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Geometry of the Huygens—Roche Figure. / Kholshevnikov, K. V.

в: Vestnik St. Petersburg University: Mathematics, Том 52, № 1, 2019, стр. 122-126.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Kholshevnikov, KV 2019, 'Geometry of the Huygens—Roche Figure', Vestnik St. Petersburg University: Mathematics, Том. 52, № 1, стр. 122-126. https://doi.org/10.3103/S1063454119010059

APA

Kholshevnikov, K. V. (2019). Geometry of the Huygens—Roche Figure. Vestnik St. Petersburg University: Mathematics, 52(1), 122-126. https://doi.org/10.3103/S1063454119010059

Vancouver

Kholshevnikov KV. Geometry of the Huygens—Roche Figure. Vestnik St. Petersburg University: Mathematics. 2019;52(1):122-126. https://doi.org/10.3103/S1063454119010059

Author

Kholshevnikov, K. V. / Geometry of the Huygens—Roche Figure. в: Vestnik St. Petersburg University: Mathematics. 2019 ; Том 52, № 1. стр. 122-126.

BibTeX

@article{2d6744057dd94591b52205ff13cdb8b7,
title = "Geometry of the Huygens—Roche Figure",
abstract = "The theory of figures of celestial bodies, which are in the state of hydrostatic equilibrium under the action of pressure, gravitational, and centrifugal forces, took the form of a rigorous mathematical theory in the second part of the 20th century. Fundamental physical laws served as its basis. The Huygens–Roche figure (its total mass is concentrated in the center, while the rotating atmosphere takes the equilibrium form) plays an important role in the theory. Properties of the figure are carefully examined. In particular, it is known that each isobar (surface of equal pressure) itself is one of the three-parameter family of Huygens—Roche surfaces. However, as far as we know, convexity (or its absence) has not been discussed in the literature. Meanwhile, there are non-convex figures between equilibrium ones. In the present paper, we find the curvature of the meridional section of an arbitrary Huygens—Roche figure both in closed form and in the form of a series in powers of the Clairaut parameter, which is basic in the theory of equilibrium figures. We succeeded in proving that the curvature is positive and is bounded away from zero. Hence, every surface of the family of Huygens—Roche figures is convex and has no points of flattening. Moreover, none of the curves on its surface has points of straightening.",
keywords = "curvature of a planar curve, equilibrium figure, gravitational potential, Huygens—Roche figure",
author = "Kholshevnikov, {K. V.}",
note = "Kholshevnikov, K.V. Vestnik St.Petersb. Univ.Math. (2019) 52: 122. https://doi.org/10.3103/S1063454119010059",
year = "2019",
doi = "10.3103/S1063454119010059",
language = "English",
volume = "52",
pages = "122--126",
journal = "Vestnik St. Petersburg University: Mathematics",
issn = "1063-4541",
publisher = "Pleiades Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Geometry of the Huygens—Roche Figure

AU - Kholshevnikov, K. V.

N1 - Kholshevnikov, K.V. Vestnik St.Petersb. Univ.Math. (2019) 52: 122. https://doi.org/10.3103/S1063454119010059

PY - 2019

Y1 - 2019

N2 - The theory of figures of celestial bodies, which are in the state of hydrostatic equilibrium under the action of pressure, gravitational, and centrifugal forces, took the form of a rigorous mathematical theory in the second part of the 20th century. Fundamental physical laws served as its basis. The Huygens–Roche figure (its total mass is concentrated in the center, while the rotating atmosphere takes the equilibrium form) plays an important role in the theory. Properties of the figure are carefully examined. In particular, it is known that each isobar (surface of equal pressure) itself is one of the three-parameter family of Huygens—Roche surfaces. However, as far as we know, convexity (or its absence) has not been discussed in the literature. Meanwhile, there are non-convex figures between equilibrium ones. In the present paper, we find the curvature of the meridional section of an arbitrary Huygens—Roche figure both in closed form and in the form of a series in powers of the Clairaut parameter, which is basic in the theory of equilibrium figures. We succeeded in proving that the curvature is positive and is bounded away from zero. Hence, every surface of the family of Huygens—Roche figures is convex and has no points of flattening. Moreover, none of the curves on its surface has points of straightening.

AB - The theory of figures of celestial bodies, which are in the state of hydrostatic equilibrium under the action of pressure, gravitational, and centrifugal forces, took the form of a rigorous mathematical theory in the second part of the 20th century. Fundamental physical laws served as its basis. The Huygens–Roche figure (its total mass is concentrated in the center, while the rotating atmosphere takes the equilibrium form) plays an important role in the theory. Properties of the figure are carefully examined. In particular, it is known that each isobar (surface of equal pressure) itself is one of the three-parameter family of Huygens—Roche surfaces. However, as far as we know, convexity (or its absence) has not been discussed in the literature. Meanwhile, there are non-convex figures between equilibrium ones. In the present paper, we find the curvature of the meridional section of an arbitrary Huygens—Roche figure both in closed form and in the form of a series in powers of the Clairaut parameter, which is basic in the theory of equilibrium figures. We succeeded in proving that the curvature is positive and is bounded away from zero. Hence, every surface of the family of Huygens—Roche figures is convex and has no points of flattening. Moreover, none of the curves on its surface has points of straightening.

KW - curvature of a planar curve

KW - equilibrium figure

KW - gravitational potential

KW - Huygens—Roche figure

UR - http://www.scopus.com/inward/record.url?scp=85064906004&partnerID=8YFLogxK

UR - https://link.springer.com/article/10.3103/S1063454119010059

U2 - 10.3103/S1063454119010059

DO - 10.3103/S1063454119010059

M3 - Article

AN - SCOPUS:85064906004

VL - 52

SP - 122

EP - 126

JO - Vestnik St. Petersburg University: Mathematics

JF - Vestnik St. Petersburg University: Mathematics

SN - 1063-4541

IS - 1

ER -

ID: 50000171