More deep sky images taken using a Dwarf3 smart scope

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A super selection of deep sky images taken by member George Buckberry using a Dwarf3 smart scope on the 3rd & 5th January 2026.

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The Crab Nebula (catalogue designations M1NGC 1952Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. Ref:https://en.wikipedia.org/wiki/Crab_Nebula

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A close up of the Crab Nebula.

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The Triangulum Galaxy is a spiral galaxy 2.878 million light-years (ly) from Earth  in the constellation Triangulum. It is catalogued as Messier 33 or NGC 598. The Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way. Ref:https://en.wikipedia.org/wiki/Triangulum_Galaxy

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Bode's Galaxy (also known as NGC 3031 or Messier 81) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. Ref:https://en.wikipedia.org/wiki/Messier_81

The galaxy above it (centre top of image) is the Cigar Galaxy also known as Messier 82.

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The Rosette Nebula (also known as Caldwell 49) is an H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. Ref: https://en.wikipedia.org/wiki/Rosette_Nebula

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The Elephant's Trunk Nebula (IC 1396A) is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light-years away from Earth. Ref:https://en.wikipedia.org/wiki/Elephant%27s_Trunk_Nebula

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The Crab Nebula, M1, NGC1952

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The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus.

The nebula was first observed by John Bevis, and corresponds to a bright supernova recorded by Chinese and Arab astronomers in 1054. Located at a distance of about 6,500 light-years (2 kpc) from Earth, the nebula has a diameter of 11 ly (3.4 pc) and expands at a rate of about 1,500 kilometres per second.

At the centre of the nebula lies the Crab Pulsar, a rotating neutron star, which emits pulses of radiation from gamma rays to radio waves with a spin rate of 30.2 times per second. The nebula was the first astronomical object identified with a historical supernova explosion.

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Images by Simon Dawes

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Messier 1 SD01

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Images by Kevin Langford

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M1 Crab cropped KL

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M1 KL Crab

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Images by Keith Rickard

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M1_KR1

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Images By Julian Tworek

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m1_jt01

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M1_20110108JT

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Images by Andrew Wilson

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m1_aw01

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