Hubble identifies unusual wrinkle in expansion rate of the universe

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Measuring the expansion rate of the universe was one of the Hubble Space Telescope's main goals when it was launched in 1990. Over the past 30 years, the space observatory has helped scientists discover and refine that accelerating rate -- as well as uncover a mysterious wrinkle that only brand-new physics may solve.

A collection of images from the NASA/ESA Hubble Space Telescope features galaxies that are all hosts to both Cepheid variables and supernovae. via CNN)

Hubble has observed more than 40 galaxies that include pulsating stars as well as exploding stars called supernovae to measure even greater cosmic distances. Both of these phenomena help astronomers to mark astronomical distances like mile markers, which have pointed to the expansion rate. Scientists don't understand the discrepancy, but acknowledge that it's weird and could require new physics.

Hubble relied on the work of astronomer Henrietta Swan Leavitt's 1912 discovery of the periods of brightness in pulsating stars called Cepheid variables. Cepheids act like cosmic mile markers as they brighten and dim periodically within our galaxy and others. Multiple teams of astronomers using the Hubble telescope have arrived at a Hubble constant value that equals 73 plus or minus 1 kilometre per second per megaparsec.

Planck, another space observatory, was used to measure the cosmic microwave background, or the leftover radiation from the big bang 13.8 billion years ago.

 

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