The Crab Nebula M1 NGC 1952 Taurus A Personalized Photo Card

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 observed by John Bevis in 1731; it corresponds to a bright supernova recorded by Chinese and Arab astronomers in 1054. At X-ray and gamma-ray energies above 30 keV, the Crab is generally the strongest persistent source in the sky, with measured flux extending to above 1012 eV. 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 kilometers per second. It is part of the Perseus Arm of the Milky Way Galaxy.

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Share your special moments with loved ones everywhere. Create your photo card from scratch or customize any existing template for free. Add custom postage for an even more personal touch!

4” x 8” (portrait) or 8” x 4” (landscape).
Printed on ultra-heavyweight (120 lb.) card stock with a gloss finish.
High quality, full-color, full-bleed printing.
Photo cards come with white #10 envelopes.
Postage rate for a photo card (up to 1 oz) is $0.45

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The Crab Nebula M1 NGC 1952 Taurus A Personalized Photo Card

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The Crab Nebula M1 NGC 1952 Taurus A

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 observed by John Bevis in 1731; it corresponds to a bright supernova recorded by Chinese and Arab astronomers in 1054. At X-ray and gamma-ray energies above 30 keV, the Crab is generally the strongest persistent source in the sky, with measured flux extending to above 1012 eV. 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 kilometers per second. It is part of the Perseus Arm of the Milky Way Galaxy.

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