Hubble law describes how the speed of recession of distant galaxies varies with the distan from Earth v = Hod, Ho 2.3 x 10-18 [s-1] Estimate the distance of an object when it moves very close to the speed of light c = 3.00 x 108 [m/s] relative to Earth.
Hubble law describes how the speed of recession of distant galaxies varies with the distan from Earth v = Hod, Ho 2.3 x 10-18 [s-1] Estimate the distance of an object when it moves very close to the speed of light c = 3.00 x 108 [m/s] relative to Earth.
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![Hubble law describes how the speed of recession of distant galaxies varies with the distance
from Earth
v = Hod,
Ho = 2.3 × 10-18 [s-1]
Estimate the distance of an object when it moves very close to the speed of light c =
3.00 x 108 [m/s] relative to Earth.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F0c392c8a-5be0-4b48-b8a1-b69c885559a8%2Fe4ae8761-b271-4336-8262-6f80c88e7767%2Fdelaw6j_processed.png&w=3840&q=75)
Transcribed Image Text:Hubble law describes how the speed of recession of distant galaxies varies with the distance
from Earth
v = Hod,
Ho = 2.3 × 10-18 [s-1]
Estimate the distance of an object when it moves very close to the speed of light c =
3.00 x 108 [m/s] relative to Earth.
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