activity
20182025
most citedGrowth Model Interpretation of Planet Size Distribution

591 citations · 643 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

8 papers · 1 filter

astro-ph.EP2025★ 1 cited

Planetesimal Impact Vapor Plumes and Nebular Shocks form Chondritic Mixtures

Sarah T. Stewart, Simon J. Lock, Philip J. Carter +3

The origin of chondrules, and the chondritic sedimentary rocks that dominate the meteoritic record, is a long-standing problem in planetary science. Here, we develop a physical mod…

astro-ph.EP2022

EOS Manual

Li Zeng, Stein B. Jacobsen, Dimitar D. Sasselov +1

The exoplanet field now abounds with new discoveries of planets and planetary systems. It is of great interest for the scientific community to understand the compositions and inter…

astro-ph.EP2022★ 11 cited

Maximum Temperatures in Evolving Protoplanetary Discs and Composition of Planetary Building Blocks

Min Li, Shichun Huang, Zhaohuan Zhu +2

The maximum temperature and radial temperature profile in a protoplanetary disc are important for the condensation of different elements in the disc. We simulate the evolution of a…

astro-ph.EP2022★ 40 cited

New Perspectives on the Exoplanet Radius Gap from a Mathematica Tool and Visualized Water Equation of State

Li Zeng, Stein B. Jacobsen, Eugenia Hyung +12

Recent astronomical observations obtained with the Kepler and TESS missions and their related ground-based follow-ups revealed an abundance of exoplanets with a size intermediate b…

astro-ph.EP2019★ 591 cited

Growth Model Interpretation of Planet Size Distribution

Li Zeng, Stein B. Jacobsen, Dimitar D. Sasselov +13

The radii and orbital periods of 4000+ confirmed/candidate exoplanets have been precisely measured by the Kepler mission. The radii show a bimodal distribution, with two peaks corr…

astro-ph.EP2019

Dust Condensation in Evolving Discs and the Composition of Planetary Building Blocks

Min Li, Shichun Huang, Michail I. Petaev +2

Partial condensation of dust from the Solar nebula is likely responsible for the diverse chemical compositions of chondrites and rocky planets/planetesimals in the inner Solar syst…