Highly elliptical orbits are a specific type of orbital path characterized by a significant difference between their closest approach (perigee) and furthest distance (apogee) from the central body they orbit. These orbits have eccentricities greater than 0.5, causing them to appear elongated and stretched, which allows for varying speeds and distances during the orbit. This unique shape can impact gravitational interactions, orbital dynamics, and the behavior of satellites within these paths.
congrats on reading the definition of highly elliptical orbits. now let's actually learn it.