I have a question that I'm hoping someone can answer for me. Is it possible, in reality, to have a body with an orbit that is both highly eccentric and tidally locked?
I don't have a great understanding of orbital mechanics, just what I have taught myself, but my understanding makes me think this isn't really possible. My understanding of tidal locking is that the same side of a given body always faces the parent body meaning the time it takes to complete one orbit is equal to the time it takes to complete one rotation and in my mind that could only be possible with orbits that are petty much circular. A highly eccentric orbit means that it is very elliptical as opposed to a more circular orbit. This would mean that the orbital velocity at the apogee is much lower than at the perigee. In order to have a planet that is tidally locked in an eccentric orbit would mean that the rotational speed would have to vary greatly from one end of the orbit to the other which, as far as I know, is not possible. Is there something wrong with my understanding of that? If so please correct me! I'm always looking to improve my knowledge of these things.
I ask because I found a WW that is both tidally locked and while it's not highly eccentric it is a bit more eccentric that I would think is possible for something to be tidally locked with my limited knowledge of the subject. The WW has an orbit of 250 days with an eccentricity of 0.15xx (again, I know that's not highly eccentric but it made me start to think about it). I did a quick search on the ol' Google but found some conflicting answers, as one would expect. I'm also sure this happens a lot in ED but I just happened to notice this particular body due to how out of place it seemed with the rest of the system it was in which is why I took a closer look at the stats.
I don't have a great understanding of orbital mechanics, just what I have taught myself, but my understanding makes me think this isn't really possible. My understanding of tidal locking is that the same side of a given body always faces the parent body meaning the time it takes to complete one orbit is equal to the time it takes to complete one rotation and in my mind that could only be possible with orbits that are petty much circular. A highly eccentric orbit means that it is very elliptical as opposed to a more circular orbit. This would mean that the orbital velocity at the apogee is much lower than at the perigee. In order to have a planet that is tidally locked in an eccentric orbit would mean that the rotational speed would have to vary greatly from one end of the orbit to the other which, as far as I know, is not possible. Is there something wrong with my understanding of that? If so please correct me! I'm always looking to improve my knowledge of these things.
I ask because I found a WW that is both tidally locked and while it's not highly eccentric it is a bit more eccentric that I would think is possible for something to be tidally locked with my limited knowledge of the subject. The WW has an orbit of 250 days with an eccentricity of 0.15xx (again, I know that's not highly eccentric but it made me start to think about it). I did a quick search on the ol' Google but found some conflicting answers, as one would expect. I'm also sure this happens a lot in ED but I just happened to notice this particular body due to how out of place it seemed with the rest of the system it was in which is why I took a closer look at the stats.