Earth Mean Orbital Speed

v⊕=29,780 m/sv_\oplus = 29,780\ \text{m/s}
Value29,780 m/s
StatusConventional / typical value
SourceNASA planetary fact sheet (mean orbital velocity)
CategoriesAstronomical
Earth Mean Orbital Speed in every speed unit
millimeter per year939,785,330,000,000 mm/yr
millimeter per day2,572,992,000,000 mm/day
millimeter per hour107,208,000,000 mm/h
inch per day101,298,900,000 in/day
foot per day8,441,574,800 ft/d
inch per hour4,220,787,400 in/h
meter per day2,572,992,000 m/d
millimeter per minute1,786,800,000 mm/min
meter per hour107,208,000 m/h
inch per minute70,346,457 in/min
millimeter per second29,780,000 mm/s
foot per minute5,862,204.7 ft/min
centimeter per second2,978,000 cm/s
meter per minute1,786,800 m/min
inch per second1,172,440.9 in/s
kilometer per hour107,208 km/h
foot per second97,703.412 ft/s
mile per hour66,615.963 mph
knot57,887.689 kn
meter per second29,780 m/s
mach (sea level)87.512563 Ma
kilometer per second29.78 km/s
speed of light0.000099335388 c

Learning zone

Take the orbit's circumference and divide by the year: about 940 million kilometres in 31.56 million seconds, near 29.8 km/s. Kepler's second law means it is not constant — Earth moves at 30.29 km/s at perihelion in early January and 29.29 km/s at aphelion in early July, which is why the northern summer half-year is a few days longer than the southern one.

The number has a distinguished experimental history. Bradley discovered stellar aberration in 1728 because starlight appears tilted by v/c ≈ 20.5 arcseconds as Earth swings around, giving the first direct proof of Earth's motion and an early value for the speed of light. A century and a half later Michelson and Morley looked for the effect of the same 30 km/s on the speed of light itself, found nothing, and set relativity in motion.