Answer:Hermes is not a planet in our solar system; it's actually an asteroid. Given that information, let's compare the eccentricity of Hermes' orbit to the orbits of the planets.
Eccentricity is a measure of how elliptical (non-circular) an orbit is. The eccentricity of an orbit ranges from 0 (perfectly circular) to 1 (highly elliptical).
The orbits of the planets in our solar system are generally quite close to being circular, with eccentricities very close to 0. For example, the eccentricity of Earth's orbit is approximately 0.017, which is very close to a perfect circle. The orbits of most planets in our solar system have similarly low eccentricities.
In contrast, an eccentricity of 0.62, as you mentioned for Hermes, is relatively high. This means that Hermes' orbit is significantly more elliptical (less circular) compared to the orbits of the planets in our solar system. An eccentricity of 0.62 would indicate a noticeably elongated and non-circular orbit.
So, to answer your question, Hermes has a more eccentric (less circular) orbit than the planets in our solar system. This is typical for many asteroids, comets, and other small celestial bodies, which often have more elongated and eccentric orbits compared to the larger planets.