Tracking neighboring quasi-satellite orbits around Phobos

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

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

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Numerical integration of satellite orbits around an oblate planet

A recurrent power series (RPS) method is constructed for the numerical integration of the equations of motion of a planet and its N satellites. The planet is considered as an oblate spheroid with the oblateness potential calculated up to the factor J4. The efficiency of the RPS method in terms of accuracy and speed is compared to that of the commonly used 10th-order Gauss-Jackson backward diffe...

متن کامل

Martian satellite orbits and ephemerides

We discuss the general characteristics of the orbits of the Martian satellites, Phobos and Deimos. We provide a concise review of the various descriptions of the orbits by both analytical theories and direct numerical integrations of their equations of motion. After summarizing the observational data used to determine the orbits, we discuss the results of our latest orbits obtained from a least...

متن کامل

Satellite Orbits Based Sky Search

The fast evolution of GNSS based applications makes it necessary the development of accurate and efficient navigation systems. The GPS usually adopts a two level strategy for position estimation: Coarse Acquisition of the PRN code, and fine tracking. In the so called “cold start” state, i.e. initialization without almanac data, coarse acquisition is a three dimensional search process of code, c...

متن کامل

Orbits in a Neighboring Dwarf Galaxy According to MOND

We study the orbits in the MOND theory within a dwarf galaxy of mass Md ∼ 108M⊙ at a distance of ∼ 100kpc from a neighboring galaxy of mass Mg = 5 × 1011M⊙, such as ours. It is assumed that a second mass m << Md is gravitationally bound to Md by a previously calculated potential for the MOND theory. This potential is obtained for a free falling mass Md in a constant external gravitational accel...

متن کامل

Bound near-equatorial orbits around neutron stars

Recent discovery of kilohertz quasi-periodic brightness oscillations of low mass X-ray binaries (LMXBs) has attracted attention to highly relativistic periodic motion near accreting neutron stars. Most models proposed so far involve (almost) inertial motion in the vicinity of the stars’ innermost stable circular orbits. In the present paper we study general-relativistic circular and eccentric o...

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

ژورنال

عنوان ژورنال: IFAC-PapersOnLine

سال: 2020

ISSN: 2405-8963

DOI: 10.1016/j.ifacol.2020.12.1952