Dr. Mark Seibert of Carnegie Institution of Washington in Pasadena, Calif. - it could only be explained as the remnant of a full-blown classical nova explosion. This finding provides the first evidence that some binary systems undergo both types of explosions. Previously, a link between the two types of novae had been predicted, but there was no evidence to support the theory.
The faint bluish streak in the bottom right corner of the image is ultraviolet light reflected by dust that may or may not be related to Z Cam. Numerous foreground and background stars and galaxies are visible as yellow and white spots. The yellow objects are strong near-ultraviolet emitters; blue features have strong far-ultraviolet emission; and white objects have nearly equal amounts of near-ultraviolet and far-ultraviolet emission.
Original Caption Released with Image
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note:
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This composite image shows Z Camelopardalis, or Z Cam, a double-star system featuring a collapsed, dead star, called a white dwarf, and a companion star, as well as a ghostly shell around the system [ http //photojournal.jpl.n asa.gov/animation/PI A09220 ]
Click on graphic to obtain download options
note
This composite image shows Z Camelopardalis, or Z Cam, a double-star system featuring a collapsed, dead star, called a white dwarf, and a companion star, as well as a ghostly shell around the system [ http //photojournal.jpl.n asa.gov/animation/PI A09220 ]
Click on graphic to obtain download options
note
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Image Credit:
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NASA/JPL-Caltech
Image_Credit
NASA/JPL-Caltech
Image Credit
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Produced By:
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California Institute of Technology
Produced_By
California Institute of Technology
Produced By
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Mission:
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Galaxy Evolution Explorer (GALEX)
Mission
Galaxy Evolution Explorer (GALEX)
Mission
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Spacecraft:
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GALEX Orbiter
Spacecraft
GALEX Orbiter
Spacecraft
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Target Name:
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Z Camelopardalis
Target_Name
Z Camelopardalis
Target Name
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Instrument:
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Far-ultraviolet Detector
Instrument
Far-ultraviolet Detector
Instrument
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Instrument:
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Near-ultraviolet Detector
Instrument
Near-ultraviolet Detector
Instrument
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Product Size:
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1800 samples x 1800 lines
Product_Size
1800 samples x 1800 lines
Product Size
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facet_what:
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Explorer
facet_what
Explorer
facet_what
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facet_what:
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Galaxy Evolution Explorer
facet_what
Galaxy Evolution Explorer
facet_what
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facet_what:
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GALEX
facet_what
GALEX
facet_what
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facet_what:
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GALEX Orbiter
facet_what
GALEX Orbiter
facet_what
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facet_what:
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Far-ultraviolet Detector
facet_what
Far-ultraviolet Detector
facet_what
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facet_what:
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Camelopardalis
facet_what
Camelopardalis
facet_what
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facet_what:
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Near-ultraviolet Detector
facet_what
Near-ultraviolet Detector
facet_what
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facet_where:
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California
facet_where
California
facet_where
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facet_where:
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Washington
facet_where
Washington
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_when:
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2003
facet_when
2003
facet_when
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facet_when_year:
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2003
facet_when_year
2003
facet_when_year
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Image #:
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PIA09220
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UID:
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SPD-PHOTJ-PIA09220
UID
SPD-PHOTJ-PIA09220
UID
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orignial url:
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orignial_url
orignial url
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