<P> For Earth, orbital eccentricity ≈ 0.0167, apoapsis = aphelion = apogee and periapsis = perihelion = perigee relative to sun . </P> <P> For Earth's annual orbit path, r / r ratio = longest_radius / shortest_radius ≈ 1.034 relative to center point of path . </P> <Table> Eccentricities of Solar System bodies <Tr> <Th> Object </Th> <Th> eccentricity </Th> </Tr> <Tr> <Td> Triton </Td> <Td> 0.00002 </Td> </Tr> <Tr> <Td> Venus </Td> <Td> 0.0068 </Td> </Tr> <Tr> <Td> Neptune </Td> <Td> 0.0086 </Td> </Tr> <Tr> <Td> Earth </Td> <Td> 0.0167 </Td> </Tr> <Tr> <Td> Titan </Td> <Td> 0.0288 </Td> </Tr> <Tr> <Td> Uranus </Td> <Td> 0.0472 </Td> </Tr> <Tr> <Td> Jupiter </Td> <Td> 0.0484 </Td> </Tr> <Tr> <Td> Saturn </Td> <Td> 0.0541 </Td> </Tr> <Tr> <Td> Moon </Td> <Td> 0.0549 </Td> </Tr> <Tr> <Td> 1 Ceres </Td> <Td> 0.0758 </Td> </Tr> <Tr> <Td> 4 Vesta </Td> <Td> 0.0887 </Td> </Tr> <Tr> <Td> Mars </Td> <Td> 0.0934 </Td> </Tr> <Tr> <Td> 10 Hygiea </Td> <Td> 0.1146 </Td> </Tr> <Tr> <Td> Makemake </Td> <Td> 0.1559 </Td> </Tr> <Tr> <Td> Haumea </Td> <Td> 0.1887 </Td> </Tr> <Tr> <Td> Mercury </Td> <Td> 0.2056 </Td> </Tr> <Tr> <Td> 2 Pallas </Td> <Td> 0.2313 </Td> </Tr> <Tr> <Td> Pluto </Td> <Td> 0.2488 </Td> </Tr> <Tr> <Td> 3 Juno </Td> <Td> 0.2555 </Td> </Tr> <Tr> <Td> 324 Bamberga </Td> <Td> 0.3400 </Td> </Tr> <Tr> <Td> Eris </Td> <Td> 0.4407 </Td> </Tr> <Tr> <Td> Nereid </Td> <Td> 0.7507 </Td> </Tr> <Tr> <Td> Sedna </Td> <Td> 0.8549 </Td> </Tr> <Tr> <Td> Halley's Comet </Td> <Td> 0.9671 </Td> </Tr> <Tr> <Td> Comet Hale - Bopp </Td> <Td> 0.9951 </Td> </Tr> <Tr> <Td> Comet Ikeya - Seki </Td> <Td> 0.9999 </Td> </Tr> </Table> <Tr> <Th> Object </Th> <Th> eccentricity </Th> </Tr>

Which two planets of our solar system have the most eccentric orbits