Scene of Multiple Explosions

Galex_glx2007-02f_img01_1024

galex_glx2007-02f_img01 May 23rd, 2007

Credit: NASA/JPL-Caltech

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.

Provider: Galaxy Evolution Explorer

Image Source: /image/galex/glx2007-02f_img01

Curator: Spitzer Space Telescope

Image Use Policy: Public Domain

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Image Details Image Details

Image Type
Observation
Object Name
Z Camelopardalis
Subject - Milky Way
Star > Evolutionary Stage > White Dwarf
Nebula > Appearance > Emission
Galex_glx2007-02f_img01_128
 

Position Details Position Details

Position
RA = 8h 25m 13.7s
DEC = 73° 6’ 39.7”
Orientation
North is up
Field of View
1.6 x 1.6 degrees
Constellation
Camelopardalis

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Blue GALEX (FUV) Ultraviolet (Far-UV) 150.0 nm
Yellow GALEX (NUV) Ultraviolet (Near-UV) 230.0 nm
Spectrum_base
Blue
Yellow
Galex_glx2007-02f_img01_1280
×
ID
glx2007-02f_img01
Subject Category
B.3.1.7.   B.4.2.1.  
Subject Name
Z Camelopardalis
Credits
NASA/JPL-Caltech
Release Date
2007-05-23
Lightyears
Redshift
Reference Url
/image/galex/glx2007-02f_img01
Type
Observation
Image Quality
Good
Distance Notes
Facility
GALEX, GALEX
Instrument
FUV, NUV
Color Assignment
Blue, Yellow
Band
Ultraviolet, Ultraviolet
Bandpass
Far-UV, Near-UV
Central Wavelength
150, 230
Start Time
Integration Time
3428.
Dataset ID
Notes
Coordinate Frame
Equinox
J2000
Reference Value
126.30714, 73.11102
Reference Dimension
3840, 3840
Reference Pixel
1920.5, 1920.5
Scale
-0.000416666666666667, 0.000416666666666667
Rotation
0.
Coordinate System Projection:
TAN
Quality
FITS Header
Notes
Creator (Curator)
Spitzer Space Telescope
URL
http://www.galex.caltech.edu
Name
Email
Telephone
Address
City
State/Province
Postal Code
Country
Rights
Public Domain
Publisher
Galaxy Evolution Explorer
Publisher ID
galex
Resource ID
Resource URL
/image/galex/glx2007-02f_img01
Related Resources
Metadata Date
2024-02-27T00:13:28Z
Metadata Version
1.2
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Detailed color mapping information coming soon...

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There is no distance meta data in this image.

 

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