The Shape Entropy of Small Bodies
-
Published:2023-02-09
Issue:4
Volume:11
Page:878
-
ISSN:2227-7390
-
Container-title:Mathematics
-
language:en
-
Short-container-title:Mathematics
Author:
Ni Yanshuo1, Zhang He1ORCID, Li Junfeng2, Baoyin Hexi2, Hu Jiaye3
Affiliation:
1. Beijing Institute of Spacecraft System Engineering, Beijing 100094, China 2. School of Aerospace Engineering, Tsinghua University, Beijing 100084, China 3. Aerospace Engineering Consulting (Beijing) Co., Ltd., China Aerospace Academy of Systems Science and Engineering, Beijing 100048, China
Abstract
The irregular shapes of small bodies usually lead to non-uniform distributions of mass, which makes dynamic behaviors in the vicinities of small bodies different to that of planets. This study proposes shape entropy (SE) as an index that compares the shapes of small bodies and spheres to describe the shape of a small body. The results of derivation and calculation of SE in two-dimensional and three-dimensional cases show that: SE is independent of the size of geometric figures but depends on the shape of the figures; the SE difference between a geometric figure and a circle or a sphere, which is the limit of SE value, reflects the difference between this figure and a circle or a sphere. Therefore, the description of shapes of small bodies, such as near-spherical, ellipsoid, and elongated, can be quantitatively described via a continuous index. Combining SE and the original inertia index, describing the shape of small bodies, can define the shapes of small bodies and provide a reasonably simple metric to describe a complex shape that is applicable to generalized discussion and analysis rather than highly detailed work on a specific, unique, polyhedral model.
Funder
National Key R&D Program of China
Subject
General Mathematics,Engineering (miscellaneous),Computer Science (miscellaneous)
Reference45 articles.
1. Shapes, structures, and evolution of small bodies;Zhang;Astrodyn,2021 2. (2022, December 09). IAU2006 General Assembly. Resolution B5: Definition of a Planet in the Solar System. Available online: https://www.iau.org/static/resolutions/Resolution_GA26-5-6.pdf. 3. Gargaud, M., Irvine, W.M., Amils, R., James, H., Pinti, D.L., Quintanilla, J.C., Rouan, D., Spohn, T., Tirard, S., and Viso, M. (2011). Encyclopedia of Astrobiology, Springer. 4. Toward understanding the origin of asteroid geometries-variety in shapes produced by equal-mass impacts;Sugiura;Astron. Astrophys.,2018 5. Orbital dynamics in the vicinity of asteroid 216 Kleopatra;Yu;Astron. J.,2012
|
|