Astronomers have used a different sort of distance indicator -- not Cepheids -- to measure the distance to the Coma cluster of galaxies. They find for the galaxy NGC 4489 a distance modulus (m-M) = 34.64 +/- 0.25. Spectra of the galaxy show that the hydrogen Balmer-alpha line appears at 672 nm instead of its rest wavelength of 656 nm. a) What is the distance to NGC 4489 based on this distance modulus? (m - M) = 5 log d - 5 [(m - M) + 5] / 5 ----> d = 10 [ 34.64 + 5] / 5 = 10 7.928 = 10 = 85,000,000 pc approx = 85 Mpc b) What is the radial velocity of this galaxy? We can use the Doppler formula to find the radial velocity: shift in wavelength speed = --------------------- * c rest wavelength (672 nm - 656 nm) = ------------------- * (300,00 km/s) 656 nm = 7300 km/s approx c) Add this galaxy to your Hubble diagram. What value for the Hubble constant do you derive now? The Hubble diagram now stretches from about 0 Mpc to 85 Mpc, and from 0 km/s to 7300 km/s. If we draw a line from the origin to this galaxy alone -- which passes close to many of the other galaxies -- we find a slope of (7300 km/s - 0 km/s) Hubble const = ----------------------- ( 85 Mpc - 0 Mpc ) 86 km/s = ---------- Mpc