Abstract
An analytical gravity modeling formulation for heterogeneous bodies is developed in this paper, in which the compact closed formulation of gravitational potential and attraction is derived analytically. Using linear-interpolated density over finite element meshes, the formulation shows global convergence and consistent reliability in both exterior and interior, and on the interface. The contribution caused by arbitrary non-spherical shape and non-uniform mass distribution is considered separately in this method, which brings natural flexibility to gravity modeling. Benchmark tests are performed to verify the global convergence and reliability. A typical application to asteroid (25143) Itokawa is shown at the end of this paper, which proves the capacity and reliability of this method in gravity modeling of a practical irregularly-shaped heterogeneous asteroid.
Similar content being viewed by others
Data Availability
All data used in this article are publicly accessible. High-resolution shape model of Itokawa can be obtained in NASA Planetary Data System.
References
Abe S, Mukai T, Hirata N, Barnouin-Jha OS, Cheng AF, Demura H, Gaskell RW, Hashimoto T, Hiraoka K, Honda T, Kubota T, Yoshikawa M (2006) Mass and local topography measurements of Itokawa by Hayabusa. Science 312(5778):1344–1347. https://doi.org/10.1126/science.1126272
Conway JT (2015) Analytical solution from vector potentials for the gravitational field of a general polyhedron. Celest Mech Dyn Astron 121(1):17–38. https://doi.org/10.1007/s10569-014-9588-x
D’Urso MG (2014a) Analytical computation of gravity effects for polyhedral bodies. J Geod 88(1):13–29. https://doi.org/10.1007/s00190-013-0664-x
D’Urso MG (2014b) Gravity effects of polyhedral bodies with linearly varying density. Celest Mech Dyn Astron 120(4):349–372. https://doi.org/10.1007/s10569-014-9578-z
D’Urso MG, Trotta S (2017) Gravity anomaly of polyhedral bodies having a polynomial density contrast. Surv Geophys 38(4):781–832. https://doi.org/10.1007/s10712-017-9411-9
Eriguchi Y, Hachisu I, Sugimoto D (1982) Dumb-bell-shape equilibria and mass-shedding pear-shape of self gravitating incompressible fluid. Prog Theor Phys 67(4):1068–1075. https://doi.org/10.1143/PTP.67.1068
Ermakov AI, Zuber MT, Smith DE, Raymond CA, Balmino G, Fu RR, Ivanov BA (2014) Constraints on Vesta’s interior structure using gravity and shape models from the Dawn mission. Icarus 240:146–160. https://doi.org/10.1016/j.icarus.2014.05.015
Fujiwara A, Kawaguchi J, Yeomans DK, Abe M, Mukai T, Okada T, Uesugi K (2006) The rubble-pile asteroid Itokawa as observed by Hayabusa. Science 312(5778):1330–1334. https://doi.org/10.1126/science.1125841
Fukushima T (2017) Precise and fast computation of the gravitational field of a general finite body and its application to the gravitational study of asteroid eros. Astron J 154(4):145. https://doi.org/10.3847/1538-3881/aa88b8
Gaskell R et al (2008) Gaskell Itokawa shape model V1.0. HAY-A-AMICA-5-ITOKAWASHAPE-V1.0. NASA planetary data system
Hansen RO (1999) An analytical expression for the gravity field of a polyhedral body with linearly varying density. Geophysics 64(1):75–77. https://doi.org/10.1190/1.1444532
Hofmann-Wellenhof B, Moritz H (2006) Physical geodesy. Springer, Berlin
Holstein H (2003) Gravimagnetic anomaly formulas for polyhedra of spatially linear media. Geophysics 68(1):157–167. https://doi.org/10.1190/1.1543203
Jänich K, Kay L (2001) Vector analysis. Springer, Berlin
Jiang Y, Baoyin HX (2016) Periodic orbit families in the gravitational field of irregular-shaped bodies. Astron J 152(5):137. https://doi.org/10.3847/0004-6256/152/5/137
