On the Orbital Periods for a Particular Case of Spherical Symmetry

A particular case of steady state and spherical symmetry - the so-called logarithmic potential introduced as the first approximation for dark coronae of galaxies - is studied. Both time and angle dependence of the distance to the centre for the orbit of a bound test particle with arbitrary initial...

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Main Authors: Ninković, S., Jovanović, B.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2008-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://saj.matf.bg.ac.rs/176/pdf/045-049.pdf
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author Ninković, S.
Jovanović, B.
author_facet Ninković, S.
Jovanović, B.
author_sort Ninković, S.
collection DOAJ
description A particular case of steady state and spherical symmetry - the so-called logarithmic potential introduced as the first approximation for dark coronae of galaxies - is studied. Both time and angle dependence of the distance to the centre for the orbit of a bound test particle with arbitrary initial conditions are calculated numerically. The main attention is paid to the ratio of the sidereal period to the anomalistic one. It is found that this ratio is only slightly variable for a given mean distance to the centre and to increase with increasing orbital eccentricity. This quantitative result may be explained by the fact that the cumulative mass dependence on the distance corresponding to the logarithmic potential obeys a power law, the case where the ratio of the second derivative of the potential to the square of angular velocity for the same distance is constant. On the other hand, compared to the period of circular motion both periods increase with increasing eccentricity.
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spelling doaj.art-6061948aa0144947a9d7448e54838f192022-12-22T01:42:39ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X2008-01-011764549On the Orbital Periods for a Particular Case of Spherical SymmetryNinković, S.Jovanović, B.A particular case of steady state and spherical symmetry - the so-called logarithmic potential introduced as the first approximation for dark coronae of galaxies - is studied. Both time and angle dependence of the distance to the centre for the orbit of a bound test particle with arbitrary initial conditions are calculated numerically. The main attention is paid to the ratio of the sidereal period to the anomalistic one. It is found that this ratio is only slightly variable for a given mean distance to the centre and to increase with increasing orbital eccentricity. This quantitative result may be explained by the fact that the cumulative mass dependence on the distance corresponding to the logarithmic potential obeys a power law, the case where the ratio of the second derivative of the potential to the square of angular velocity for the same distance is constant. On the other hand, compared to the period of circular motion both periods increase with increasing eccentricity.http://saj.matf.bg.ac.rs/176/pdf/045-049.pdfStellar dynamics
spellingShingle Ninković, S.
Jovanović, B.
On the Orbital Periods for a Particular Case of Spherical Symmetry
Serbian Astronomical Journal
Stellar dynamics
title On the Orbital Periods for a Particular Case of Spherical Symmetry
title_full On the Orbital Periods for a Particular Case of Spherical Symmetry
title_fullStr On the Orbital Periods for a Particular Case of Spherical Symmetry
title_full_unstemmed On the Orbital Periods for a Particular Case of Spherical Symmetry
title_short On the Orbital Periods for a Particular Case of Spherical Symmetry
title_sort on the orbital periods for a particular case of spherical symmetry
topic Stellar dynamics
url http://saj.matf.bg.ac.rs/176/pdf/045-049.pdf
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