Chandra X-ray Observatory: Kepler's Supernova Remnant (close-up, X-ray data)
This image shows a section of the remains of Kepler's Supernova, the most recent exploding star to be seen in the Milky Way Galaxy. It was first observed 400 years ago when it was thought to be 'a new star'. In fact, it was the the gas and dust from an exploding star, rapidly expanding. These remnants have now reached a diameter of 14 light years wide and are still expanding at 4 million miles per hour.
This image was taken by the Chandra X-ray Observatory.
Credit:NASA, CXC and S. Holt (F.W. Olin College of Engineering)
About the Image
About the Object
Name: | Kepler's SN |
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Type: | Milky Way : Nebula : Type : Supernova Remnant |
Distance: | 13000 light years |
Constellation: | Ophiuchus |
Category: | Nebulae |
Coordinates
Position (RA): | 17 30 37.93 |
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Position (Dec): | -21° 28' 46.56" |
Field of view: | 1.66 x 2.07 arcminutes |
Orientation: | North is -0.0° left of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
X-ray High energy X-ray |
Chandra
ACIS | |
X-ray Medium energy X-ray |
Chandra
ACIS | |
X-ray Low energy X-ray |
Chandra
ACIS | |
Infrared Mid-IR | 24 μm |
Chandra
ACIS |