Size, mass, and composition At the time of its discovery, Kepler-78b was the exoplanet most similar to Earth in terms of
mass,
radius, and mean
density. The planet is approximately 1.69 times the mass and 1.12 times the radius of Earth. Two independent teams were involved in pioneering work to estimate the planet's mass. Their estimates were made possible because Kepler-78b's gravity causes a "wobble" in the orbit of the host star. While the method has been used to characterize
gas giants, it is difficult to estimate the mass of Earth-sized exoplanets, because their gravity is too weak to produce a visible influence. In this case, the planet's orbit is close enough to its star to produce a detectable effect. to estimate that the planet has a mass 1.86 times that of the Earth and a radius 1.16 times greater. The other, led by Andrew Howard of the
University of Hawaii at Manoa, used data from the High Resolution Eschelle Spectrometer at the
W.M. Keck Observatory in
Hawaii to estimate the mass as 1.69 times that of the Earth and the radius as 1.12 times larger. Both estimates put the planet's density at about , equivalent to Earth's density. This measurement is possibly indicative of a rock-iron composition like Earth's. The iron core could build up to 40% of the planet mass. Due to its extremely close solar orbit, which is about 40 times closer than
Mercury is to the Sun, the planet's surface is estimated to be at a temperature of . ==Origin==