Escape of asteroids from the main belt

被引:87
|
作者
Granvik, Mikael [1 ]
Morbidelli, Alessandro [2 ]
Vokrouhlicky, David [3 ]
Bottke, William F. [4 ]
Nesvorny, David [4 ]
Jedicke, Robert [5 ]
机构
[1] Univ Helsinki, Dept Phys, POB 64, FIN-00014 Helsinki, Finland
[2] Observ Cote Azur, Blvd Observ, F-06304 Nice 4, France
[3] Charles Univ Prague, Inst Astron, V Holesovickach 2, CR-18000 Prague 8, Czech Republic
[4] Southwest Res Inst, 1050 Walnut St,Ste 300, Boulder, CO 80302 USA
[5] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
基金
芬兰科学院;
关键词
minor planets; asteroids:; general; methods: numerical; methods: statistical; surveys; celestial mechanics; planets and satellites: dynamical evolution and stability; SECULAR SPIN DYNAMICS; PROPER ELEMENTS; YARKOVSKY; ORIGIN; BEHAVIOR; MOTION; INTEGRATOR; EVOLUTION; OBJECTS; SEARCH;
D O I
10.1051/0004-6361/201629252
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We locate escape routes from the main asteroid belt, particularly into the near-Earth-object (NEO) region, and estimate the relative fluxes for different escape routes as a function of object size under the influence of the Yarkovsky semimajor-axis drift. Methods. We integrated the orbits of 78 355 known and 14 094 cloned main-belt objects and Cybele and Hilda asteroids (hereafter collectively called MBOs) for 100 Myr and recorded the characteristics of the escaping objects. The selected sample of MBOs with perihelion distance q > 1.3 au and semimajor axis a < 4.1 au is essentially complete, with an absolute magnitude limit ranging from H-V < 15. 9 in the inner belt (a < 2.5 au) to HV < 14.4 in the outer belt (2.5 au < a < 4.1 au). We modeled the semimajor- axis drift caused by the Yarkovsky force and assigned four different sizes ( diameters of 0.1, 0.3, 1.0, and 3.0 km) and random spin obliquities (either 0 deg or 180 deg) for each test asteroid. Results. We find more than ten obvious escape routes from the asteroid belt to the NEO region, and they typically coincide with low-order mean-motion resonances with Jupiter and secular resonances. The locations of the escape routes are independent of the semimajor-axis drift rate and thus are also independent of the asteroid diameter. The locations of the escape routes are likewise unaffected when we added a model for Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) cycles coupled with secular evolution of the rotation pole as a result of the solar gravitational torque. A Yarkovsky- only model predicts a flux of asteroids entering the NEO region that is too high compared to the observationally constrained flux, and the discrepancy grows larger for smaller asteroids. A combined Yarkovsky and YORP model predicts a flux of small NEOs that is approximately a factor of 5 too low compared to an observationally constrained estimate. This suggests that the characteristic timescale of the YORP cycle is longer than our canonical YORP model predicts.
引用
收藏
页数:13
相关论文
共 50 条
  • [1] Inner main belt asteroids in Slivan states?
    Vrastil, J.
    Vokrouhlicky, D.
    ASTRONOMY & ASTROPHYSICS, 2015, 579
  • [2] Prediction for close approaches with terrestrial planets of asteroids from the main belt
    Zhou, Yufan Fane
    Li, Zhiyuan
    Li, Hailiang
    Zhou, Liyong
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2025, 538 (01) : 258 - 265
  • [3] Stability time-scale prediction for main-belt asteroids using neural networks
    Liu, Chao
    Gong, Shengping
    Li, Junfeng
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 502 (04) : 5362 - 5369
  • [4] Research of the family associations of active asteroids in the main belt
    Xin, Yingqi
    Shi, Jianchun
    Ma, Yuehua
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 527 (04) : 10309 - 10334
  • [5] Ancient and primordial collisional families as the main sources of X-type asteroids of the inner main belt
    Delbo, Marco
    Avdelhdou, Chrysa
    Morbidelh, Alessandro
    ASTRONOMY & ASTROPHYSICS, 2019, 624
  • [6] Polarimetric survey of main-belt asteroids
    Gil-Hutton, R.
    Garcia-Migani, E.
    ASTRONOMY & ASTROPHYSICS, 2017, 607
  • [7] A photometric search for active Main Belt asteroids
    Cikota, S.
    Ortiz, J. L.
    Cikota, A.
    Morales, N.
    Tancredi, G.
    ASTRONOMY & ASTROPHYSICS, 2014, 562
  • [8] Main belt asteroids taxonomical information from dark energy survey data
    Carruba, V.
    Camargo, J. I. B.
    Aljbaae, S.
    Ferreira, F. S.
    Lin, E.
    Figueiredo-Peixoto, V.
    Banda-Huarca, M. V.
    Pieres, A.
    Boufleur, R. C.
    da Costa, L. N.
    Abbott, T. M. C.
    Aguena, M.
    Allam, Sahar S.
    Alves, O.
    Bernardinelli, P. H.
    Bertin, E.
    Brooks, D.
    Rosell, A. Carnero
    Carretero, J.
    Pereira, M. E. S.
    Davis, T. M.
    De Vicente, J.
    Desai, S.
    Doel, P.
    Ferrero, I.
    Friedel, D.
    Frieman, J.
    Garcia-Bellido, J.
    Gatti, M.
    Giannini, G.
    Gruen, D.
    Gruendl, R. A.
    Herner, K.
    Hinton, S. R.
    Hollowood, D. L.
    James, D. J.
    Kent, S.
    Kuehn, K.
    Lahav, O.
    Marshall, J. L.
    Mena-Fernandez, J.
    Miquel, R.
    Palmese, A.
    Malagon, A. A. Plazas
    Rodriguez-Monroy, M.
    Sanchez, E.
    Santiago, B.
    Schubnell, M.
    Smith, M.
    Suchyta, E.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 527 (03) : 6495 - 6505
  • [9] Possible origin of Mars-crossing asteroids and related dynamical properties of inner main-belt asteroids
    Liu, Shanhong
    Wang, Xin
    Han, Yilong
    Hou, Xiyun
    Yan, Jianguo
    Cao, Jianfeng
    Gao, Jian
    Li, Xie
    ASTRONOMY & ASTROPHYSICS, 2024, 692
  • [10] Thermal properties of large main-belt asteroids observed by Herschel PACS
    Ali-Lagoa, V
    Mueller, T. G.
    Kiss, C.
    Szakats, R.
    Marton, G.
    Farkas-Takacs, A.
    Bartczak, P.
    Butkiewicz-Bak, M.
    Dudzinski, G.
    Marciniak, A.
    Podlewska-Gaca, E.
    Duffard, R.
    Santos-Sanz, P.
    Ortiz, J. L.
    ASTRONOMY & ASTROPHYSICS, 2020, 638