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Resembling a nightmarish beast rearing its head from a crimson sea, this celestial object is actually just a pillar of gas and dust. Called the Cone Nebula (in NGC 2264) - so named because in ground-based images it has a conical shape - this monstrous pillar resides in a turbulent star-forming region.
The barred spiral galaxy NGC 1672, showing up clusters of hot young blue stars along its spiral arms, and clouds of hydrogen gas glowing in red. Delicate curtains of dust partially obscure and redden the light of the stars behind them. NGC 1672's symmetric look is emphasised by the four principal arms, edged by eye-catching dust lanes that extend out from the centre.
The brightly glowing plumes seen in this mage are reminiscent of an underwater scene, with turquoise-tinted currents and nebulous strands reaching out into the surroundings.However, this is no ocean
This image, not unlike a pointillist painting, shows the star-studded centre of the Milky Way towards the constellation of Sagittarius
