Tangled — cosmic edition
This dark, tangled web is an object named SNR 0454-67.2. It formed in a very violent fashion — it is a supernova remnant, created after a massive star ended its life in a cataclysmic explosion and threw its constituent material out into surrounding space. This created the messy formation we see in this NASA/ESA Hubble Space Telescope image, with threads of red snaking amidst dark, turbulent clouds.
SNR 0454-67.2 is situated in the Large Magellanic Cloud, a dwarf spiral galaxy that lies close to the Milky Way. The remnant is likely the result of a Type Ia supernova explosion; this category of supernovae is formed from the death of a white dwarf star, which grows and grows by siphoning material from a stellar companion until it reaches a critical mass and then explodes.
As they always form via a specific mechanism — when the white dwarf hits a particular mass — these explosions always have a well-known luminosity, and are thus used as markers (standard candles) for scientists to obtain and measure distances throughout the Universe.
Credit:ESA/Hubble, NASA
About the Image
| Id: | potw1848a | 
|---|---|
| Type: | Observation | 
| Release date: | 26 November 2018, 06:00 | 
| Size: | 3945 x 4165 px | 
About the Object
| Name: | SNR 0454-67.2 | 
|---|---|
| Type: | Local Universe : Nebula : Type : Supernova Remnant | 
| Distance: | 163000 light years | 
| Constellation: | Dorado | 
| Category: | Nebulae | 
Image Formats
Wallpapers
Coordinates
| Position (RA): | 4 54 31.32 | 
|---|---|
| Position (Dec): | -67° 12' 55.72" | 
| Field of view: | 2.60 x 2.75 arcminutes | 
| Orientation: | North is 185.5° left of vertical | 
Colours & filters
| Band | Wavelength | Telescope | 
|---|---|---|
| Optical G | 475 nm | Hubble Space Telescope WFC3 | 
| Optical V | 555 nm | Hubble Space Telescope WFC3 | 
| Optical H-alpha | 656 nm | Hubble Space Telescope WFC3 | 
| Optical I | 814 nm | Hubble Space Telescope WFC3 | 
 
    



