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Supernova remnant G266.2-1.2 (NASA, Chandra, 10/28/13) | by NASA Marshall Space Flight

Sh2-155 o Caldewell 9 Nebulosa de la Caverna

16 of the most jaw-dropping space photos of the year

Comet Lovejoy

Nebulosa de Orión (M 42) a 1350 años luz de la Tierra

A Tidal Galaxy "A previously unsuspected tidal dwarf galaxy candidate appears only in the ultraviolet, indicating the presence of many hot young stars as seen in this cool space Image. IC 4970, the small disk galaxy interacting with NGC 6872, is located above the spiral’s central region. The spiral is 522,000 light-years across from the tip of one outstretched arm to the tip of the other, which makes it about five times the size of our home galaxy, the Milky Way

NGC7129: star-forming region & reflection nebula in Cepheus, about 3000 ly away; stars in this nebula are about 1 Ma old. The red blobs above & below the nebula are Herbig Haro objects, the result of jets of gas streaming away from young stars in the nebula

Jeje,Sideral,Galaxias,Universo,Nubes De Polvo,Las Nubes,Universo Increíble,El Grupo De Árboles,Nebula Cone

IC 1805: The Heart Distance: 7,500 Light Years Located in the Perseus arm of the Galaxy in the constellation Cassiopeia. This is an emission nebula showing glowing gas and darker dust lanes. The nebula is formed by plasma of ionized hydrogen and free electrons. The nebula’s intense red output and its configuration are driven by the radiation emanating from a small group of stars near the nebula’s

Hickson Compact Group 92, taken from Nasa's Hubble Space Telescope. Otherwise known as Stephan's Quintet, refers to a group of five galaxies.