Academia Sinica Institute of Astronomy & Astrophysics
中央研究院天文及天文物理研究所
Go Back
Research Gallery > Planetary Sciences

Research Gallery

Planetary Sciences

Contribution of several MMRs populations to the production of JFCs
Image Credit: M. A. Muñoz-Gutiérrez
Contribution of several MMRs populations to the production of JFCs
The number of new visible Jupiter Family Comets (JFCs) produced by each mean motion resonance (MMR) with Neptune, in our numerical simulations including the 34 largest dwarf planets (DPs, red line) or only the giant planets (black line).
Also shown in the Figure are the numbers of JFCs produced in two long-term (1 Gyr) simulations of the 3:2 population: including Pluto as a massive object along with the giant planets (orange line) and including the four massive Plutinos named in the Figure (green line).
Page Top
TEL: 886-2-3365-2200 FAX: 886-2-2367-7849
General: asiaa_replace2@_asiaa.sinica.edu.tw Media Request: epo_replace2@_asiaa.sinica.edu.tw
11F of AS/NTU Astronomy-Mathematics Building, No.1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan, R.O.C.