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Hubble's Cepheid Variable in M31, Bruce Van Deventer

Hubble's Cepheid Variable in M31

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Hubble's Cepheid Variable in M31, Bruce Van Deventer

Hubble's Cepheid Variable in M31

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Description

Hubble's Cepheid Variable was the first of a number of Cepheid variable stars discovered by Edwin Hubble, using the 100 inch Hooker telescope on Mt. Wilson, and which proved that "spiral nebulae" are galaxies outside of our own and not spinning clouds of gas and dust within our own galaxy. It's about 19th magnitude. Cepheids are extremely luminous stars which is why they can be seen as individual stars even in other galaxies. It's pretty amazing that an amateur telescope can image this star in a three minute exposure. Imaged at Burnt Tree Hill observatory in Cle Elum, Washington. The image on the right is the full frame image, on the left lower is a negative enlagement with concentric rings around the star and above is a screenshot from Aladin Lite of the star from DSS2.

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Hubble's Cepheid Variable in M31, Bruce Van Deventer