Spitzer Space Telescope: Kepler's Supernova Remnant (close-up, infrared 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, 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:

NASA, ESA, The Hubble Heritage Team (STScI/AURA)

About the Image

NASA press release
Id:opo0429m
Type:Observation
Release date:6 October 2004, 18:00
Size:363 x 438 px

About the Object

Name:Kepler's SN
Type:Milky Way : Nebula : Type : Supernova Remnant
Distance:13000 light years
Constellation:Ophiuchus
Category:Nebulae

Image Formats

r.titleLarge JPEG
51.0 KB
r.titleScreensize JPEG
152.2 KB

Coordinates

Position (RA):17 30 37.87
Position (Dec):-21° 28' 44.63"
Field of view:1.85 x 2.23 arcminutes
Orientation:North is 2.9° right of vertical


Colours & filters

BandWavelengthTelescope
Infrared
Near-IR
3.6 μmSpitzer Space Telescope
IRAC
Infrared
Near-IR
4.5 μmSpitzer Space Telescope
IRAC
Infrared
Mid-IR
8.0 μmSpitzer Space Telescope
IRAC

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