Lowry SC, Weissman PR, Duddy SR, Rozitis B, Fitzsimmons A, Green SF, van Oers P (2014) The internal structure of asteroid (25143) Itokawa as revealed by detection of YORP spin-up. A &A 562:A48. https://doi.org/10.1051/0004-6361/201322602
Petrović S (1996) Determination of the potential of homogeneous polyhedral bodies using line integrals. J Geod 71(1):44–52. https://doi.org/10.1007/s001900050074
Romain G, Jean-Pierre B (2001) Ellipsoidal Harmonic expansions of the gravitational potential: theory and application. Celest Mech Dyn Astron 79(4):235–275. https://doi.org/10.1023/a:1017555515763
Scheeres D, Gaskell R, Abe S, Barnouin-Jha O, Hashimoto T, Kawaguchi J, Hirata N (2006) The actual dynamical environment about Itokawa. In: Paper presented at the AIAA/AAS astrodynamics specialist conference and exhibit
Scheeres DJ, French AS, Tricarico P, Chesley SR, Takahashi Y, Farnocchia D, McMahon JW, Brack DN, Davis AB, Ballouz RL, Jawin ER, Lauretta DS (2020) Heterogeneous mass distribution of the rubble-pile asteroid (101955) Bennu. Sci Adv 6(41):eabc3350. https://doi.org/10.1126/sciadv.abc3350
Tsoulis D (2012) Analytical computation of the full gravity tensor of a homogeneous arbitrarily shaped polyhedral source using line integrals. Geophysics 77(2):F1–F11. https://doi.org/10.1190/geo2010-0334.1
Tsoulis D, Petrović S (2001) On the singularities of the gravity field of a homogeneous polyhedral body. Geophysics 66(2):535–539. https://doi.org/10.1190/1.1444944
Wei B, Shang H (2021) Global gravity field modeling of small bodies with heterogeneous mass distributions. J Guid Control Dyn 10(2514/1):G005945
Werner RA (1994) The gravitational potential of a homogeneous polyhedron or don’t cut corners. Celest Mech Dyn Astron 59(3):253–278. https://doi.org/10.1007/bf00692875
Werner RA, Scheeres DJ (1996) Exterior gravitation of a polyhedron derived and compared with harmonic and mascon gravitation representations of asteroid 4769 Castalia. Celest Mech Dyn Astron 65(3):313–344
Wittick PT, Russell RP (2017) Mascon models for small body gravity fields. In: Paper presented at the AAS/AIAA astrodynamics specialist conference
Wittick P, Russell R (2018) Hybrid gravity models for Kleopatra, Itokawa, and Comet 67P/C-G. In: AAS/AIAA astrodynamics specialist conference (18)
Yu Y (2016) Orbital dynamics in the gravitational field of small bodies. Springer, Berlin
Yu Y, Michel P, Hirabayashi M, Schwartz SR, Zhang Y, Richardson DC, Liu X (2018) The dynamical complexity of surface mass shedding from a top-shaped asteroid near the critical spin limit. Astron J 156(2):59. https://doi.org/10.3847/1538-3881/aaccf7
Yu Y, Cheng B, Hayabayashi M, Michel P, Baoyin H (2019) A finite element method for computational full two-body problem: I. The mutual potential and derivatives over bilinear tetrahedron elements. Celest Mech Dyn Astron 131(11):51. https://doi.org/10.1007/s10569-019-9930-4
Acknowledgements
The authors acknowledge financial support provided by the National Natural Science Foundation of China Grant Nos. 12022212 and 11872223.
Author information
Authors and Affiliations
Contributions
YY, JFL and WYD devised the project and conceptual ideas. Technical details were completed by WYD, YY and HB. WYD performed the computational works. WYD and BC analyzed computation results. The paper writing was completed by WYD, YY and BC. All authors approved of this manuscript.
Corresponding authors
Rights and permissions
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
About this article
Cite this article
Dai, WY., Yu, Y., Cheng, B. et al. Analytical formulation for gravitation modeling of mass-heterogeneous bodies. J Geod 96, 100 (2022). https://doi.org/10.1007/s00190-022-01684-z
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s00190-022-01684-z