For Researchers · Hubble's Law
Hubble's Law for a binary star
Built for researchers prototyping or validating an idea. Prototype fast, reproduce exactly, and share a citable, interactive version of your model. Simulate a binary star live below — adjust the inputs and watch it respond, right in your browser.
Hubble's Law & RedshiftLive
the expanding universe
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Every distant galaxy recedes at a velocity proportional to its distance: v = H₀·d. This uniform expansion is the same seen from any galaxy — there is no center. The inverse of H₀ gives the Hubble time, a rough estimate of the age of the universe.
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H₀70 km/s/Mpc
Hubble time14.0 Gyr
v at 100 Mpc7,000 km/s
Governing equation
Reading this result: Right in the Hubble-tension zone: this H₀ gives a Hubble time of 14.0 Gyr, close to the measured 13.8-Gyr age of the universe.
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- Yes — this version of "Hubble's Law for a binary star" is framed for researchers prototyping or validating an idea. Prototype fast, reproduce exactly, and share a citable, interactive version of your model.
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