Spitzer Space Telescope: Kepler's Supernova Remnant (infrared data)
This image shows 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, taken by the Spitzer Space Telescope in the Infrared, shows microscopic dust particles — coloured red — that have been heated by the supernova shock wave.
Credit: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 41.06 |
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Position (Dec): | -21° 29' 26.79" |
Field of view: | 5.55 x 5.55 arcminutes |
Orientation: | North is 2.8° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
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Infrared Near-IR | 3.6 μm | Spitzer Space Telescope IRAC |
Infrared Near-IR | 4.5 μm | Spitzer Space Telescope IRAC |
Infrared Mid-IR | 8.0 μm | Spitzer Space Telescope IRAC |
Infrared Mid-IR | 24 μm | Spitzer Space Telescope IRAC |