Tilting Saturn. I. Analytic Model

نویسندگان

  • William R. Ward
  • Douglas P. Hamilton
چکیده

The tilt of Saturn’s spin axis to its orbit plane is 26N7, while that of Jupiter is only 3N1. We offer an explanation for this puzzling difference owing to gravitational perturbations of Saturn by the planet Neptune. A similarity between the precession period of Saturn’s spin axis and the 1:87 ; 10 yr precession period of Neptune’s slightly inclined orbit plane implicates a resonant interaction between these planets as responsible for tilting Saturn from an initially more upright state. We make a case that Saturn was captured into this resonance during the erosion of the Kuiper belt , which decreased the rate of regression of Neptune’s orbit plane. Penetrating the resonance pumped up Saturn’s obliquity to its current value. The spin axis may also be librating in the resonance with an amplitude k31 , and we discuss possible causes of this and the implied constraint on Saturn’s moment of inertia. Matching the current pole position to the predicted outcome could place constraints on early solar system processes.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Tilting Saturn. Ii. Numerical Model

We argue that the gas giants Jupiter and Saturn were both formed with their rotation axes nearly perpendicular to their orbital planes, and that the large current tilt of the ringed planet was acquired in a post-formation event. We identify the responsible mechanism as trapping into a secular spin-orbit resonance that couples the angular momentum of Saturn’s rotation to that of Neptune’s orbit....

متن کامل

Nonuniform viscosity in the solar nebula and large masses of Jupiter and Saturn

I report a novel theory that nonuniform viscous frictional force in the solar nebula accounts for the largest mass of Jupiter and Saturn and their largest amount of H and He among the planets, two outstanding facts that are unsolved puzzles in our understanding of origin of the Solar System. It is shown that the nebula model of uniform viscosity does not match the present planet masses. By stud...

متن کامل

Titan in subsonic and supersonic flow

[1] The Titan-Saturn plasma interaction is studied using a global numerical kinetic model. The developed selfconsistent three-dimensional quasi-neutral hybrid model is used to study Titan’s interaction with supersonic and subsonic plasma flow. The subsonic flow case represents Titan in the Kronian magnetosphere during the Voyager-1 flyby. The supersonic and weakly supermagnetosonic flow cases a...

متن کامل

Seven armed, elephant-legged Shapour or Saturn? (Study an Image in Iskandarnāma Naghali(1856-57AD)

Iskandarnāma Naghali as the last version of Alexander’s story in the Safavid era, which was republished and illustrated in Qajar dynasty, became one of the most popular folk tales of that time. The story of Alexander has got a special place among folkloric literature due to the various versions of its in prose and poetry and numerous narratives of it in Greek, Pahlavi, Farsi and so on. Thus, th...

متن کامل

Tetrahedral Mechanism Crawling on a Slope

Crawling mechanisms with energetic and control autonomy may move and steer by sliding on the ground. The paper presents an analytic and MBS simulation study on the possibilities and limits of steering a tetrahedral mechanism on a slope. The mechanism movement is analyzed using an equivalent 3d model. The analysis is structural, kinematical, static and dynamic. The limit conditions for stability...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2004