Kepler's equation and eccentric anomaly From the wiki article about eccentric anomaly follows:

$$\cos E = \frac{x}{a}$$
$$\sin E = \frac{y}{b}$$

where E - eccentric anomaly, a - semi-major axis, b - semi-minor axis, P = P(x,y) a point on elleptic orbit. So if you know an E, you can find a position on an orbit:

$$x = a \cos E$$
$$y = b \sin E$$

However, from article on Kepler's eqution follows:

$$x = a (\cos E - e)$$
$$y = b \sin E$$

Please, help to understand why these formaluae differ? I expect them to be the same.
Both formulae are correct. The discrepancy is because the formula from the eccentric anomaly article uses the centre of the ellipse as the origin, but the formula from the Kepler's equation article uses a focus of the ellipse (i.e, the central gravitating body, eg the Sun) as the origin. Note that $c = ae$ is the distance from the ellipse centre to a focus