Accretion in the Edgeworth-Kuiper Belt: Forming 100-1000 KM Radius Bodies at 30 AU and Beyond.

Details Accretion in the Edgeworth-Kuiper Belt: Forming 100-1000 KM Radius Bodies at 30 AU and Beyond. Accretion in the Edgeworth-Kuiper Belt: Forming 100-1000 KM Radius Bodies at 30 AU and Beyond.

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aj....114..841s&link_type=abstract

The Astronomical Journal, v. 114, p. 841.

Astronomy and Astrophysics

Astronomy

85

Accretion, Interplanetary Medium, Minor Planets

Scientific paper

We employ a time-dependent collisional evolution code to study the conditions under which the ≍50-200km radius Edgeworth-Kuiper Objects (EKOs) in the region between 30 and 50 AU [now called the Edgeworth-Kuiper Belt, or EKB; Edgeworth, K. E. 1943, JBAA, 53, 181; Edgeworth, K. E. 1949, MNRAS, 109, 600; Kuiper, G. P. 1951, Astrophysics: A Topical Symposium (McGraw-Hill, New York)] were formed. Assuming that these bodies were created by pairwise accretion beginning with 1 to 10 km building blocks, we find that three conditions were required, namely, (i) at least 10Msun and more likely 35 Msunof solids in the primordial 30-50 AU zone, (ii) mean random orbital eccentricities of order 0.002 or smaller, and (iii) mechanically strong building blocks. Furthermore, we find that the accretion of 100-200 km radius bodies in the 30-50 AU region from collisions among a starting population of 1-10 km building blocks required ≍108-109 yr, with the lower range only being reached for 30-50 AU zone masses approaching of solids or mean random orbital eccentricities <0.005 (which may not be realistic after gas dissipation). Therefore, unless accretion had already produced many building blocks significantly larger than 10 km in diameter at the time the nebular gas was removed, our results indicate that Neptune did not form on a time scale much shorter than ˜70 Myr, and could well have required many hundreds of Myr to approach its final mass. We also explore the growth of Pluto-scale (i.e., radius 1000-1200 km) objects in the 30-50 AU region under a variety of assumptions. We further find that once ˜300 hundred kilometer radius objects were formed, the growth of 1000 km radius and larger objects occurs relatively easily and comparatively quickly. The lack of many Plutos in the 30-50 AU zone therefore argues strongly that growth was terminated in that region rather abruptly at the time the presently observed population of 100-200 km radius EKOs were being completed. In the region beyond 50 AU where Neptune's dynamical influence was much reduced, model runs yield 100-1000 km radius, and perhaps even larger bodies which should be detectable with on-going or soon-to-be started surveys. We suggest that if dynamical conditions did not remain calm enough to allow Pluto itself to be grown in the 30-50 AU zone before perturbations from Neptune created a dynamically erosive, low-mass environment there, then it may be that Pluto was grown beyond the influence of Neptune's perturbations and later transported inward, perhaps in part via the Charon-forming collision.

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