Hubble constant = 70 km/s/Mpc = 2.3×10−18s−1
{"title":"The speed at which a distant galaxy moves away from us...","description":"Wrong","type":"incorrect","color":"#99CCFF","code":"[{\"shape\":\"poly\",\"coords\":\"82,133\"},{\"shape\":\"rect\",\"coords\":\"10,16,12,16\"},{\"shape\":\"poly\",\"coords\":\"144,22\"},{\"shape\":\"rect\",\"coords\":\"1,18,30,56\"}]"} {"title":"...is directly proportional to its distance from us.","description":"Wrong","type":"incorrect","color":"#ffff00","code":"[{\"shape\":\"rect\",\"coords\":\"166,7,194,54\"}]"} {"title":"Hubble constant = 70 km/s/Mpc = 2.3 × 10 sup −18 s sup −1","description":"Correct!","type":"correct","color":"#00ff00","code":"[{\"shape\":\"rect\",\"coords\":\"93,9,142,56\"}]"}This direct proportionality is called the Hubble law, and the constant H0 in Equation 28-9 is called the Hubble constant. Astronomers typically measure distances in the cosmos in parsecs (pc), a unit equal to 3.26 light-years. One light-year (ly) is the distance that light travels in one year, equal to 3.09×1016m. The current best value of H0 is about 70 km / s / Mpc, where 1 Mpc = 1 megaparsec = 106 pc=3.26×106 ly.